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href="/search/?searchtype=author&query=Wang%2C+E&start=150" class="pagination-link " aria-label="Page 4" aria-current="page">4 </a> </li> <li> <a href="/search/?searchtype=author&query=Wang%2C+E&start=200" class="pagination-link " aria-label="Page 5" aria-current="page">5 </a> </li> <li><span class="pagination-ellipsis">…</span></li> </ul> </nav> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2502.12659">arXiv:2502.12659</a> <span> [<a href="https://arxiv.org/pdf/2502.12659">pdf</a>, <a href="https://arxiv.org/format/2502.12659">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Computers and Society">cs.CY</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> </div> </div> <p class="title is-5 mathjax"> The Hidden Risks of Large Reasoning Models: A Safety Assessment of R1 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Zhou%2C+K">Kaiwen Zhou</a>, <a href="/search/?searchtype=author&query=Liu%2C+C">Chengzhi Liu</a>, <a href="/search/?searchtype=author&query=Zhao%2C+X">Xuandong Zhao</a>, <a href="/search/?searchtype=author&query=Jangam%2C+S">Shreedhar Jangam</a>, <a href="/search/?searchtype=author&query=Srinivasa%2C+J">Jayanth Srinivasa</a>, <a href="/search/?searchtype=author&query=Liu%2C+G">Gaowen Liu</a>, <a href="/search/?searchtype=author&query=Song%2C+D">Dawn Song</a>, <a href="/search/?searchtype=author&query=Wang%2C+X+E">Xin Eric Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2502.12659v1-abstract-short" style="display: inline;"> The rapid development of large reasoning models, such as OpenAI-o3 and DeepSeek-R1, has led to significant improvements in complex reasoning over non-reasoning large language models~(LLMs). However, their enhanced capabilities, combined with the open-source access of models like DeepSeek-R1, raise serious safety concerns, particularly regarding their potential for misuse. In this work, we present… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.12659v1-abstract-full').style.display = 'inline'; document.getElementById('2502.12659v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2502.12659v1-abstract-full" style="display: none;"> The rapid development of large reasoning models, such as OpenAI-o3 and DeepSeek-R1, has led to significant improvements in complex reasoning over non-reasoning large language models~(LLMs). However, their enhanced capabilities, combined with the open-source access of models like DeepSeek-R1, raise serious safety concerns, particularly regarding their potential for misuse. In this work, we present a comprehensive safety assessment of these reasoning models, leveraging established safety benchmarks to evaluate their compliance with safety regulations. Furthermore, we investigate their susceptibility to adversarial attacks, such as jailbreaking and prompt injection, to assess their robustness in real-world applications. Through our multi-faceted analysis, we uncover four key findings: (1) There is a significant safety gap between the open-source R1 models and the o3-mini model, on both safety benchmark and attack, suggesting more safety effort on R1 is needed. (2) The distilled reasoning model shows poorer safety performance compared to its safety-aligned base models. (3) The stronger the model's reasoning ability, the greater the potential harm it may cause when answering unsafe questions. (4) The thinking process in R1 models pose greater safety concerns than their final answers. Our study provides insights into the security implications of reasoning models and highlights the need for further advancements in R1 models' safety to close the gap. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.12659v1-abstract-full').style.display = 'none'; document.getElementById('2502.12659v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2025. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2502.12409">arXiv:2502.12409</a> <span> [<a href="https://arxiv.org/pdf/2502.12409">pdf</a>, <a href="https://arxiv.org/format/2502.12409">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Astrophysics of Galaxies">astro-ph.GA</span> </div> </div> <p class="title is-5 mathjax"> Dominant Role of Coplanar Inflows in Driving Disk Evolution Revealed by Gas-Phase Metallicity Gradients </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Lyu%2C+C">Cheqiu Lyu</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Enci Wang</a>, <a href="/search/?searchtype=author&query=Zhang%2C+H">Hongxin Zhang</a>, <a href="/search/?searchtype=author&query=Peng%2C+Y">Yingjie Peng</a>, <a href="/search/?searchtype=author&query=Wang%2C+X">Xin Wang</a>, <a href="/search/?searchtype=author&query=Li%2C+H">Haixin Li</a>, <a href="/search/?searchtype=author&query=Ma%2C+C">Chengyu Ma</a>, <a href="/search/?searchtype=author&query=Yu%2C+H">Haoran Yu</a>, <a href="/search/?searchtype=author&query=Chen%2C+Z">Zeyu Chen</a>, <a href="/search/?searchtype=author&query=Jia%2C+C">Cheng Jia</a>, <a href="/search/?searchtype=author&query=Kong%2C+X">Xu Kong</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2502.12409v1-abstract-short" style="display: inline;"> Using spatially resolved spectroscopic data from the MaNGA sample, we investigate the parameters influencing the radial gradients of gas-phase metallicity ($\nabla\log(\mathrm{O/H})$), to determine whether disk formation is primarily driven by coplanar gas inflow or by the independent evolution of distinct regions within the disk. Our results show that $\nabla \log(\mathrm{O/H})$ strongly correlat… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.12409v1-abstract-full').style.display = 'inline'; document.getElementById('2502.12409v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2502.12409v1-abstract-full" style="display: none;"> Using spatially resolved spectroscopic data from the MaNGA sample, we investigate the parameters influencing the radial gradients of gas-phase metallicity ($\nabla\log(\mathrm{O/H})$), to determine whether disk formation is primarily driven by coplanar gas inflow or by the independent evolution of distinct regions within the disk. Our results show that $\nabla \log(\mathrm{O/H})$ strongly correlates with local gas-phase metallicity at a given stellar mass, with steeper gradients observed in metal-poorer disks. This trend supports the coplanar gas inflow scenario, wherein the gas is progressively enriched by in situ star formation as it flows inward. In contrast, the radial gradient of stellar mass surface density shows very weak correlations with $\nabla \log(\mathrm{O/H})$, which is inconsistent with the independent evolution mode, where gas inflow, star formation, and metal enrichment occur independently within each annulus of the disk. Furthermore, we find that $\nabla \log(\mathrm{O/H})$ is also closely correlated with an indicator of local gas turbulence $蟽_{\mathrm{gas}}/R_{\mathrm{e}}$, highlighting the competing roles of turbulence and coplanar inflow in shaping metallicity gradients. Our results provide indirect observational evidence supporting coplanar gas inflow as the driving mechanism for disk evolution. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.12409v1-abstract-full').style.display = 'none'; document.getElementById('2502.12409v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 17 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2025. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">16 pages, 5+4 figures. Accepted by ApJL</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2502.06982">arXiv:2502.06982</a> <span> [<a href="https://arxiv.org/pdf/2502.06982">pdf</a>, <a href="https://arxiv.org/format/2502.06982">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Machine Learning">cs.LG</span> </div> </div> <p class="title is-5 mathjax"> Machine Learning Fleet Efficiency: Analyzing and Optimizing Large-Scale Google TPU Systems with ML Productivity Goodput </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Wongpanich%2C+A">Arissa Wongpanich</a>, <a href="/search/?searchtype=author&query=Oguntebi%2C+T">Tayo Oguntebi</a>, <a href="/search/?searchtype=author&query=Paredes%2C+J+B">Jose Baiocchi Paredes</a>, <a href="/search/?searchtype=author&query=Wang%2C+Y+E">Yu Emma Wang</a>, <a href="/search/?searchtype=author&query=Phothilimthana%2C+P+M">Phitchaya Mangpo Phothilimthana</a>, <a href="/search/?searchtype=author&query=Mitra%2C+R">Ritwika Mitra</a>, <a href="/search/?searchtype=author&query=Zhou%2C+Z">Zongwei Zhou</a>, <a href="/search/?searchtype=author&query=Kumar%2C+N">Naveen Kumar</a>, <a href="/search/?searchtype=author&query=Reddi%2C+V+J">Vijay Janapa Reddi</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2502.06982v1-abstract-short" style="display: inline;"> Recent years have seen the emergence of machine learning (ML) workloads deployed in warehouse-scale computing (WSC) settings, also known as ML fleets. As the computational demands placed on ML fleets have increased due to the rise of large models and growing demand for ML applications, it has become increasingly critical to measure and improve the efficiency of such systems. However, there is not… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.06982v1-abstract-full').style.display = 'inline'; document.getElementById('2502.06982v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2502.06982v1-abstract-full" style="display: none;"> Recent years have seen the emergence of machine learning (ML) workloads deployed in warehouse-scale computing (WSC) settings, also known as ML fleets. As the computational demands placed on ML fleets have increased due to the rise of large models and growing demand for ML applications, it has become increasingly critical to measure and improve the efficiency of such systems. However, there is not yet an established methodology to characterize ML fleet performance and identify potential performance optimizations accordingly. This paper presents a large-scale analysis of an ML fleet based on Google's TPUs, introducing a framework to capture fleet-wide efficiency, systematically evaluate performance characteristics, and identify optimization strategies for the fleet. We begin by defining an ML fleet, outlining its components, and analyzing an example Google ML fleet in production comprising thousands of accelerators running diverse workloads. Our study reveals several critical insights: first, ML fleets extend beyond the hardware layer, with model, data, framework, compiler, and scheduling layers significantly impacting performance; second, the heterogeneous nature of ML fleets poses challenges in characterizing individual workload performance; and third, traditional utilization-based metrics prove insufficient for ML fleet characterization. To address these challenges, we present the "ML Productivity Goodput" (MPG) metric to measure ML fleet efficiency. We show how to leverage this metric to characterize the fleet across the ML system stack. We also present methods to identify and optimize performance bottlenecks using MPG, providing strategies for managing warehouse-scale ML systems in general. Lastly, we demonstrate quantitative evaluations from applying these methods to a real ML fleet for internal-facing Google TPU workloads, where we observed tangible improvements. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.06982v1-abstract-full').style.display = 'none'; document.getElementById('2502.06982v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2025. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2502.04488">arXiv:2502.04488</a> <span> [<a href="https://arxiv.org/pdf/2502.04488">pdf</a>, <a href="https://arxiv.org/format/2502.04488">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> </div> </div> <p class="title is-5 mathjax"> Building A Unified AI-centric Language System: analysis, framework and future work </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Wang%2C+E+H">Edward Hong Wang</a>, <a href="/search/?searchtype=author&query=Wen%2C+C+X">Cynthia Xin Wen</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2502.04488v1-abstract-short" style="display: inline;"> Recent advancements in large language models have demonstrated that extended inference through techniques can markedly improve performance, yet these gains come with increased computational costs and the propagation of inherent biases found in natural languages. This paper explores the design of a unified AI-centric language system that addresses these challenges by offering a more concise, unambi… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.04488v1-abstract-full').style.display = 'inline'; document.getElementById('2502.04488v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2502.04488v1-abstract-full" style="display: none;"> Recent advancements in large language models have demonstrated that extended inference through techniques can markedly improve performance, yet these gains come with increased computational costs and the propagation of inherent biases found in natural languages. This paper explores the design of a unified AI-centric language system that addresses these challenges by offering a more concise, unambiguous, and computationally efficient alternative to traditional human languages. We analyze the limitations of natural language such as gender bias, morphological irregularities, and contextual ambiguities and examine how these issues are exacerbated within current Transformer architectures, where redundant attention heads and token inefficiencies prevail. Drawing on insights from emergent artificial communication systems and constructed languages like Esperanto and Lojban, we propose a framework that translates diverse natural language inputs into a streamlined AI-friendly language, enabling more efficient model training and inference while reducing memory footprints. Finally, we outline a pathway for empirical validation through controlled experiments, paving the way for a universal interchange format that could revolutionize AI-to-AI and human-to-AI interactions by enhancing clarity, fairness, and overall performance. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.04488v1-abstract-full').style.display = 'none'; document.getElementById('2502.04488v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2025. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2502.04136">arXiv:2502.04136</a> <span> [<a href="https://arxiv.org/pdf/2502.04136">pdf</a>, <a href="https://arxiv.org/ps/2502.04136">ps</a>, <a href="https://arxiv.org/format/2502.04136">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Combinatorics">math.CO</span> </div> </div> <p class="title is-5 mathjax"> $r$-Enriched Permutations and an Inequality of B贸na-McLennan-White </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Chen%2C+W+Y+C">William Y. C. Chen</a>, <a href="/search/?searchtype=author&query=Wang%2C+E+L">Elena L. Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2502.04136v1-abstract-short" style="display: inline;"> This paper is concerned with a duality between $r$-regular permutations and $r$-cycle permutations, and a monotone property due to B贸na-McLennan-White on the probability $p_r(n)$ for a random permutation of $\{1,2,\ldots, n\}$ to have an $r$-th root, where $r$ is a prime. For $r=2$, the duality relates permutations with odd cycles to permutations with even cycles. In general, given $r\geq 2$, we… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.04136v1-abstract-full').style.display = 'inline'; document.getElementById('2502.04136v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2502.04136v1-abstract-full" style="display: none;"> This paper is concerned with a duality between $r$-regular permutations and $r$-cycle permutations, and a monotone property due to B贸na-McLennan-White on the probability $p_r(n)$ for a random permutation of $\{1,2,\ldots, n\}$ to have an $r$-th root, where $r$ is a prime. For $r=2$, the duality relates permutations with odd cycles to permutations with even cycles. In general, given $r\geq 2$, we define an $r$-enriched permutation to be a permutation with $r$-singular cycles colored by one of the colors $1, 2, \ldots, r-1 $. In this setup, we discover a duality between $r$-regular permutations and enriched $r$-cycle permutations, which yields a stronger version of an inequality of B贸na-McLennan-White. This answers their question of seeking a fully combinatorial understanding of the monotone property. When $r$ is a prime power $q^l$, we further show that $p_r(n)$ is monotone without using generating functions. In the case $n+1 \not\equiv 0 \pmod q$, the equality $p_r(n)=p_r(n+1)$ has been established by Chernoff. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.04136v1-abstract-full').style.display = 'none'; document.getElementById('2502.04136v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2025. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">24 pages</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">MSC Class:</span> 05A05; 05A19; 05A20 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2502.02201">arXiv:2502.02201</a> <span> [<a href="https://arxiv.org/pdf/2502.02201">pdf</a>, <a href="https://arxiv.org/format/2502.02201">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Human-Computer Interaction">cs.HC</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Emerging Technologies">cs.ET</span> </div> </div> <p class="title is-5 mathjax"> Can You Move These Over There? An LLM-based VR Mover for Supporting Object Manipulation </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Wang%2C+X+E">Xiangzhi Eric Wang</a>, <a href="/search/?searchtype=author&query=Sin%2C+Z+P+T">Zackary P. T. Sin</a>, <a href="/search/?searchtype=author&query=Jia%2C+Y">Ye Jia</a>, <a href="/search/?searchtype=author&query=Archer%2C+D">Daniel Archer</a>, <a href="/search/?searchtype=author&query=Fong%2C+W+H+Y">Wynonna H. Y. Fong</a>, <a href="/search/?searchtype=author&query=Li%2C+Q">Qing Li</a>, <a href="/search/?searchtype=author&query=Li%2C+C">Chen Li</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2502.02201v1-abstract-short" style="display: inline;"> In our daily lives, we can naturally convey instructions for the spatial manipulation of objects using words and gestures. Transposing this form of interaction into virtual reality (VR) object manipulation can be beneficial. We propose VR Mover, an LLM-empowered solution that can understand and interpret the user's vocal instruction to support object manipulation. By simply pointing and speaking,… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.02201v1-abstract-full').style.display = 'inline'; document.getElementById('2502.02201v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2502.02201v1-abstract-full" style="display: none;"> In our daily lives, we can naturally convey instructions for the spatial manipulation of objects using words and gestures. Transposing this form of interaction into virtual reality (VR) object manipulation can be beneficial. We propose VR Mover, an LLM-empowered solution that can understand and interpret the user's vocal instruction to support object manipulation. By simply pointing and speaking, the LLM can manipulate objects without structured input. Our user study demonstrates that VR Mover enhances user usability, overall experience and performance on multi-object manipulation, while also reducing workload and arm fatigue. Users prefer the proposed natural interface for broad movements and may complementarily switch to gizmos or virtual hands for finer adjustments. These findings are believed to contribute to design implications for future LLM-based object manipulation interfaces, highlighting the potential for more intuitive and efficient user interactions in VR environments. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2502.02201v1-abstract-full').style.display = 'none'; document.getElementById('2502.02201v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 4 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2025. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">64 pages (30 in main text), 22 figures (19 in main text)</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.16672">arXiv:2501.16672</a> <span> [<a href="https://arxiv.org/pdf/2501.16672">pdf</a>, <a href="https://arxiv.org/format/2501.16672">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Information Retrieval">cs.IR</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Logic in Computer Science">cs.LO</span> </div> </div> <p class="title is-5 mathjax"> VeriFact: Verifying Facts in LLM-Generated Clinical Text with Electronic Health Records </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Chung%2C+P">Philip Chung</a>, <a href="/search/?searchtype=author&query=Swaminathan%2C+A">Akshay Swaminathan</a>, <a href="/search/?searchtype=author&query=Goodell%2C+A+J">Alex J. Goodell</a>, <a href="/search/?searchtype=author&query=Kim%2C+Y">Yeasul Kim</a>, <a href="/search/?searchtype=author&query=Reincke%2C+S+M">S. Momsen Reincke</a>, <a href="/search/?searchtype=author&query=Han%2C+L">Lichy Han</a>, <a href="/search/?searchtype=author&query=Deverett%2C+B">Ben Deverett</a>, <a href="/search/?searchtype=author&query=Sadeghi%2C+M+A">Mohammad Amin Sadeghi</a>, <a href="/search/?searchtype=author&query=Ariss%2C+A">Abdel-Badih Ariss</a>, <a href="/search/?searchtype=author&query=Ghanem%2C+M">Marc Ghanem</a>, <a href="/search/?searchtype=author&query=Seong%2C+D">David Seong</a>, <a href="/search/?searchtype=author&query=Lee%2C+A+A">Andrew A. Lee</a>, <a href="/search/?searchtype=author&query=Coombes%2C+C+E">Caitlin E. Coombes</a>, <a href="/search/?searchtype=author&query=Bradshaw%2C+B">Brad Bradshaw</a>, <a href="/search/?searchtype=author&query=Sufian%2C+M+A">Mahir A. Sufian</a>, <a href="/search/?searchtype=author&query=Hong%2C+H+J">Hyo Jung Hong</a>, <a href="/search/?searchtype=author&query=Nguyen%2C+T+P">Teresa P. Nguyen</a>, <a href="/search/?searchtype=author&query=Rasouli%2C+M+R">Mohammad R. Rasouli</a>, <a href="/search/?searchtype=author&query=Kamra%2C+K">Komal Kamra</a>, <a href="/search/?searchtype=author&query=Burbridge%2C+M+A">Mark A. Burbridge</a>, <a href="/search/?searchtype=author&query=McAvoy%2C+J+C">James C. McAvoy</a>, <a href="/search/?searchtype=author&query=Saffary%2C+R">Roya Saffary</a>, <a href="/search/?searchtype=author&query=Ma%2C+S+P">Stephen P. Ma</a>, <a href="/search/?searchtype=author&query=Dash%2C+D">Dev Dash</a>, <a href="/search/?searchtype=author&query=Xie%2C+J">James Xie</a> , et al. (4 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.16672v1-abstract-short" style="display: inline;"> Methods to ensure factual accuracy of text generated by large language models (LLM) in clinical medicine are lacking. VeriFact is an artificial intelligence system that combines retrieval-augmented generation and LLM-as-a-Judge to verify whether LLM-generated text is factually supported by a patient's medical history based on their electronic health record (EHR). To evaluate this system, we introd… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.16672v1-abstract-full').style.display = 'inline'; document.getElementById('2501.16672v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.16672v1-abstract-full" style="display: none;"> Methods to ensure factual accuracy of text generated by large language models (LLM) in clinical medicine are lacking. VeriFact is an artificial intelligence system that combines retrieval-augmented generation and LLM-as-a-Judge to verify whether LLM-generated text is factually supported by a patient's medical history based on their electronic health record (EHR). To evaluate this system, we introduce VeriFact-BHC, a new dataset that decomposes Brief Hospital Course narratives from discharge summaries into a set of simple statements with clinician annotations for whether each statement is supported by the patient's EHR clinical notes. Whereas highest agreement between clinicians was 88.5%, VeriFact achieves up to 92.7% agreement when compared to a denoised and adjudicated average human clinican ground truth, suggesting that VeriFact exceeds the average clinician's ability to fact-check text against a patient's medical record. VeriFact may accelerate the development of LLM-based EHR applications by removing current evaluation bottlenecks. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.16672v1-abstract-full').style.display = 'none'; document.getElementById('2501.16672v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 27 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">62 pages, 5 figures, 1 table, pre-print manuscript</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.15153">arXiv:2501.15153</a> <span> [<a href="https://arxiv.org/pdf/2501.15153">pdf</a>, <a href="https://arxiv.org/format/2501.15153">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> </div> <p class="title is-5 mathjax"> Roles of $螖(1232)$, $N^*(1520)$, and $N^*(1650)$ resonances in $纬p\to 蟺^0 蟺^0 p$ reaction within an effective Lagrangian approach </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Dai%2C+M">Meng-Yuan Dai</a>, <a href="/search/?searchtype=author&query=Liu%2C+S">Si-Wei Liu</a>, <a href="/search/?searchtype=author&query=Chen%2C+C">Cheng Chen</a>, <a href="/search/?searchtype=author&query=Li%2C+D">De-Min Li</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">En Wang</a>, <a href="/search/?searchtype=author&query=Xie%2C+J">Ju-Jun Xie</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.15153v1-abstract-short" style="display: inline;"> Roles of the $螖(1232)$, ${N}^{*}(1520)$, and ${N}^{*}(1650)$ resonances in the $纬p\to{蟺}^{0}{蟺}^{0}p $ reaction near threshold is investigated within an effective Lagrangian approach. We have calculated the differential cross sections of the $纬p\to{蟺}^{0}{蟺}^{0}p$ reaction by including the contributions from the $螖(1232)$, ${N}^{*}(1520)$, and ${N}^{*}(1650)$ intermediate states decaying into… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.15153v1-abstract-full').style.display = 'inline'; document.getElementById('2501.15153v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.15153v1-abstract-full" style="display: none;"> Roles of the $螖(1232)$, ${N}^{*}(1520)$, and ${N}^{*}(1650)$ resonances in the $纬p\to{蟺}^{0}{蟺}^{0}p $ reaction near threshold is investigated within an effective Lagrangian approach. We have calculated the differential cross sections of the $纬p\to{蟺}^{0}{蟺}^{0}p$ reaction by including the contributions from the $螖(1232)$, ${N}^{*}(1520)$, and ${N}^{*}(1650)$ intermediate states decaying into $蟺^0 p$ via the $s$-channel nucleon pole and $t$-channel $蟻$ exchange, and found that the current experimental measurements can be well reproduced. The production of $螖(1232)$ is mainly from the mechanism of the $s$-channel nucleon pole, while the ${N}^{*}(1520)$ and ${N}^{*}(1650)$ are produced from the mechanism of the $t$-channel $蟻$ exchange. It is expected that more experimental data on the $纬p \to 蟺^0 蟺^0 p$ reaction can be used to explore the properties of the low-lying excited baryon states and also the scalar $f_0(500)$ and $f_0(980)$ mesons. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.15153v1-abstract-full').style.display = 'none'; document.getElementById('2501.15153v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 25 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">9 pages, 5 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.14385">arXiv:2501.14385</a> <span> [<a href="https://arxiv.org/pdf/2501.14385">pdf</a>, <a href="https://arxiv.org/format/2501.14385">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> Study $螢_c^+ \to 螞{\bar{K}}^0 蟺^+$ and search for the low-lying baryons $螢(1/2^-)$ and $危(1/2^-)$ </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Li%2C+Y">Ying Li</a>, <a href="/search/?searchtype=author&query=Lyu%2C+W">Wen-Tao Lyu</a>, <a href="/search/?searchtype=author&query=Wang%2C+G">Guan-Ying Wang</a>, <a href="/search/?searchtype=author&query=Li%2C+L">Longke Li</a>, <a href="/search/?searchtype=author&query=Yan%2C+W">Wen-Cheng Yan</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">En Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.14385v1-abstract-short" style="display: inline;"> Since searches for the low-lying excited baryons $螢(1/2^-)$ and $危(1/2^-)$ are crucial to deepening our understanding of the light baryon spectrum, we have investigated the Cabibbo-favored process $螢_c^+ \to 螞{\bar{K}}^0 蟺^+$ by taking into account the $S$-wave pseudoscalar meson-octet baryon interactions within the chiral unitary approach, which could dynamically generate the resonances… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.14385v1-abstract-full').style.display = 'inline'; document.getElementById('2501.14385v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.14385v1-abstract-full" style="display: none;"> Since searches for the low-lying excited baryons $螢(1/2^-)$ and $危(1/2^-)$ are crucial to deepening our understanding of the light baryon spectrum, we have investigated the Cabibbo-favored process $螢_c^+ \to 螞{\bar{K}}^0 蟺^+$ by taking into account the $S$-wave pseudoscalar meson-octet baryon interactions within the chiral unitary approach, which could dynamically generate the resonances $螢(1/2^-)$ and $危(1/2^-)$. The contributions from the excited kaons are double Cabibbo-suppressed, and the contribution from the $危(1385)$ is also suppressed due to Korner-Pati-Woo theory, thus those states are expected to play negligible contributions in this process. We have predicted the $\bar{K}^0 螞$ and $蟺^+螞$ invariant mass distributions, which have the clear signals of the $螢(1/2^-)$ and $危(1/2^-)$. Thus, the $螢_c^+ \to 螞{\bar{K}}^0 蟺^+$ is an ideal process to search for the low-lying baryons $螢(1/2^-)$ and $危(1/2^-)$, and we make a call for a precise measurements of this process in experiments, such as Belle II, LHCb, and the proposed Super Tau-Charm Facility (STCF). <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.14385v1-abstract-full').style.display = 'none'; document.getElementById('2501.14385v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 24 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">8 pages, 9 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.14249">arXiv:2501.14249</a> <span> [<a href="https://arxiv.org/pdf/2501.14249">pdf</a>, <a href="https://arxiv.org/format/2501.14249">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Machine Learning">cs.LG</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> </div> </div> <p class="title is-5 mathjax"> Humanity's Last Exam </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Phan%2C+L">Long Phan</a>, <a href="/search/?searchtype=author&query=Gatti%2C+A">Alice Gatti</a>, <a href="/search/?searchtype=author&query=Han%2C+Z">Ziwen Han</a>, <a href="/search/?searchtype=author&query=Li%2C+N">Nathaniel Li</a>, <a href="/search/?searchtype=author&query=Hu%2C+J">Josephina Hu</a>, <a href="/search/?searchtype=author&query=Zhang%2C+H">Hugh Zhang</a>, <a href="/search/?searchtype=author&query=Zhang%2C+C+B+C">Chen Bo Calvin Zhang</a>, <a href="/search/?searchtype=author&query=Shaaban%2C+M">Mohamed Shaaban</a>, <a href="/search/?searchtype=author&query=Ling%2C+J">John Ling</a>, <a href="/search/?searchtype=author&query=Shi%2C+S">Sean Shi</a>, <a href="/search/?searchtype=author&query=Choi%2C+M">Michael Choi</a>, <a href="/search/?searchtype=author&query=Agrawal%2C+A">Anish Agrawal</a>, <a href="/search/?searchtype=author&query=Chopra%2C+A">Arnav Chopra</a>, <a href="/search/?searchtype=author&query=Khoja%2C+A">Adam Khoja</a>, <a href="/search/?searchtype=author&query=Kim%2C+R">Ryan Kim</a>, <a href="/search/?searchtype=author&query=Ren%2C+R">Richard Ren</a>, <a href="/search/?searchtype=author&query=Hausenloy%2C+J">Jason Hausenloy</a>, <a href="/search/?searchtype=author&query=Zhang%2C+O">Oliver Zhang</a>, <a href="/search/?searchtype=author&query=Mazeika%2C+M">Mantas Mazeika</a>, <a href="/search/?searchtype=author&query=Nguyen%2C+T">Tung Nguyen</a>, <a href="/search/?searchtype=author&query=Anderson%2C+D">Daron Anderson</a>, <a href="/search/?searchtype=author&query=Shah%2C+I+A">Imad Ali Shah</a>, <a href="/search/?searchtype=author&query=Doroshenko%2C+M">Mikhail Doroshenko</a>, <a href="/search/?searchtype=author&query=Stokes%2C+A+C">Alun Cennyth Stokes</a>, <a href="/search/?searchtype=author&query=Mahmood%2C+M">Mobeen Mahmood</a> , et al. (710 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.14249v4-abstract-short" style="display: inline;"> Benchmarks are important tools for tracking the rapid advancements in large language model (LLM) capabilities. However, benchmarks are not keeping pace in difficulty: LLMs now achieve over 90\% accuracy on popular benchmarks like MMLU, limiting informed measurement of state-of-the-art LLM capabilities. In response, we introduce Humanity's Last Exam (HLE), a multi-modal benchmark at the frontier of… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.14249v4-abstract-full').style.display = 'inline'; document.getElementById('2501.14249v4-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.14249v4-abstract-full" style="display: none;"> Benchmarks are important tools for tracking the rapid advancements in large language model (LLM) capabilities. However, benchmarks are not keeping pace in difficulty: LLMs now achieve over 90\% accuracy on popular benchmarks like MMLU, limiting informed measurement of state-of-the-art LLM capabilities. In response, we introduce Humanity's Last Exam (HLE), a multi-modal benchmark at the frontier of human knowledge, designed to be the final closed-ended academic benchmark of its kind with broad subject coverage. HLE consists of 3,000 questions across dozens of subjects, including mathematics, humanities, and the natural sciences. HLE is developed globally by subject-matter experts and consists of multiple-choice and short-answer questions suitable for automated grading. Each question has a known solution that is unambiguous and easily verifiable, but cannot be quickly answered via internet retrieval. State-of-the-art LLMs demonstrate low accuracy and calibration on HLE, highlighting a significant gap between current LLM capabilities and the expert human frontier on closed-ended academic questions. To inform research and policymaking upon a clear understanding of model capabilities, we publicly release HLE at https://lastexam.ai. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.14249v4-abstract-full').style.display = 'none'; document.getElementById('2501.14249v4-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 24 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">27 pages, 6 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.13896">arXiv:2501.13896</a> <span> [<a href="https://arxiv.org/pdf/2501.13896">pdf</a>, <a href="https://arxiv.org/format/2501.13896">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computer Vision and Pattern Recognition">cs.CV</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Machine Learning">cs.LG</span> </div> </div> <p class="title is-5 mathjax"> GUI-Bee: Align GUI Action Grounding to Novel Environments via Autonomous Exploration </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Fan%2C+Y">Yue Fan</a>, <a href="/search/?searchtype=author&query=Zhao%2C+H">Handong Zhao</a>, <a href="/search/?searchtype=author&query=Zhang%2C+R">Ruiyi Zhang</a>, <a href="/search/?searchtype=author&query=Shen%2C+Y">Yu Shen</a>, <a href="/search/?searchtype=author&query=Wang%2C+X+E">Xin Eric Wang</a>, <a href="/search/?searchtype=author&query=Wu%2C+G">Gang Wu</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.13896v2-abstract-short" style="display: inline;"> Graphical User Interface (GUI) action grounding is a critical step in GUI automation that maps language instructions to actionable elements on GUI screens. Most recent works of GUI action grounding leverage large GUI datasets to fine-tune MLLMs. However, the fine-tuning data always covers limited GUI environments, and we find the performance of the resulting model deteriorates in novel environment… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.13896v2-abstract-full').style.display = 'inline'; document.getElementById('2501.13896v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.13896v2-abstract-full" style="display: none;"> Graphical User Interface (GUI) action grounding is a critical step in GUI automation that maps language instructions to actionable elements on GUI screens. Most recent works of GUI action grounding leverage large GUI datasets to fine-tune MLLMs. However, the fine-tuning data always covers limited GUI environments, and we find the performance of the resulting model deteriorates in novel environments. We argue that the GUI grounding models should be further aligned to the novel environments to reveal their full potential, when the inference is known to involve novel environments, i.e., environments not used during the previous fine-tuning. To realize this, we first propose GUI-Bee, an MLLM-based autonomous agent, to collect high-quality, environment-specific data through exploration and then continuously fine-tune GUI grounding models with the collected data. Our agent leverages a novel Q-value-Incentive In-Context Reinforcement Learning (Q-ICRL) method to optimize exploration efficiency and data quality. Additionally, we introduce NovelScreenSpot, a benchmark for testing how well the data can help align GUI action grounding models to novel environments and demonstrate the effectiveness of data collected by GUI-Bee in the experiments. Furthermore, we conduct an ablation study to validate the Q-ICRL method in enhancing the efficiency of GUI-Bee. Project page: https://gui-bee.github.io <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.13896v2-abstract-full').style.display = 'none'; document.getElementById('2501.13896v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 27 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 23 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.12263">arXiv:2501.12263</a> <span> [<a href="https://arxiv.org/pdf/2501.12263">pdf</a>, <a href="https://arxiv.org/format/2501.12263">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Computer Vision and Pattern Recognition">cs.CV</span> </div> </div> <p class="title is-5 mathjax"> mmCooper: A Multi-agent Multi-stage Communication-efficient and Collaboration-robust Cooperative Perception Framework </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Liu%2C+B">Bingyi Liu</a>, <a href="/search/?searchtype=author&query=Teng%2C+J">Jian Teng</a>, <a href="/search/?searchtype=author&query=Xue%2C+H">Hongfei Xue</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Enshu Wang</a>, <a href="/search/?searchtype=author&query=Zhu%2C+C">Chuanhui Zhu</a>, <a href="/search/?searchtype=author&query=Wang%2C+P">Pu Wang</a>, <a href="/search/?searchtype=author&query=Wu%2C+L">Libing Wu</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.12263v1-abstract-short" style="display: inline;"> Collaborative perception significantly enhances individual vehicle perception performance through the exchange of sensory information among agents. However, real-world deployment faces challenges due to bandwidth constraints and inevitable calibration errors during information exchange. To address these issues, we propose mmCooper, a novel multi-agent, multi-stage, communication-efficient, and col… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.12263v1-abstract-full').style.display = 'inline'; document.getElementById('2501.12263v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.12263v1-abstract-full" style="display: none;"> Collaborative perception significantly enhances individual vehicle perception performance through the exchange of sensory information among agents. However, real-world deployment faces challenges due to bandwidth constraints and inevitable calibration errors during information exchange. To address these issues, we propose mmCooper, a novel multi-agent, multi-stage, communication-efficient, and collaboration-robust cooperative perception framework. Our framework leverages a multi-stage collaboration strategy that dynamically and adaptively balances intermediate- and late-stage information to share among agents, enhancing perceptual performance while maintaining communication efficiency. To support robust collaboration despite potential misalignments and calibration errors, our framework captures multi-scale contextual information for robust fusion in the intermediate stage and calibrates the received detection results to improve accuracy in the late stage. We validate the effectiveness of mmCooper through extensive experiments on real-world and simulated datasets. The results demonstrate the superiority of our proposed framework and the effectiveness of each component. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.12263v1-abstract-full').style.display = 'none'; document.getElementById('2501.12263v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.04298">arXiv:2501.04298</a> <span> [<a href="https://arxiv.org/pdf/2501.04298">pdf</a>, <a href="https://arxiv.org/ps/2501.04298">ps</a>, <a href="https://arxiv.org/format/2501.04298">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> Coupled channel effects for the bottom-strange mesons </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Hao%2C+W">Wei Hao</a>, <a href="/search/?searchtype=author&query=Sultan%2C+M+A">M. Atif Sultan</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">En Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.04298v1-abstract-short" style="display: inline;"> We have calculated the mass spectrum of $B_s$ mesons within a nonrelativistic potential model considering coupled channel effects, and the corresponding strong decay widths within the $^3P_0$ model using the numerically calculated wave functions. By comparing with the available experimental data, we find that the states $B_s$, $B_s^*$, $B_{s1}(5830)$, and $B_{s2}^*(5840)$ could be interpreted as t… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.04298v1-abstract-full').style.display = 'inline'; document.getElementById('2501.04298v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.04298v1-abstract-full" style="display: none;"> We have calculated the mass spectrum of $B_s$ mesons within a nonrelativistic potential model considering coupled channel effects, and the corresponding strong decay widths within the $^3P_0$ model using the numerically calculated wave functions. By comparing with the available experimental data, we find that the states $B_s$, $B_s^*$, $B_{s1}(5830)$, and $B_{s2}^*(5840)$ could be interpreted as the $B_s(1^1S_0)$, $B_s(1^3S_1)$, $B_s(1P^\prime)$, and $B_s(1^3P_2)$, respectively. Although the quantum numbers of the newly observed $B_s(6064)$ and $B_s(6158)$ states have not been determined, our results support the assignments of $B_s(1^3D_3)$ and $B_s(1^3D_1)$ for them. Our predictions are helpful in searching for the bottom-strange meson in future experiments. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.04298v1-abstract-full').style.display = 'none'; document.getElementById('2501.04298v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 8 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.02859">arXiv:2501.02859</a> <span> [<a href="https://arxiv.org/pdf/2501.02859">pdf</a>, <a href="https://arxiv.org/format/2501.02859">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> Roles of the $N(1535)$ and $a_0(980)$ in the process $螞_c^+ \to 蟺^+畏n$ </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Li%2C+M">Meng-Yuan Li</a>, <a href="/search/?searchtype=author&query=Lyu%2C+W">Wen-Tao Lyu</a>, <a href="/search/?searchtype=author&query=Liu%2C+L">Li-Juan Liu</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">En Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.02859v1-abstract-short" style="display: inline;"> We have investigated the process $螞_c^+ \to 蟺^+畏n$ by taking into account the contributions from the nucleon resonance $N(1535)$ and the scalar meson $a_0(980)$, which could be dynamically generated by the interaction of the $S$-wave pseudosalar meson-octet baryon and the $S$-wave pseudosalar meson-pseudosalar meson, respectively. Our results show that, in $畏n$ invariant mass distribution, there i… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.02859v1-abstract-full').style.display = 'inline'; document.getElementById('2501.02859v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.02859v1-abstract-full" style="display: none;"> We have investigated the process $螞_c^+ \to 蟺^+畏n$ by taking into account the contributions from the nucleon resonance $N(1535)$ and the scalar meson $a_0(980)$, which could be dynamically generated by the interaction of the $S$-wave pseudosalar meson-octet baryon and the $S$-wave pseudosalar meson-pseudosalar meson, respectively. Our results show that, in $畏n$ invariant mass distribution, there is a significant near-threshold enhancement structure, which could be associated with $N(1535)$. On the other hand, one can find a clear cusp structure of $a_0(980)$ in $蟺^+畏$ invariant mass distribution. We further estimate the ratio $R$ = $\mathcal{B}(螞_c^+ \to a_0(980)^+ n)/\mathcal{B}(螞_c^+ \to 蟺^+畏n)\approx 0.313$. Our results can be tested by BESIII, Belle~II, and the proposed Super Tau-Charm Facility experiments in the future. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.02859v1-abstract-full').style.display = 'none'; document.getElementById('2501.02859v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">8 pages, 9 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.02839">arXiv:2501.02839</a> <span> [<a href="https://arxiv.org/pdf/2501.02839">pdf</a>, <a href="https://arxiv.org/format/2501.02839">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> Evidence of the open-flavor tetraquark $T_{c\bar{s}2}$ in the process $B^+\to D^{*-}D_s^+蟺^+$ </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Lyu%2C+W">Wen-Tao Lyu</a>, <a href="/search/?searchtype=author&query=Liu%2C+L">Li-Juan Liu</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">En Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.02839v1-abstract-short" style="display: inline;"> The newly observed open-flavor tetraquark $T_{c\bar{s}0}(2900)$ has attracted many attentions, and searching for its spin partners is crucial to exploring the internal structure of those states. In this work, we will show that, the $D_s^+蟺^+$ invariant mass distribution of the process $B^+\to D^{*-}D_s^+蟺^+$ measured by LHCb has a resonant-like structure around 2830~MeV, which could be associated… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.02839v1-abstract-full').style.display = 'inline'; document.getElementById('2501.02839v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.02839v1-abstract-full" style="display: none;"> The newly observed open-flavor tetraquark $T_{c\bar{s}0}(2900)$ has attracted many attentions, and searching for its spin partners is crucial to exploring the internal structure of those states. In this work, we will show that, the $D_s^+蟺^+$ invariant mass distribution of the process $B^+\to D^{*-}D_s^+蟺^+$ measured by LHCb has a resonant-like structure around 2830~MeV, which could be associated with the predicted $T_{c\bar{s}2}$, the spin $J=2$ partner of $T_{c\bar{s}0}(2900)$. Furthermore, we have evaluated the momenta of the angular mass distribution, which are very different for each of the spin assumptions, and have larger strength at the resonant energy than the peaks seen in the angular integrated mass distribution. We make a call for the experimental determination of these magnitudes, which could be used to pin down the existence of the $T_{c\bar{s}2}$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.02839v1-abstract-full').style.display = 'none'; document.getElementById('2501.02839v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 5 figures, comments are welcome</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.00715">arXiv:2501.00715</a> <span> [<a href="https://arxiv.org/pdf/2501.00715">pdf</a>, <a href="https://arxiv.org/format/2501.00715">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> </div> </div> <p class="title is-5 mathjax"> eRevise+RF: A Writing Evaluation System for Assessing Student Essay Revisions and Providing Formative Feedback </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Liu%2C+Z">Zhexiong Liu</a>, <a href="/search/?searchtype=author&query=Litman%2C+D">Diane Litman</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Elaine Wang</a>, <a href="/search/?searchtype=author&query=Li%2C+T">Tianwen Li</a>, <a href="/search/?searchtype=author&query=Gobat%2C+M">Mason Gobat</a>, <a href="/search/?searchtype=author&query=Matsumura%2C+L+C">Lindsay Clare Matsumura</a>, <a href="/search/?searchtype=author&query=Correnti%2C+R">Richard Correnti</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.00715v1-abstract-short" style="display: inline;"> The ability to revise essays in response to feedback is important for students' writing success. An automated writing evaluation (AWE) system that supports students in revising their essays is thus essential. We present eRevise+RF, an enhanced AWE system for assessing student essay revisions (e.g., changes made to an essay to improve its quality in response to essay feedback) and providing revisio… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.00715v1-abstract-full').style.display = 'inline'; document.getElementById('2501.00715v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.00715v1-abstract-full" style="display: none;"> The ability to revise essays in response to feedback is important for students' writing success. An automated writing evaluation (AWE) system that supports students in revising their essays is thus essential. We present eRevise+RF, an enhanced AWE system for assessing student essay revisions (e.g., changes made to an essay to improve its quality in response to essay feedback) and providing revision feedback. We deployed the system with 6 teachers and 406 students across 3 schools in Pennsylvania and Louisiana. The results confirmed its effectiveness in (1) assessing student essays in terms of evidence usage, (2) extracting evidence and reasoning revisions across essays, and (3) determining revision success in responding to feedback. The evaluation also suggested eRevise+RF is a helpful system for young students to improve their argumentative writing skills through revision and formative feedback. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.00715v1-abstract-full').style.display = 'none'; document.getElementById('2501.00715v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 31 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2501.00204">arXiv:2501.00204</a> <span> [<a href="https://arxiv.org/pdf/2501.00204">pdf</a>, <a href="https://arxiv.org/format/2501.00204">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Multimedia">cs.MM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Social and Information Networks">cs.SI</span> </div> </div> <p class="title is-5 mathjax"> MSM-BD: Multimodal Social Media Bot Detection Using Heterogeneous Information </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Wu%2C+T">Tingxuan Wu</a>, <a href="/search/?searchtype=author&query=Ma%2C+Z">Zhaorui Ma</a>, <a href="/search/?searchtype=author&query=Cui%2C+Y">Yanjun Cui</a>, <a href="/search/?searchtype=author&query=Zhou%2C+Z">Ziyi Zhou</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Eric Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2501.00204v1-abstract-short" style="display: inline;"> Although social bots can be engineered for constructive applications, their potential for misuse in manipulative schemes and malware distribution cannot be overlooked. This dichotomy underscores the critical need to detect social bots on social media platforms. Advances in artificial intelligence have improved the abilities of social bots, allowing them to generate content that is almost indisting… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.00204v1-abstract-full').style.display = 'inline'; document.getElementById('2501.00204v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2501.00204v1-abstract-full" style="display: none;"> Although social bots can be engineered for constructive applications, their potential for misuse in manipulative schemes and malware distribution cannot be overlooked. This dichotomy underscores the critical need to detect social bots on social media platforms. Advances in artificial intelligence have improved the abilities of social bots, allowing them to generate content that is almost indistinguishable from human-created content. These advancements require the development of more advanced detection techniques to accurately identify these automated entities. Given the heterogeneous information landscape on social media, spanning images, texts, and user statistical features, we propose MSM-BD, a Multimodal Social Media Bot Detection approach using heterogeneous information. MSM-BD incorporates specialized encoders for heterogeneous information and introduces a cross-modal fusion technology, Cross-Modal Residual Cross-Attention (CMRCA), to enhance detection accuracy. We validate the effectiveness of our model through extensive experiments using the TwiBot-22 dataset. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2501.00204v1-abstract-full').style.display = 'none'; document.getElementById('2501.00204v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2025. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Accept at Springer Nature in Studies in Computational Intelligence</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2412.19743">arXiv:2412.19743</a> <span> [<a href="https://arxiv.org/pdf/2412.19743">pdf</a>, <a href="https://arxiv.org/format/2412.19743">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> Flavor Physics at CEPC: a General Perspective </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Ai%2C+X">Xiaocong Ai</a>, <a href="/search/?searchtype=author&query=Altmannshofer%2C+W">Wolfgang Altmannshofer</a>, <a href="/search/?searchtype=author&query=Athron%2C+P">Peter Athron</a>, <a href="/search/?searchtype=author&query=Bai%2C+X">Xiaozhi Bai</a>, <a href="/search/?searchtype=author&query=Calibbi%2C+L">Lorenzo Calibbi</a>, <a href="/search/?searchtype=author&query=Cao%2C+L">Lu Cao</a>, <a href="/search/?searchtype=author&query=Che%2C+Y">Yuzhi Che</a>, <a href="/search/?searchtype=author&query=Chen%2C+C">Chunhui Chen</a>, <a href="/search/?searchtype=author&query=Chen%2C+J">Ji-Yuan Chen</a>, <a href="/search/?searchtype=author&query=Chen%2C+L">Long Chen</a>, <a href="/search/?searchtype=author&query=Chen%2C+M">Mingshui Chen</a>, <a href="/search/?searchtype=author&query=Chen%2C+S">Shanzhen Chen</a>, <a href="/search/?searchtype=author&query=Chen%2C+X">Xuan Chen</a>, <a href="/search/?searchtype=author&query=Cheng%2C+S">Shan Cheng</a>, <a href="/search/?searchtype=author&query=Chiang%2C+C">Cheng-Wei Chiang</a>, <a href="/search/?searchtype=author&query=Crivellin%2C+A">Andreas Crivellin</a>, <a href="/search/?searchtype=author&query=Cui%2C+H">Hanhua Cui</a>, <a href="/search/?searchtype=author&query=Deschamps%2C+O">Olivier Deschamps</a>, <a href="/search/?searchtype=author&query=Descotes-Genon%2C+S">S茅bastien Descotes-Genon</a>, <a href="/search/?searchtype=author&query=Du%2C+X">Xiaokang Du</a>, <a href="/search/?searchtype=author&query=Fang%2C+S">Shuangshi Fang</a>, <a href="/search/?searchtype=author&query=Gao%2C+Y">Yu Gao</a>, <a href="/search/?searchtype=author&query=Geng%2C+L">Li-Sheng Geng</a>, <a href="/search/?searchtype=author&query=Goldenzweig%2C+P">Pablo Goldenzweig</a>, <a href="/search/?searchtype=author&query=Gu%2C+J">Jiayin Gu</a> , et al. (116 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2412.19743v2-abstract-short" style="display: inline;"> We discuss the landscape of flavor physics at the Circular Electron-Positron Collider (CEPC), based on the nominal luminosity outlined in its Technical Design Report. The CEPC is designed to operate in multiple modes to address a variety of tasks. At the $Z$ pole, the expected production of 4 Tera $Z$ bosons will provide unique and highly precise measurements of $Z$ boson couplings, while the subs… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.19743v2-abstract-full').style.display = 'inline'; document.getElementById('2412.19743v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2412.19743v2-abstract-full" style="display: none;"> We discuss the landscape of flavor physics at the Circular Electron-Positron Collider (CEPC), based on the nominal luminosity outlined in its Technical Design Report. The CEPC is designed to operate in multiple modes to address a variety of tasks. At the $Z$ pole, the expected production of 4 Tera $Z$ bosons will provide unique and highly precise measurements of $Z$ boson couplings, while the substantial number of boosted heavy-flavored quarks and leptons produced in clean $Z$ decays will facilitate investigations into their flavor physics with unprecedented precision. We investigate the prospects of measuring various physics benchmarks and discuss their implications for particle theories and phenomenological models. Our studies indicate that, with its highlighted advantages and anticipated excellent detector performance, the CEPC can explore beauty and $蟿$ physics in ways that are superior to or complementary with the Belle II and Large-Hadron-Collider-beauty experiments, potentially enabling the detection of new physics at energy scales of 10 TeV and above. This potential also extends to the observation of yet-to-be-discovered rare and exotic processes, as well as testing fundamental principles such as lepton flavor universality, lepton and baryon number conservation, etc., making the CEPC a vibrant platform for flavor physics research. The $WW$ threshold scan, Higgs-factory operation and top-pair productions of the CEPC further enhance its merits in this regard, especially for measuring the Cabibbo-Kobayashi-Maskawa matrix elements, and Flavor-Changing-Neutral-Current physics of Higgs boson and top quarks. We outline the requirements for detector performance and considerations for future development to achieve the anticipated scientific goals. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.19743v2-abstract-full').style.display = 'none'; document.getElementById('2412.19743v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 31 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 27 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2412.18544">arXiv:2412.18544</a> <span> [<a href="https://arxiv.org/pdf/2412.18544">pdf</a>, <a href="https://arxiv.org/format/2412.18544">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Machine Learning">cs.LG</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Machine Learning">stat.ML</span> </div> </div> <p class="title is-5 mathjax"> Consistency Checks for Language Model Forecasters </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Paleka%2C+D">Daniel Paleka</a>, <a href="/search/?searchtype=author&query=Sudhir%2C+A+P">Abhimanyu Pallavi Sudhir</a>, <a href="/search/?searchtype=author&query=Alvarez%2C+A">Alejandro Alvarez</a>, <a href="/search/?searchtype=author&query=Bhat%2C+V">Vineeth Bhat</a>, <a href="/search/?searchtype=author&query=Shen%2C+A">Adam Shen</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Evan Wang</a>, <a href="/search/?searchtype=author&query=Tram%C3%A8r%2C+F">Florian Tram猫r</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2412.18544v2-abstract-short" style="display: inline;"> Forecasting is a task that is difficult to evaluate: the ground truth can only be known in the future. Recent work showing LLM forecasters rapidly approaching human-level performance begs the question: how can we benchmark and evaluate these forecasters instantaneously? Following the consistency check framework, we measure the performance of forecasters in terms of the consistency of their predict… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.18544v2-abstract-full').style.display = 'inline'; document.getElementById('2412.18544v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2412.18544v2-abstract-full" style="display: none;"> Forecasting is a task that is difficult to evaluate: the ground truth can only be known in the future. Recent work showing LLM forecasters rapidly approaching human-level performance begs the question: how can we benchmark and evaluate these forecasters instantaneously? Following the consistency check framework, we measure the performance of forecasters in terms of the consistency of their predictions on different logically-related questions. We propose a new, general consistency metric based on arbitrage: for example, if a forecasting AI illogically predicts that both the Democratic and Republican parties have 60% probability of winning the 2024 US presidential election, an arbitrageur can trade against the forecaster's predictions and make a profit. We build an automated evaluation system that generates a set of base questions, instantiates consistency checks from these questions, elicits the predictions of the forecaster, and measures the consistency of the predictions. We then build a standard, proper-scoring-rule forecasting benchmark, and show that our (instantaneous) consistency metrics correlate with LLM forecasters' ground truth Brier scores (which are only known in the future). We also release a consistency benchmark that resolves in 2028, providing a long-term evaluation tool for forecasting. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.18544v2-abstract-full').style.display = 'none'; document.getElementById('2412.18544v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 9 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 24 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">55 pages, 25 figures. Submitted to ICLR 2025</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2412.15001">arXiv:2412.15001</a> <span> [<a href="https://arxiv.org/pdf/2412.15001">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Mesoscale and Nanoscale Physics">cond-mat.mes-hall</span> </div> </div> <p class="title is-5 mathjax"> Observation of liquid-solid transition of nanoconfined water at ambient temperature </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Zheng%2C+W">Wentian Zheng</a>, <a href="/search/?searchtype=author&query=Zhang%2C+S">Shichen Zhang</a>, <a href="/search/?searchtype=author&query=Jiang%2C+J">Jian Jiang</a>, <a href="/search/?searchtype=author&query=He%2C+Y">Yipeng He</a>, <a href="/search/?searchtype=author&query=St%C3%B6hr%2C+R">Rainer St枚hr</a>, <a href="/search/?searchtype=author&query=Denisenko%2C+A">Andrej Denisenko</a>, <a href="/search/?searchtype=author&query=Wrachtrup%2C+J">J枚rg Wrachtrup</a>, <a href="/search/?searchtype=author&query=Zeng%2C+X+C">Xiao Cheng Zeng</a>, <a href="/search/?searchtype=author&query=Bian%2C+K">Ke Bian</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">En-Ge Wang</a>, <a href="/search/?searchtype=author&query=Jiang%2C+Y">Ying Jiang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2412.15001v1-abstract-short" style="display: inline;"> Nanoconfined water plays an indispensable role in various phenomena in biology, chemistry, and engineering. It exhibits many abnormal properties compared to bulk water, especially under strong confinement. However, the origin of those anomalies is still elusive due to the lack of structural information on hydrogen-bonding networks. Considering the inhomogeneity of the nanocavity and the tiny amoun… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.15001v1-abstract-full').style.display = 'inline'; document.getElementById('2412.15001v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2412.15001v1-abstract-full" style="display: none;"> Nanoconfined water plays an indispensable role in various phenomena in biology, chemistry, and engineering. It exhibits many abnormal properties compared to bulk water, especially under strong confinement. However, the origin of those anomalies is still elusive due to the lack of structural information on hydrogen-bonding networks. Considering the inhomogeneity of the nanocavity and the tiny amount of water molecules, conventional optical spectroscopies and nuclear magnetic resonance (NMR) fail to realize the structure analysis of nanoconfined water. Here, we addressed this issue by combining scanning probe microscopy (SPM) with advanced quantum sensing(QS) based on an atomic-size quantum sensor like nitrogen-vacancy (NV) center in diamond, which can apply the nanoscale-NMR for characterizing both the dynamics and structure of confined water at ambient conditions. We built a two-dimensional (2D) nanoconfined water system with a hexagonal-boron nitride (hBN) flake and a hydrophilic diamond surface. By using the SPM tip to measure the confinement size precisely, we observed a critical confinement size of ~2 nm, below which the water diffusion was significantly suppressed and the hydrogen-bonding network of water showed an ordered structure. Meanwhile, molecular dynamics (MD) simulation revealed a solid-like water contact layer on the diamond surface under strong confinement, which also reproduced the measured nanoscale-NMR spectra and confirmed the liquid-solid phase transition observed in the experiments. Notably, with this new SPM-QS platform, our results showed a promising way to elucidate the abnormal properties of nanoconfined water in future applications. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.15001v1-abstract-full').style.display = 'none'; document.getElementById('2412.15001v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2412.14260">arXiv:2412.14260</a> <span> [<a href="https://arxiv.org/pdf/2412.14260">pdf</a>, <a href="https://arxiv.org/format/2412.14260">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Measurement of the branching fraction and $\it CP$-violating asymmetry of the decay $B^{0} \rightarrow 蟺^{0} 蟺^{0}$ using $387$ million bottom-antibottom meson pairs in Belle II data </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Belle+II+Collaboration"> Belle II Collaboration</a>, <a href="/search/?searchtype=author&query=Adachi%2C+I">I. Adachi</a>, <a href="/search/?searchtype=author&query=Aggarwal%2C+L">L. Aggarwal</a>, <a href="/search/?searchtype=author&query=Ahmed%2C+H">H. Ahmed</a>, <a href="/search/?searchtype=author&query=Aihara%2C+H">H. Aihara</a>, <a href="/search/?searchtype=author&query=Alhakami%2C+M">M. Alhakami</a>, <a href="/search/?searchtype=author&query=Aloisio%2C+A">A. Aloisio</a>, <a href="/search/?searchtype=author&query=Althubiti%2C+N">N. Althubiti</a>, <a href="/search/?searchtype=author&query=Ky%2C+N+A">N. Anh Ky</a>, <a href="/search/?searchtype=author&query=Asner%2C+D+M">D. M. Asner</a>, <a href="/search/?searchtype=author&query=Atmacan%2C+H">H. Atmacan</a>, <a href="/search/?searchtype=author&query=Aushev%2C+V">V. Aushev</a>, <a href="/search/?searchtype=author&query=Aversano%2C+M">M. Aversano</a>, <a href="/search/?searchtype=author&query=Ayad%2C+R">R. Ayad</a>, <a href="/search/?searchtype=author&query=Babu%2C+V">V. Babu</a>, <a href="/search/?searchtype=author&query=Bae%2C+H">H. Bae</a>, <a href="/search/?searchtype=author&query=Baghel%2C+N+K">N. K. Baghel</a>, <a href="/search/?searchtype=author&query=Bahinipati%2C+S">S. Bahinipati</a>, <a href="/search/?searchtype=author&query=Bambade%2C+P">P. Bambade</a>, <a href="/search/?searchtype=author&query=Banerjee%2C+S">Sw. Banerjee</a>, <a href="/search/?searchtype=author&query=Bansal%2C+S">S. Bansal</a>, <a href="/search/?searchtype=author&query=Barrett%2C+M">M. Barrett</a>, <a href="/search/?searchtype=author&query=Bartl%2C+M">M. Bartl</a>, <a href="/search/?searchtype=author&query=Baudot%2C+J">J. Baudot</a>, <a href="/search/?searchtype=author&query=Baur%2C+A">A. Baur</a> , et al. (415 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2412.14260v1-abstract-short" style="display: inline;"> We measure the branching fraction and $\it CP$-violating flavor-dependent rate asymmetry of $B^{0} \to 蟺^{0} 蟺^{0}$ decays reconstructed using the Belle II detector in an electron-positron collision sample containing $387 \times 10^{6}$ $B\overline{B}$ pairs. Using an optimized event selection, we find $126\pm 20$ signal decays in a fit to background-discriminating and flavor-sensitive distributio… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.14260v1-abstract-full').style.display = 'inline'; document.getElementById('2412.14260v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2412.14260v1-abstract-full" style="display: none;"> We measure the branching fraction and $\it CP$-violating flavor-dependent rate asymmetry of $B^{0} \to 蟺^{0} 蟺^{0}$ decays reconstructed using the Belle II detector in an electron-positron collision sample containing $387 \times 10^{6}$ $B\overline{B}$ pairs. Using an optimized event selection, we find $126\pm 20$ signal decays in a fit to background-discriminating and flavor-sensitive distributions. The resulting branching fraction is $(1.25 \pm 0.23)\times 10^{-6}$ and the $\it CP$-violating asymmetry is $0.03 \pm 0.30$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.14260v1-abstract-full').style.display = 'none'; document.getElementById('2412.14260v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> Belle II Preprint 2024-032, KEK Preprint 2024-34 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2412.12510">arXiv:2412.12510</a> <span> [<a href="https://arxiv.org/pdf/2412.12510">pdf</a>, <a href="https://arxiv.org/format/2412.12510">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computers and Society">cs.CY</span> </div> </div> <p class="title is-5 mathjax"> Can Large Language Models Understand You Better? An MBTI Personality Detection Dataset Aligned with Population Traits </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Li%2C+B">Bohan Li</a>, <a href="/search/?searchtype=author&query=Guan%2C+J">Jiannan Guan</a>, <a href="/search/?searchtype=author&query=Dou%2C+L">Longxu Dou</a>, <a href="/search/?searchtype=author&query=Feng%2C+Y">Yunlong Feng</a>, <a href="/search/?searchtype=author&query=Wang%2C+D">Dingzirui Wang</a>, <a href="/search/?searchtype=author&query=Xu%2C+Y">Yang Xu</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Enbo Wang</a>, <a href="/search/?searchtype=author&query=Chen%2C+Q">Qiguang Chen</a>, <a href="/search/?searchtype=author&query=Wang%2C+B">Bichen Wang</a>, <a href="/search/?searchtype=author&query=Xu%2C+X">Xiao Xu</a>, <a href="/search/?searchtype=author&query=Zhang%2C+Y">Yimeng Zhang</a>, <a href="/search/?searchtype=author&query=Qin%2C+L">Libo Qin</a>, <a href="/search/?searchtype=author&query=Zhao%2C+Y">Yanyan Zhao</a>, <a href="/search/?searchtype=author&query=Zhu%2C+Q">Qingfu Zhu</a>, <a href="/search/?searchtype=author&query=Che%2C+W">Wanxiang Che</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2412.12510v1-abstract-short" style="display: inline;"> The Myers-Briggs Type Indicator (MBTI) is one of the most influential personality theories reflecting individual differences in thinking, feeling, and behaving. MBTI personality detection has garnered considerable research interest and has evolved significantly over the years. However, this task tends to be overly optimistic, as it currently does not align well with the natural distribution of pop… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.12510v1-abstract-full').style.display = 'inline'; document.getElementById('2412.12510v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2412.12510v1-abstract-full" style="display: none;"> The Myers-Briggs Type Indicator (MBTI) is one of the most influential personality theories reflecting individual differences in thinking, feeling, and behaving. MBTI personality detection has garnered considerable research interest and has evolved significantly over the years. However, this task tends to be overly optimistic, as it currently does not align well with the natural distribution of population personality traits. Specifically, (1) the self-reported labels in existing datasets result in incorrect labeling issues, and (2) the hard labels fail to capture the full range of population personality distributions. In this paper, we optimize the task by constructing MBTIBench, the first manually annotated high-quality MBTI personality detection dataset with soft labels, under the guidance of psychologists. As for the first challenge, MBTIBench effectively solves the incorrect labeling issues, which account for 29.58% of the data. As for the second challenge, we estimate soft labels by deriving the polarity tendency of samples. The obtained soft labels confirm that there are more people with non-extreme personality traits. Experimental results not only highlight the polarized predictions and biases in LLMs as key directions for future research, but also confirm that soft labels can provide more benefits to other psychological tasks than hard labels. The code and data are available at https://github.com/Personality-NLP/MbtiBench. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.12510v1-abstract-full').style.display = 'none'; document.getElementById('2412.12510v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 16 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Accepted by COLING 2025. 28 papges, 20 figures, 10 tables</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2412.11498">arXiv:2412.11498</a> <span> [<a href="https://arxiv.org/pdf/2412.11498">pdf</a>, <a href="https://arxiv.org/ps/2412.11498">ps</a>, <a href="https://arxiv.org/format/2412.11498">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> Strangeonium spectrum with the screening effects and interpretation of $h_1(1911)$ and $h_1(2316)$ observed by BESIII </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Hao%2C+W">Wei Hao</a>, <a href="/search/?searchtype=author&query=Sultan%2C+M+A">M. Atif Sultan</a>, <a href="/search/?searchtype=author&query=Liu%2C+L">Li-Juan Liu</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">En Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2412.11498v1-abstract-short" style="display: inline;"> Motivated by two news states $h_1(1911)$ and $h_1(2316)$ observed by BESIII, we have investigated the mass spectrum and the strong decay properties of the strangeonium mesons within the modified Godfrey-Isgur model by considering the screening effects. We have determined the free parameters using the masses and widths of the well established $s\bar{s}$ states $蠁(1020)$, $蠁(1680)$, $h_1(1415)$,… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.11498v1-abstract-full').style.display = 'inline'; document.getElementById('2412.11498v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2412.11498v1-abstract-full" style="display: none;"> Motivated by two news states $h_1(1911)$ and $h_1(2316)$ observed by BESIII, we have investigated the mass spectrum and the strong decay properties of the strangeonium mesons within the modified Godfrey-Isgur model by considering the screening effects. We have determined the free parameters using the masses and widths of the well established $s\bar{s}$ states $蠁(1020)$, $蠁(1680)$, $h_1(1415)$, $f_2^\prime(1525)$, and $蠁_3(1850)$. According to our results, $h_1(1911)$ and $h_1(2316)$ could be well explained as states $h_1(2^1P_1)$ and $h_1(3^1P_1)$ $s\bar{s}$ states, respectively. Meanwhile, the possible assignments of $X(2000)$, $畏_2(1870)$, and $蠁(2170)$ as $3^3S_1$, $1^1D_2$, and $2^3D_1$ are also discussed. Furthermore, the masses and widths of the $2S$, $3S$, $1P$, $2P$, $3P$, $1D$, and $2D$ $s\bar{s}$ states are also given and compared with various theoretical predictions, which is helpful for the observations and confirmations of these states in future. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.11498v1-abstract-full').style.display = 'none'; document.getElementById('2412.11498v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 16 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2412.08948">arXiv:2412.08948</a> <span> [<a href="https://arxiv.org/pdf/2412.08948">pdf</a>, <a href="https://arxiv.org/format/2412.08948">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Computer Vision and Pattern Recognition">cs.CV</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> </div> </div> <p class="title is-5 mathjax"> Mojito: Motion Trajectory and Intensity Control for Video Generation </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=He%2C+X">Xuehai He</a>, <a href="/search/?searchtype=author&query=Wang%2C+S">Shuohang Wang</a>, <a href="/search/?searchtype=author&query=Yang%2C+J">Jianwei Yang</a>, <a href="/search/?searchtype=author&query=Wu%2C+X">Xiaoxia Wu</a>, <a href="/search/?searchtype=author&query=Wang%2C+Y">Yiping Wang</a>, <a href="/search/?searchtype=author&query=Wang%2C+K">Kuan Wang</a>, <a href="/search/?searchtype=author&query=Zhan%2C+Z">Zheng Zhan</a>, <a href="/search/?searchtype=author&query=Ruwase%2C+O">Olatunji Ruwase</a>, <a href="/search/?searchtype=author&query=Shen%2C+Y">Yelong Shen</a>, <a href="/search/?searchtype=author&query=Wang%2C+X+E">Xin Eric Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2412.08948v2-abstract-short" style="display: inline;"> Recent advancements in diffusion models have shown great promise in producing high-quality video content. However, efficiently training video diffusion models capable of integrating directional guidance and controllable motion intensity remains a challenging and under-explored area. To tackle these challenges, this paper introduces Mojito, a diffusion model that incorporates both motion trajectory… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.08948v2-abstract-full').style.display = 'inline'; document.getElementById('2412.08948v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2412.08948v2-abstract-full" style="display: none;"> Recent advancements in diffusion models have shown great promise in producing high-quality video content. However, efficiently training video diffusion models capable of integrating directional guidance and controllable motion intensity remains a challenging and under-explored area. To tackle these challenges, this paper introduces Mojito, a diffusion model that incorporates both motion trajectory and intensity control for text-to-video generation. Specifically, Mojito features a Directional Motion Control (DMC) module that leverages cross-attention to efficiently direct the generated object's motion without training, alongside a Motion Intensity Modulator (MIM) that uses optical flow maps generated from videos to guide varying levels of motion intensity. Extensive experiments demonstrate Mojito's effectiveness in achieving precise trajectory and intensity control with high computational efficiency, generating motion patterns that closely match specified directions and intensities, providing realistic dynamics that align well with natural motion in real-world scenarios. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.08948v2-abstract-full').style.display = 'none'; document.getElementById('2412.08948v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 12 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2412.08492">arXiv:2412.08492</a> <span> [<a href="https://arxiv.org/pdf/2412.08492">pdf</a>, <a href="https://arxiv.org/format/2412.08492">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Combinatorics">math.CO</span> </div> </div> <p class="title is-5 mathjax"> Tilings of the sphere by congruent pentagons IV: Edge combination $a^4b$ with general angles </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Shu%2C+J">Junjie Shu</a>, <a href="/search/?searchtype=author&query=Liao%2C+Y">Yixi Liao</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Erxiao Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2412.08492v1-abstract-short" style="display: inline;"> We classify edge-to-edge tilings of the sphere by congruent pentagons with the edge combination $a^4b$ and with any irrational angle in degree: they are three $1$-parameter families of pentagonal subdivisions of the Platonic solids, with $12, 24$ and $60$ tiles; and a sequence of $1$-parameter families of pentagons admitting non-symmetric $3$-layer earth map tilings together with their various rea… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.08492v1-abstract-full').style.display = 'inline'; document.getElementById('2412.08492v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2412.08492v1-abstract-full" style="display: none;"> We classify edge-to-edge tilings of the sphere by congruent pentagons with the edge combination $a^4b$ and with any irrational angle in degree: they are three $1$-parameter families of pentagonal subdivisions of the Platonic solids, with $12, 24$ and $60$ tiles; and a sequence of $1$-parameter families of pentagons admitting non-symmetric $3$-layer earth map tilings together with their various rearrangements under extra conditions. Their parameter moduli and geometric data are all computed in both exact and numerical form. The total numbers of different tilings for any fixed such pentagon are counted explicitly. As a byproduct, the degenerate pentagons produce naturally many new non-edge-to-edge quadrilateral tilings. A sequel of this paper will handle $a^4b$-pentagons with all angles being rational in degree by solving some trigonometric Diophantine equations, to complete our full classification of edge-to-edge tilings of the sphere by congruent pentagons. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.08492v1-abstract-full').style.display = 'none'; document.getElementById('2412.08492v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">46 pages,36 figures, 31 tables</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">MSC Class:</span> 52C20; 05B45 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2412.07176">arXiv:2412.07176</a> <span> [<a href="https://arxiv.org/pdf/2412.07176">pdf</a>, <a href="https://arxiv.org/format/2412.07176">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Astrophysics of Galaxies">astro-ph.GA</span> </div> </div> <p class="title is-5 mathjax"> The first exploration of the correlations between \textit{WISE} 12 \micron\ and CO emission in early-type galaxies </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Gao%2C+Y">Yang Gao</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Enci Wang</a>, <a href="/search/?searchtype=author&query=Tan%2C+Q">Qing-Hua Tan</a>, <a href="/search/?searchtype=author&query=Davis%2C+T+A">Timothy A. Davis</a>, <a href="/search/?searchtype=author&query=Liang%2C+F">Fu-Heng Liang</a>, <a href="/search/?searchtype=author&query=Jiang%2C+X">Xue-Jian Jiang</a>, <a href="/search/?searchtype=author&query=Gai%2C+N">Ning Gai</a>, <a href="/search/?searchtype=author&query=Jiao%2C+Q">Qian Jiao</a>, <a href="/search/?searchtype=author&query=Shi%2C+D">DongDong Shi</a>, <a href="/search/?searchtype=author&query=Feng%2C+S">Shuai Feng</a>, <a href="/search/?searchtype=author&query=Tang%2C+Y">Yanke Tang</a>, <a href="/search/?searchtype=author&query=Li%2C+S">Shijie Li</a>, <a href="/search/?searchtype=author&query=Wang%2C+Y">Yi-Fan Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2412.07176v1-abstract-short" style="display: inline;"> We present the analysis of a comprehensive sample of 352 early-type galaxies using public data, to investigate the correlations between CO luminosities and mid-infrared luminosities observed by \textit{Wide-field Infrared Survey Explorer} (\textit{WISE}). We find strong correlations between both CO (1-0) and CO (2-1) luminosities and 12 \micron\ luminosity, boasting a correlation coefficient great… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.07176v1-abstract-full').style.display = 'inline'; document.getElementById('2412.07176v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2412.07176v1-abstract-full" style="display: none;"> We present the analysis of a comprehensive sample of 352 early-type galaxies using public data, to investigate the correlations between CO luminosities and mid-infrared luminosities observed by \textit{Wide-field Infrared Survey Explorer} (\textit{WISE}). We find strong correlations between both CO (1-0) and CO (2-1) luminosities and 12 \micron\ luminosity, boasting a correlation coefficient greater than 0.9 and an intrinsic scatter smaller than 0.1 dex. The consistent slopes observed for the relationships of CO (1-0) and CO (2-1) suggest that the line ratio R21 lacks correlation with mid-infrared emission in early-type galaxies, which is significantly different from star-forming galaxies. Moreover, the slopes of $L_{\rm CO (1-0)}$--$L_{\mbox{12\micron}}$ and $L_{\rm CO (2-1)}$--$L_{\mbox{12\micron}}$ relations in early-type galaxies are steeper than those observed in star-forming galaxies. Given the absence of correlation with color, morphology or sSFR, the correlation between deviations and the molecular gas mass surface density could be eliminated by correcting the possible 12 \micron\ emission from old stars or adopting a systematically different $伪_{\rm CO}$. The latter, on average, is equivalent to adding an constant CO brightness density, specifically ${2.8{_{-0.6}}\!\!\!\!\!\!\!\!\!^{+0.8}}~[\mathrm{K~km~s^{-1}}]$ and ${4.4{_{-1.4}}\!\!\!\!\!\!\!\!\!^{+2.2}}~[\mathrm{K~km~s^{-1}}]$ for CO (1-0) and (2-1) respectively. These explorations will serve as useful tools for estimating the molecular gas content in gas-poor galaxies and understanding associated quenching processes. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.07176v1-abstract-full').style.display = 'none'; document.getElementById('2412.07176v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 9 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">20 pages, 6 figures, accepted for publication in ApJ</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.18869">arXiv:2411.18869</a> <span> [<a href="https://arxiv.org/pdf/2411.18869">pdf</a>, <a href="https://arxiv.org/format/2411.18869">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Lattice">hep-lat</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Theory">hep-th</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</span> </div> </div> <p class="title is-5 mathjax"> Quantum computing of chirality imbalance in SU(2) gauge theory </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Zhang%2C+G">Guofeng Zhang</a>, <a href="/search/?searchtype=author&query=Guo%2C+X">Xingyu Guo</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Enke Wang</a>, <a href="/search/?searchtype=author&query=Xing%2C+H">Hongxi Xing</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.18869v2-abstract-short" style="display: inline;"> We implement a variational quantum algorithm to investigate the chiral condensate in a 1+1 dimensional SU(2) non-Abelian gauge theory. The algorithm is evaluated using a proposed Monte Carlo sampling method, which allows the extension to large qubit systems. The obtained results through quantum simulations on classical and actual quantum hardware are in good agreement with exact diagonalization of… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.18869v2-abstract-full').style.display = 'inline'; document.getElementById('2411.18869v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.18869v2-abstract-full" style="display: none;"> We implement a variational quantum algorithm to investigate the chiral condensate in a 1+1 dimensional SU(2) non-Abelian gauge theory. The algorithm is evaluated using a proposed Monte Carlo sampling method, which allows the extension to large qubit systems. The obtained results through quantum simulations on classical and actual quantum hardware are in good agreement with exact diagonalization of the lattice Hamiltonian, revealing the phenomena of chiral symmetry breaking and restoration as functions of both temperature and chemical potential. Our findings underscore the potential of near-term quantum computing for exploring QCD systems at finite temperature and density in non-Abelian gauge theories. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.18869v2-abstract-full').style.display = 'none'; document.getElementById('2411.18869v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 1 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 27 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">9 pages, 6 figures, submitted to science bulletin, fixed issues with figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.14032">arXiv:2411.14032</a> <span> [<a href="https://arxiv.org/pdf/2411.14032">pdf</a>, <a href="https://arxiv.org/format/2411.14032">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Measurement of the inclusive branching fractions for $B_s^0$ decays into $D$ mesons via hadronic tagging </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Belle"> Belle</a>, <a href="/search/?searchtype=author&query=Collaborations%2C+B+I">Belle II Collaborations</a>, <a href="/search/?searchtype=author&query=%3A"> :</a>, <a href="/search/?searchtype=author&query=Adachi%2C+I">I. Adachi</a>, <a href="/search/?searchtype=author&query=Aggarwal%2C+L">L. Aggarwal</a>, <a href="/search/?searchtype=author&query=Ahmed%2C+H">H. Ahmed</a>, <a href="/search/?searchtype=author&query=Aihara%2C+H">H. Aihara</a>, <a href="/search/?searchtype=author&query=Akopov%2C+N">N. Akopov</a>, <a href="/search/?searchtype=author&query=Aloisio%2C+A">A. Aloisio</a>, <a href="/search/?searchtype=author&query=Said%2C+S+A">S. Al Said</a>, <a href="/search/?searchtype=author&query=Althubiti%2C+N">N. Althubiti</a>, <a href="/search/?searchtype=author&query=Ky%2C+N+A">N. Anh Ky</a>, <a href="/search/?searchtype=author&query=Asner%2C+D+M">D. M. Asner</a>, <a href="/search/?searchtype=author&query=Atmacan%2C+H">H. Atmacan</a>, <a href="/search/?searchtype=author&query=Aushev%2C+T">T. Aushev</a>, <a href="/search/?searchtype=author&query=Aushev%2C+V">V. Aushev</a>, <a href="/search/?searchtype=author&query=Aversano%2C+M">M. Aversano</a>, <a href="/search/?searchtype=author&query=Ayad%2C+R">R. Ayad</a>, <a href="/search/?searchtype=author&query=Babu%2C+V">V. Babu</a>, <a href="/search/?searchtype=author&query=Bae%2C+H">H. Bae</a>, <a href="/search/?searchtype=author&query=Baghel%2C+N+K">N. K. Baghel</a>, <a href="/search/?searchtype=author&query=Bahinipati%2C+S">S. Bahinipati</a>, <a href="/search/?searchtype=author&query=Bambade%2C+P">P. Bambade</a>, <a href="/search/?searchtype=author&query=Banerjee%2C+S">Sw. Banerjee</a>, <a href="/search/?searchtype=author&query=Bansal%2C+S">S. Bansal</a> , et al. (430 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.14032v2-abstract-short" style="display: inline;"> We report measurements of the absolute branching fractions $\mathcal{B}(B_s^0 \to D_s^{\pm} X)$, $\mathcal{B}(B_s^0 \to D^0/\bar{D}^0 X)$, and $\mathcal{B}(B_s^0 \to D^{\pm} X)$, where the latter is measured for the first time. The results are based on a 121.4\,fb$^{-1}$ data sample collected at the $违(10860)$ resonance by the Belle detector at the KEKB asymmetric-energy $e^+ e^-$ collider. We rec… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.14032v2-abstract-full').style.display = 'inline'; document.getElementById('2411.14032v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.14032v2-abstract-full" style="display: none;"> We report measurements of the absolute branching fractions $\mathcal{B}(B_s^0 \to D_s^{\pm} X)$, $\mathcal{B}(B_s^0 \to D^0/\bar{D}^0 X)$, and $\mathcal{B}(B_s^0 \to D^{\pm} X)$, where the latter is measured for the first time. The results are based on a 121.4\,fb$^{-1}$ data sample collected at the $违(10860)$ resonance by the Belle detector at the KEKB asymmetric-energy $e^+ e^-$ collider. We reconstruct one $B_s^0$ meson in $e^+e^- \to 违(10860) \to B_s^{*} \bar{B}_s^{*}$ events and measure yields of $D_s^+$, $D^0$, and $D^+$ mesons in the rest of the event. We obtain $\mathcal{B}(B_s^0 \to D_s^{\pm} X) = (68.6 \pm 7.2 \pm 4.0)\%$, $\mathcal{B}(B_s^0 \to D^0/\bar{D}^0 X) = (21.5 \pm 6.1 \pm 1.8)\%$, and $\mathcal{B}(B_s^0 \to D^{\pm} X) = (12.6 \pm 4.6 \pm 1.3)\%$, where the first uncertainty is statistical and the second is systematic. Averaging with previous Belle measurements gives $\mathcal{B}(B_s^0 \to D_s^{\pm} X) = (63.4 \pm 4.5 \pm 2.2)\%$ and $\mathcal{B}(B_s^0 \to D^0/\bar{D}^0 X) = (23.9 \pm 4.1 \pm 1.8)\%$. For the $B_s^0$ production fraction at the $违(10860)$, we find $f_s = (21.4^{+1.5}_{-1.7})\%$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.14032v2-abstract-full').style.display = 'none'; document.getElementById('2411.14032v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 21 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">23 pages, 9 figures, submitted to JHEP</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> Belle II Preprint 2024-030, KEK Preprint 2024-32 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.10127">arXiv:2411.10127</a> <span> [<a href="https://arxiv.org/pdf/2411.10127">pdf</a>, <a href="https://arxiv.org/format/2411.10127">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Measurement of $B \to K{}^{*}(892)纬$ decays at Belle II </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Belle+II+Collaboration"> Belle II Collaboration</a>, <a href="/search/?searchtype=author&query=Adachi%2C+I">I. Adachi</a>, <a href="/search/?searchtype=author&query=Aggarwal%2C+L">L. Aggarwal</a>, <a href="/search/?searchtype=author&query=Ahmed%2C+H">H. Ahmed</a>, <a href="/search/?searchtype=author&query=Aihara%2C+H">H. Aihara</a>, <a href="/search/?searchtype=author&query=Akopov%2C+N">N. Akopov</a>, <a href="/search/?searchtype=author&query=Aloisio%2C+A">A. Aloisio</a>, <a href="/search/?searchtype=author&query=Althubiti%2C+N">N. Althubiti</a>, <a href="/search/?searchtype=author&query=Ky%2C+N+A">N. Anh Ky</a>, <a href="/search/?searchtype=author&query=Asner%2C+D+M">D. M. Asner</a>, <a href="/search/?searchtype=author&query=Atmacan%2C+H">H. Atmacan</a>, <a href="/search/?searchtype=author&query=Aushev%2C+T">T. Aushev</a>, <a href="/search/?searchtype=author&query=Aushev%2C+V">V. Aushev</a>, <a href="/search/?searchtype=author&query=Aversano%2C+M">M. Aversano</a>, <a href="/search/?searchtype=author&query=Ayad%2C+R">R. Ayad</a>, <a href="/search/?searchtype=author&query=Babu%2C+V">V. Babu</a>, <a href="/search/?searchtype=author&query=Bae%2C+H">H. Bae</a>, <a href="/search/?searchtype=author&query=Baghel%2C+N+K">N. K. Baghel</a>, <a href="/search/?searchtype=author&query=Bahinipati%2C+S">S. Bahinipati</a>, <a href="/search/?searchtype=author&query=Bambade%2C+P">P. Bambade</a>, <a href="/search/?searchtype=author&query=Banerjee%2C+S">Sw. Banerjee</a>, <a href="/search/?searchtype=author&query=Bansal%2C+S">S. Bansal</a>, <a href="/search/?searchtype=author&query=Barrett%2C+M">M. Barrett</a>, <a href="/search/?searchtype=author&query=Bartl%2C+M">M. Bartl</a>, <a href="/search/?searchtype=author&query=Baudot%2C+J">J. Baudot</a> , et al. (429 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.10127v1-abstract-short" style="display: inline;"> We present measurements of $B \to K{}^{*}(892)纬$ decays using $365\,{\rm fb}^{-1}$ of data collected from 2019 to 2022 by the Belle~II experiment at the SuperKEKB asymmetric-energy $e^+e^-$ collider. The data sample contains $(387 \pm 6) \times 10^6$ $B\overline{B}$ events. We measure branching fractions ($\mathcal{B}$) and $C\!P$ asymmetries ($\mathcal{A}_{C\!P}$) for both $B^{0}\to K{}^{*0}纬$ an… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.10127v1-abstract-full').style.display = 'inline'; document.getElementById('2411.10127v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.10127v1-abstract-full" style="display: none;"> We present measurements of $B \to K{}^{*}(892)纬$ decays using $365\,{\rm fb}^{-1}$ of data collected from 2019 to 2022 by the Belle~II experiment at the SuperKEKB asymmetric-energy $e^+e^-$ collider. The data sample contains $(387 \pm 6) \times 10^6$ $B\overline{B}$ events. We measure branching fractions ($\mathcal{B}$) and $C\!P$ asymmetries ($\mathcal{A}_{C\!P}$) for both $B^{0}\to K{}^{*0}纬$ and $B^{+}\to K{}^{*+}纬$ decays. The difference in $C\!P$ asymmetries ($螖\mathcal{A}_{C\!P}$) and the isospin asymmetry ($螖_{0+}$) between these neutral and charged channels are also measured. We obtain the following branching fractions and $C\!P$ asymmetries: $\mathcal{B} (B^{0} \to K{}^{*0}纬) = (4.14 \pm 0.10 \pm 0.11 ) \times 10^{-5}$, $\mathcal{B} (B^{+} \to K{}^{*+}纬) = (4.02 \pm 0.13 \pm 0.13 )\times 10^{-5}$, $\mathcal{A}_{C\!P} (B^{0} \to K{}^{*0}纬) = (-3.3 \pm 2.3 \pm 0.4 )\%$, and $\mathcal{A}_{C\!P} (B^{+} \to K{}^{*+}纬) = (-0.7 \pm 2.9 \pm 0.6 )\%$. The measured difference in $C\!P$ asymmetries is $螖\mathcal{A}_{C\!P} = (+2.6 \pm 3.8 \pm 0.7 )\%$, and the measured isospin asymmetry is $螖_{0+} = (+5.0 \pm 2.0 \pm 1.5 )\%$. The first uncertainties listed are statistical and the second are systematic. These results are consistent with world-average values and theory predictions. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.10127v1-abstract-full').style.display = 'none'; document.getElementById('2411.10127v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 15 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> Belle II Preprint 2024-029; KEK Preprint 2024-31 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.09765">arXiv:2411.09765</a> <span> [<a href="https://arxiv.org/pdf/2411.09765">pdf</a>, <a href="https://arxiv.org/format/2411.09765">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Cosmology and Nongalactic Astrophysics">astro-ph.CO</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> The Neutrino Mass Bound from Leptogenesis Revisited </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Garbrecht%2C+B">Bj枚rn Garbrecht</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Edward Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.09765v1-abstract-short" style="display: inline;"> We revisit unflavoured leptogenesis in the seesaw model applying recent improvements in the computation of $CP$-conserving and $CP$-violating equilibration rates. These are relevant for the relativistic regime of the sterile Majorana fermions and the dynamics of the Standard Model particles acting as spectator processes. In order to probe the regime of large (${\cal O}(10^2)$) washout parameters,… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.09765v1-abstract-full').style.display = 'inline'; document.getElementById('2411.09765v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.09765v1-abstract-full" style="display: none;"> We revisit unflavoured leptogenesis in the seesaw model applying recent improvements in the computation of $CP$-conserving and $CP$-violating equilibration rates. These are relevant for the relativistic regime of the sterile Majorana fermions and the dynamics of the Standard Model particles acting as spectator processes. In order to probe the regime of large (${\cal O}(10^2)$) washout parameters, we add $螖L = 2$ washout processes, which we derive in the CTP-formalism. We then perform a parameter scan of the final baryon asymmetry and find a constraint $m_{\text{lightest}} \lesssim 0.15 \, \rm eV$ on the absolute neutrino mass scale, which is slightly less stringent than previously reported bounds obtained without the aforementioned improvements. The relaxation of the bounds is mainly due to partially equilibrated spectator fields, which protect part of the asymmetry from washout and lead to larger final asymmetries. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.09765v1-abstract-full').style.display = 'none'; document.getElementById('2411.09765v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">14 pages, 4 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> TUM-HEP-1535/24 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.08485">arXiv:2411.08485</a> <span> [<a href="https://arxiv.org/pdf/2411.08485">pdf</a>, <a href="https://arxiv.org/format/2411.08485">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Astrophysics of Galaxies">astro-ph.GA</span> </div> </div> <p class="title is-5 mathjax"> The circumgalactic medium traced by Mg II absorption with DESI: dependence on galaxy stellar mass, star formation rate and azimuthal angle </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Chen%2C+Z">Zeyu Chen</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Enci Wang</a>, <a href="/search/?searchtype=author&query=Zou%2C+H">Hu Zou</a>, <a href="/search/?searchtype=author&query=Zou%2C+S">Siwei Zou</a>, <a href="/search/?searchtype=author&query=Gao%2C+Y">Yang Gao</a>, <a href="/search/?searchtype=author&query=Wang%2C+H">Huiyuan Wang</a>, <a href="/search/?searchtype=author&query=Yu%2C+H">Haoran Yu</a>, <a href="/search/?searchtype=author&query=Jia%2C+C">Cheng Jia</a>, <a href="/search/?searchtype=author&query=Li%2C+H">Haixin Li</a>, <a href="/search/?searchtype=author&query=Ma%2C+C">Chengyu Ma</a>, <a href="/search/?searchtype=author&query=Yao%2C+Y">Yao Yao</a>, <a href="/search/?searchtype=author&query=Ding%2C+W">Weiyu Ding</a>, <a href="/search/?searchtype=author&query=Zhu%2C+R">Runyu Zhu</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.08485v2-abstract-short" style="display: inline;"> Understanding the circumgalactic medium (CGM) distribution of galaxies is the key to revealing the dynamical exchange of materials between galaxies and their surroundings. In this work, we use DESI EDR dataset to investigate the cool CGM of galaxies ($0.3<z<1.7$) with stacking the spectra of background QSOs to obtain Mg II absorption of foreground galaxies. The equivalent width of Mg II absorption… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.08485v2-abstract-full').style.display = 'inline'; document.getElementById('2411.08485v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.08485v2-abstract-full" style="display: none;"> Understanding the circumgalactic medium (CGM) distribution of galaxies is the key to revealing the dynamical exchange of materials between galaxies and their surroundings. In this work, we use DESI EDR dataset to investigate the cool CGM of galaxies ($0.3<z<1.7$) with stacking the spectra of background QSOs to obtain Mg II absorption of foreground galaxies. The equivalent width of Mg II absorption strongly correlates to stellar mass with EW(Mg II) $\propto M_{*}^{0.5}$ for star-forming galaxies with $\log M_{*}/M_{\odot} < 10$, but is independent with mass for galaxies above this mass. At given stellar mass, EW(Mg II) is larger for galaxies of higher star formation rate with impact parameter less than $50$ kpc, while showing little dependence on galaxy size. By studying the dependence on azimuthal angle, we find EW(Mg II) is strongest at the direction near the minor axis for star-forming galaxies with $\log M_{*}/M_{\odot} < 10.0$, while no dependence on azimuthal angle is seen for luminous red galaxies. This indicates that the outflow associated with star formation enhances the Mg II absorption. However, for galaxies with $\log M_{*}/M_{\odot} > 10.0$, the EW(Mg II) at the minor axis is largely suppressed with respect to low mass galaxies. This suggests that the competing processes, such as stellar feedback and gravity, play a key role in shaping the distribution of outflowing gas. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.08485v2-abstract-full').style.display = 'none'; document.getElementById('2411.08485v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 9 January, 2025; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 13 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">20 pages, 17 figures. Submitted to ApJ. Comments are welcome</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.07598">arXiv:2411.07598</a> <span> [<a href="https://arxiv.org/pdf/2411.07598">pdf</a>, <a href="https://arxiv.org/format/2411.07598">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> </div> </div> <p class="title is-5 mathjax"> Problem-Oriented Segmentation and Retrieval: Case Study on Tutoring Conversations </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Wang%2C+R+E">Rose E. Wang</a>, <a href="/search/?searchtype=author&query=Wirawarn%2C+P">Pawan Wirawarn</a>, <a href="/search/?searchtype=author&query=Lam%2C+K">Kenny Lam</a>, <a href="/search/?searchtype=author&query=Khattab%2C+O">Omar Khattab</a>, <a href="/search/?searchtype=author&query=Demszky%2C+D">Dorottya Demszky</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.07598v1-abstract-short" style="display: inline;"> Many open-ended conversations (e.g., tutoring lessons or business meetings) revolve around pre-defined reference materials, like worksheets or meeting bullets. To provide a framework for studying such conversation structure, we introduce Problem-Oriented Segmentation & Retrieval (POSR), the task of jointly breaking down conversations into segments and linking each segment to the relevant reference… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.07598v1-abstract-full').style.display = 'inline'; document.getElementById('2411.07598v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.07598v1-abstract-full" style="display: none;"> Many open-ended conversations (e.g., tutoring lessons or business meetings) revolve around pre-defined reference materials, like worksheets or meeting bullets. To provide a framework for studying such conversation structure, we introduce Problem-Oriented Segmentation & Retrieval (POSR), the task of jointly breaking down conversations into segments and linking each segment to the relevant reference item. As a case study, we apply POSR to education where effectively structuring lessons around problems is critical yet difficult. We present LessonLink, the first dataset of real-world tutoring lessons, featuring 3,500 segments, spanning 24,300 minutes of instruction and linked to 116 SAT math problems. We define and evaluate several joint and independent approaches for POSR, including segmentation (e.g., TextTiling), retrieval (e.g., ColBERT), and large language models (LLMs) methods. Our results highlight that modeling POSR as one joint task is essential: POSR methods outperform independent segmentation and retrieval pipelines by up to +76% on joint metrics and surpass traditional segmentation methods by up to +78% on segmentation metrics. We demonstrate POSR's practical impact on downstream education applications, deriving new insights on the language and time use in real-world lesson structures. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.07598v1-abstract-full').style.display = 'none'; document.getElementById('2411.07598v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 12 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">EMNLP 2024 Findings. Our code and dataset are open-sourced at https://github.com/rosewang2008/posr</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.07458">arXiv:2411.07458</a> <span> [<a href="https://arxiv.org/pdf/2411.07458">pdf</a>, <a href="https://arxiv.org/format/2411.07458">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Astrophysics of Galaxies">astro-ph.GA</span> </div> </div> <p class="title is-5 mathjax"> Size Growth on Short Timescales of Star-Forming Galaxies: Insights from Size Variation with Rest-Frame Wavelength with JADES </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Jia%2C+C">Cheng Jia</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Enci Wang</a>, <a href="/search/?searchtype=author&query=Wang%2C+H">Huiyuan Wang</a>, <a href="/search/?searchtype=author&query=Li%2C+H">Hui Li</a>, <a href="/search/?searchtype=author&query=Yao%2C+Y">Yao Yao</a>, <a href="/search/?searchtype=author&query=Song%2C+J">Jie Song</a>, <a href="/search/?searchtype=author&query=Zhang%2C+H">Hongxin Zhang</a>, <a href="/search/?searchtype=author&query=Rong%2C+Y">Yu Rong</a>, <a href="/search/?searchtype=author&query=Chen%2C+Y">Yangyao Chen</a>, <a href="/search/?searchtype=author&query=Yu%2C+H">Haoran Yu</a>, <a href="/search/?searchtype=author&query=Chen%2C+Z">Zeyu Chen</a>, <a href="/search/?searchtype=author&query=Li%2C+H">Haixin Li</a>, <a href="/search/?searchtype=author&query=Ma%2C+C">Chengyu Ma</a>, <a href="/search/?searchtype=author&query=Kong%2C+X">Xu Kong</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.07458v1-abstract-short" style="display: inline;"> We investigate size variation with rest-frame wavelength for star-forming galaxies based on the second JWST Advanced Deep Extragalactic Survey data release. Star-forming galaxies are typically smaller at longer wavelength from UV-to-NIR at $z<3.5$, especially for more massive galaxies, indicating the inside-out assembly with in-situ star formation if ignoring dust attenuation. The size variation w… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.07458v1-abstract-full').style.display = 'inline'; document.getElementById('2411.07458v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.07458v1-abstract-full" style="display: none;"> We investigate size variation with rest-frame wavelength for star-forming galaxies based on the second JWST Advanced Deep Extragalactic Survey data release. Star-forming galaxies are typically smaller at longer wavelength from UV-to-NIR at $z<3.5$, especially for more massive galaxies, indicating the inside-out assembly with in-situ star formation if ignoring dust attenuation. The size variation with wavelength shows strong dependence on stellar mass, and shows little or no dependence on redshift, specific star formation rate and galaxy environment. This suggests that the size growth of star-forming galaxies is a self-regulated process primarily governed by stellar mass. We model size as a function of both mass and redshift simultaneously, obtaining $R_{\rm e} \propto M_*^{0.23} (1+z)^{-1.04}$ at a wavelength of 0.45 ${渭\mathrm{m}}$, and $R_{\rm e} \propto M_*^{0.20} (1+z)^{-1.08}$ at 1.0 ${渭\mathrm{m}}$. Based on this size evolution and the star formation main sequence from the literature, we obtain the locus of typical size growth for individual galaxies of different masses on the mass-size plane. The moving trend of galaxies on the mass-size plane, which indicates the slopes of their locus, strongly correlates with the size ratio between 0.45 ${渭\mathrm{m}}$ and 1.0 ${渭\mathrm{m}}$, supporting the idea that the size variation with wavelength provides important information on size growth of galaxies on short timescales. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.07458v1-abstract-full').style.display = 'none'; document.getElementById('2411.07458v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Accepted for publication in ApJ, 19 pages, 11 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.07134">arXiv:2411.07134</a> <span> [<a href="https://arxiv.org/pdf/2411.07134">pdf</a>, <a href="https://arxiv.org/format/2411.07134">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Optimization and Control">math.OC</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Probability">math.PR</span> </div> </div> <p class="title is-5 mathjax"> Zero-sum Dynkin games under common and independent Poisson constraints </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Hobson%2C+D">David Hobson</a>, <a href="/search/?searchtype=author&query=Liang%2C+G">Gechun Liang</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Edward Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.07134v1-abstract-short" style="display: inline;"> Zero-sum Dynkin games under the Poisson constraint have been studied widely in the recent literature. In such a game the players are only allowed to stop at the event times of a Poisson process. The constraint can be modelled in two different ways: either both players share the same Poisson process (the common constraint) or each player has her own Poisson process (the independent constraint). In… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.07134v1-abstract-full').style.display = 'inline'; document.getElementById('2411.07134v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.07134v1-abstract-full" style="display: none;"> Zero-sum Dynkin games under the Poisson constraint have been studied widely in the recent literature. In such a game the players are only allowed to stop at the event times of a Poisson process. The constraint can be modelled in two different ways: either both players share the same Poisson process (the common constraint) or each player has her own Poisson process (the independent constraint). In the Markovian case where the payoff is given by a pair of functions of an underlying diffusion, we give sufficient conditions under which the solution of the game (the value function, and the optimal stopping sets for each player) under the common (respectively, independent) constraint is also the solution of the game under the independent (respectively, common) constraint. Roughly speaking, if the stopping sets of the maximiser and minimiser in the game under the common constraint are disjoint, then the solution to the game is the same under both the common and the independent constraint. However, the fact that the stopping sets are disjoint in the game under the independent constraint, is not sufficient to guarantee that the solution of the game under the independent constraint is also the solution under the common constraint. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.07134v1-abstract-full').style.display = 'none'; document.getElementById('2411.07134v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">25 pages</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">MSC Class:</span> 60G40; 91A05; 49L20 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.06821">arXiv:2411.06821</a> <span> [<a href="https://arxiv.org/pdf/2411.06821">pdf</a>, <a href="https://arxiv.org/format/2411.06821">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> The Boundary Effect of QGP Droplet and Self-similarity Effect of Hadrons on QGP-hadron Phase Transition </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Dai%2C+T">Tingting Dai</a>, <a href="/search/?searchtype=author&query=Ding%2C+H">Huiqiang Ding</a>, <a href="/search/?searchtype=author&query=Cheng%2C+L">Luan Cheng</a>, <a href="/search/?searchtype=author&query=Zhang%2C+W">Weining Zhang</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Enke Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.06821v1-abstract-short" style="display: inline;"> We investigate the boundary effect of QGP droplet and self-similarity effect of hadrons on QGP-hadron phase transition. In intermediate or low energy collisions, when the transverse momentum is below QCD scale, QGP cannot be produced. However, if the transverse momentum fluctuates to a relatively large value, small scale QGP droplet is produced. The modified MIT bag model with multiple reflection… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.06821v1-abstract-full').style.display = 'inline'; document.getElementById('2411.06821v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.06821v1-abstract-full" style="display: none;"> We investigate the boundary effect of QGP droplet and self-similarity effect of hadrons on QGP-hadron phase transition. In intermediate or low energy collisions, when the transverse momentum is below QCD scale, QGP cannot be produced. However, if the transverse momentum fluctuates to a relatively large value, small scale QGP droplet is produced. The modified MIT bag model with multiple reflection expansion method is employed to study the QGP droplet with the curved boundary effect. It is found that the energy density, entropy density and pressure of QGP with the influence are smaller than those without the influence. In hadron phase, we propose Two-Body Fractal Model (TBFM) to study the self-similarity structure, arising from the resonance, quantum correlation and interaction effects. It is observed that energy density, entropy density and pressure increase due to the self-similarity structure. We calculate the transverse momentum spectra of pions with the self-similarity structure influence, showing a good agreement with the experimental data. Considering both the boundary effect and self-similarity structure influence, our model predicts an increase in the transition temperature compared to scenarios without these two effects in HIAF energy region $2.2\sim 4.5 \,\text{GeV}$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.06821v1-abstract-full').style.display = 'none'; document.getElementById('2411.06821v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">28 pages, 9 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.02976">arXiv:2411.02976</a> <span> [<a href="https://arxiv.org/pdf/2411.02976">pdf</a>, <a href="https://arxiv.org/ps/2411.02976">ps</a>, <a href="https://arxiv.org/format/2411.02976">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> Spectrum and decay properties of the charmed mesons involving the coupled channel effects </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Hao%2C+W">Wei Hao</a>, <a href="/search/?searchtype=author&query=Sultan%2C+M+A">M. Atif Sultan</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">En Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.02976v1-abstract-short" style="display: inline;"> The mass spectrum of the charmed mesons is investigated by considering the coupled channel effects within the nonrelativistic potential model. The predicted masses of the charmed mesons are in agreement with experimental data. The strong decay properties are further analyzed within the $^3P_0$ model by using numerical wave functions obtained from nonrelativistic potential model. Based on the predi… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.02976v1-abstract-full').style.display = 'inline'; document.getElementById('2411.02976v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.02976v1-abstract-full" style="display: none;"> The mass spectrum of the charmed mesons is investigated by considering the coupled channel effects within the nonrelativistic potential model. The predicted masses of the charmed mesons are in agreement with experimental data. The strong decay properties are further analyzed within the $^3P_0$ model by using numerical wave functions obtained from nonrelativistic potential model. Based on the predicted masses and decay properties, we give a classification of the recently observed charmed states. Especially, we have effectively explained the masses and decay properties of the $D_1^*(2600)$ and $D_1^*(2760)$ by considering the $S$-$D$ mixing. Furthermore, the predicted masses and decay properties of the $2P$ wave states are helpful to search for them experimentally in future. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.02976v1-abstract-full').style.display = 'none'; document.getElementById('2411.02976v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.01700">arXiv:2411.01700</a> <span> [<a href="https://arxiv.org/pdf/2411.01700">pdf</a>, <a href="https://arxiv.org/format/2411.01700">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Chemical Physics">physics.chem-ph</span> </div> </div> <p class="title is-5 mathjax"> Attosecond Coherent Electron Motion in a Photoionized Aromatic Molecule </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Driver%2C+T">Taran Driver</a>, <a href="/search/?searchtype=author&query=Guo%2C+Z">Zhaoheng Guo</a>, <a href="/search/?searchtype=author&query=Isele%2C+E">Erik Isele</a>, <a href="/search/?searchtype=author&query=Grell%2C+G">Gilbert Grell</a>, <a href="/search/?searchtype=author&query=Ruberti%2C+M">Marco Ruberti</a>, <a href="/search/?searchtype=author&query=ONeal%2C+J+T">Jordan T. ONeal</a>, <a href="/search/?searchtype=author&query=Alexander%2C+O">Oliver Alexander</a>, <a href="/search/?searchtype=author&query=Beauvarlet%2C+S">Sandra Beauvarlet</a>, <a href="/search/?searchtype=author&query=Cesar%2C+D">David Cesar</a>, <a href="/search/?searchtype=author&query=Duris%2C+J">Joseph Duris</a>, <a href="/search/?searchtype=author&query=Garratt%2C+D">Douglas Garratt</a>, <a href="/search/?searchtype=author&query=Larsen%2C+K+A">Kirk A. Larsen</a>, <a href="/search/?searchtype=author&query=Li%2C+S">Siqi Li</a>, <a href="/search/?searchtype=author&query=Koloren%C4%8D%2C+P">P艡emysl Koloren膷</a>, <a href="/search/?searchtype=author&query=McCracken%2C+G+A">Gregory A. McCracken</a>, <a href="/search/?searchtype=author&query=Tuthill%2C+D">Daniel Tuthill</a>, <a href="/search/?searchtype=author&query=Wang%2C+Z">Zifan Wang</a>, <a href="/search/?searchtype=author&query=Berrah%2C+N">Nora Berrah</a>, <a href="/search/?searchtype=author&query=Bostedt%2C+C">Christoph Bostedt</a>, <a href="/search/?searchtype=author&query=Borne%2C+K">Kurtis Borne</a>, <a href="/search/?searchtype=author&query=Cheng%2C+X">Xinxin Cheng</a>, <a href="/search/?searchtype=author&query=DiMauro%2C+L+F">Louis F. DiMauro</a>, <a href="/search/?searchtype=author&query=Doumy%2C+G">Gilles Doumy</a>, <a href="/search/?searchtype=author&query=Franz%2C+P+L">Paris L. Franz</a>, <a href="/search/?searchtype=author&query=Kamalov%2C+A">Andrei Kamalov</a> , et al. (28 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.01700v1-abstract-short" style="display: inline;"> In molecular systems, the ultrafast motion of electrons initiates the process of chemical change. Tracking this electronic motion across molecules requires coupling attosecond time resolution to atomic-scale spatial sensitivity. In this work, we employ a pair of attosecond x-ray pulses from an x-ray free-electron laser to follow electron motion resulting from the sudden removal of an electron from… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.01700v1-abstract-full').style.display = 'inline'; document.getElementById('2411.01700v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.01700v1-abstract-full" style="display: none;"> In molecular systems, the ultrafast motion of electrons initiates the process of chemical change. Tracking this electronic motion across molecules requires coupling attosecond time resolution to atomic-scale spatial sensitivity. In this work, we employ a pair of attosecond x-ray pulses from an x-ray free-electron laser to follow electron motion resulting from the sudden removal of an electron from a prototypical aromatic system, para-aminophenol. X-ray absorption enables tracking this motion with atomic-site specificity. Our measurements are compared with state-of-the-art computational modeling, reproducing the observed response across multiple timescales. Sub-femtosecond dynamics are assigned to states undergoing non-radiative decay, while few-femtosecond oscillatory motion is associated with electronic wavepacket motion in stable cation states, that will eventually couple to nuclear motion. Our work provides insight on the ultrafast charge motion preceding and initiating chemical transformations in moderately complex systems, and provides a powerful benchmark for computational models of ultrafast charge motion in matter. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.01700v1-abstract-full').style.display = 'none'; document.getElementById('2411.01700v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 3 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2411.00958">arXiv:2411.00958</a> <span> [<a href="https://arxiv.org/pdf/2411.00958">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Materials Science">cond-mat.mtrl-sci</span> </div> </div> <p class="title is-5 mathjax"> Computational investigation of formation enthalpies and phase stability for rare earth oxyphosphates </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Wang%2C+E+X">Edric X. Wang</a>, <a href="/search/?searchtype=author&query=Wang%2C+L">Ligen Wang</a>, <a href="/search/?searchtype=author&query=Hong%2C+Q">Qi-Jun Hong</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2411.00958v1-abstract-short" style="display: inline;"> Rare earth phosphates have garnered significant interest due to their versatile properties, including high chemical stability, thermal resistance, luminescence, and the ability to adopt various crystalline structures. Density functional theory (DFT)-based ab initio methods have become essential tools for complementing experimental studies. In this paper, we performed DFT calculations on rare earth… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.00958v1-abstract-full').style.display = 'inline'; document.getElementById('2411.00958v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.00958v1-abstract-full" style="display: none;"> Rare earth phosphates have garnered significant interest due to their versatile properties, including high chemical stability, thermal resistance, luminescence, and the ability to adopt various crystalline structures. Density functional theory (DFT)-based ab initio methods have become essential tools for complementing experimental studies. In this paper, we performed DFT calculations on rare earth (RE; here considered as lanthanides + Y) oxyphosphates to examine their formation enthalpies and phase stability. The calculations were conducted using the GGA-PBE and r2SCAN exchange-correlation functionals. Our results indicate that both functionals predict similar phase stabilities for REPO4 and RE3PO7. However, the r2SCAN functional provides significantly more accurate formation enthalpies for the monazite and xenotime REPO4, aligning closely with experimental data. Furthermore, the inclusion of lattice vibrational entropy enhances the free energy predictions, leading to improved agreement with experimental observations on phase stability. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.00958v1-abstract-full').style.display = 'none'; document.getElementById('2411.00958v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 1 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.22485">arXiv:2410.22485</a> <span> [<a href="https://arxiv.org/pdf/2410.22485">pdf</a>, <a href="https://arxiv.org/format/2410.22485">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="General Relativity and Quantum Cosmology">gr-qc</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Cosmology and Nongalactic Astrophysics">astro-ph.CO</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</span> </div> </div> <p class="title is-5 mathjax"> Quantum Cosmology on Quantum Computer </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Wang%2C+C+E">Chih-Chien Erich Wang</a>, <a href="/search/?searchtype=author&query=Wu%2C+J+P">Jiun-Huei Proty Wu</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.22485v1-abstract-short" style="display: inline;"> With physical quantum computers becoming increasingly accessible, research on their applications across various fields has advanced rapidly. In this paper, we present the first study of quantum cosmology conducted on physical quantum computers, employing a newly proposed Hybrid Quantum-Classical (HQC) algorithm rather than the commonly used Variational Quantum Eigensolver (VQE). Specifically, we s… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.22485v1-abstract-full').style.display = 'inline'; document.getElementById('2410.22485v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.22485v1-abstract-full" style="display: none;"> With physical quantum computers becoming increasingly accessible, research on their applications across various fields has advanced rapidly. In this paper, we present the first study of quantum cosmology conducted on physical quantum computers, employing a newly proposed Hybrid Quantum-Classical (HQC) algorithm rather than the commonly used Variational Quantum Eigensolver (VQE). Specifically, we solve a constrained Hamiltonian equation derived by quantizing the Friedmann equation in cosmology. To solve this constraint equation, H |psi> = 0, where H is a Hamiltonian operator and |psi> = |psi(theta)> is the wave function of phase angle theta describing the cosmic quantum state, we iteratively use the quantum computer to compute the eigenvalues of <psi | H | psi>, while a classical computer manages the underlying probability density function within the Probabilistic Bisection Algorithm (PBA) to update theta until the solution of <psi | H | psi> = 0 is achieved to a desired accuracy. Executing our algorithm on IBM's quantum computers, we attain a high-precision solution for theta, achieving approximately 1 percent error. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.22485v1-abstract-full').style.display = 'none'; document.getElementById('2410.22485v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 29 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">8 pages, 4 figure</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.21834">arXiv:2410.21834</a> <span> [<a href="https://arxiv.org/pdf/2410.21834">pdf</a>, <a href="https://arxiv.org/format/2410.21834">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1674-1137/adb385">10.1088/1674-1137/adb385 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Probing the mass effect of heavy quark jets in high-energy nuclear collisions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Wang%2C+S">Sa Wang</a>, <a href="/search/?searchtype=author&query=Li%2C+S">Shuang Li</a>, <a href="/search/?searchtype=author&query=Li%2C+Y">Yao Li</a>, <a href="/search/?searchtype=author&query=Zhang%2C+B">Ben-Wei Zhang</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Enke Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.21834v2-abstract-short" style="display: inline;"> The production of heavy quark (HQ) jets provides a new arena to address the mass effect of jet quenching in heavy-ion physics. This paper presents a theoretical study of HQ jet yield suppression in Pb+Pb collisions at the LHC and focuses on the energy loss of HQ jets produced by different mechanisms. The p+p baseline is carried out by the SHERPA generator, and the jet-medium interactions are descr… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.21834v2-abstract-full').style.display = 'inline'; document.getElementById('2410.21834v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.21834v2-abstract-full" style="display: none;"> The production of heavy quark (HQ) jets provides a new arena to address the mass effect of jet quenching in heavy-ion physics. This paper presents a theoretical study of HQ jet yield suppression in Pb+Pb collisions at the LHC and focuses on the energy loss of HQ jets produced by different mechanisms. The p+p baseline is carried out by the SHERPA generator, and the jet-medium interactions are described by the SHELL transport model, which considers the elastic and inelastic partonic energy loss in the quark-gluon plasma (QGP). In p+p collisions, our numerical results indicate that the HQ jets from gluon splitting ($g \rightarrow Q$-jet) give the dominant contribution at high $p_T$, and it shows more dispersive structures than the HQ-initiated one ($Q \rightarrow Q$-jet). In nucleus-nucleus collisions, our calculations are consistent with the inclusive and b-jet $R_{AA}$ recently measured by the ATLAS collaboration, which suggests a remarkable manifestation of the mass effect of jet energy loss. As a result of the dispersive substructure, the $g \rightarrow Q$-jet will lose more energy than the $Q \rightarrow Q$-jet in the QGP. Due to the significant contribution of $g \rightarrow c$-jet, the $R_{AA}$ of c-jet will be comparable or even smaller than that of inclusive jet. To experimentally distinguish the $g \rightarrow Q$-jet and $Q \rightarrow Q$-jet, we propose the event selection strategies based on their topological features and test the performances. By isolating the $c \rightarrow c$-jet and $b \rightarrow b$-jet, the jets initiated by heavy quarks, we predict that the order of their $R_{AA}$ are in line with the mass hierarchy of energy loss. Future measurements on the $R_{AA}$ of $Q \rightarrow Q$-jet and $g \rightarrow Q$-jet will provide a unique chance to test the flavor/mass dependence of energy loss at the jet level. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.21834v2-abstract-full').style.display = 'none'; document.getElementById('2410.21834v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 12 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">12 pages, 12 figures. The version to be published in CPC</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.16181">arXiv:2410.16181</a> <span> [<a href="https://arxiv.org/pdf/2410.16181">pdf</a>, <a href="https://arxiv.org/format/2410.16181">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Search for $h_b(2P)\to纬蠂_{bJ}(1P)$ at $\sqrt{s} = 10.860$ GeV </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Belle+Collaboration"> Belle Collaboration</a>, <a href="/search/?searchtype=author&query=Boschetti%2C+A">A. Boschetti</a>, <a href="/search/?searchtype=author&query=Mussa%2C+R">R. Mussa</a>, <a href="/search/?searchtype=author&query=Tamponi%2C+U">U. Tamponi</a>, <a href="/search/?searchtype=author&query=Adachi%2C+I">I. Adachi</a>, <a href="/search/?searchtype=author&query=Aihara%2C+H">H. Aihara</a>, <a href="/search/?searchtype=author&query=Asner%2C+D+M">D. M. Asner</a>, <a href="/search/?searchtype=author&query=Aushev%2C+T">T. Aushev</a>, <a href="/search/?searchtype=author&query=Ayad%2C+R">R. Ayad</a>, <a href="/search/?searchtype=author&query=Banerjee%2C+S">Sw. Banerjee</a>, <a href="/search/?searchtype=author&query=Belous%2C+K">K. Belous</a>, <a href="/search/?searchtype=author&query=Bennett%2C+J">J. Bennett</a>, <a href="/search/?searchtype=author&query=Bessner%2C+M">M. Bessner</a>, <a href="/search/?searchtype=author&query=Biswas%2C+D">D. Biswas</a>, <a href="/search/?searchtype=author&query=Bobrov%2C+A">A. Bobrov</a>, <a href="/search/?searchtype=author&query=Bodrov%2C+D">D. Bodrov</a>, <a href="/search/?searchtype=author&query=Bozek%2C+A">A. Bozek</a>, <a href="/search/?searchtype=author&query=Bra%C4%8Dko%2C+M">M. Bra膷ko</a>, <a href="/search/?searchtype=author&query=Branchini%2C+P">P. Branchini</a>, <a href="/search/?searchtype=author&query=Browder%2C+T+E">T. E. Browder</a>, <a href="/search/?searchtype=author&query=Budano%2C+A">A. Budano</a>, <a href="/search/?searchtype=author&query=Chang%2C+M+-">M. -C. Chang</a>, <a href="/search/?searchtype=author&query=Cheon%2C+B+G">B. G. Cheon</a>, <a href="/search/?searchtype=author&query=Chilikin%2C+K">K. Chilikin</a>, <a href="/search/?searchtype=author&query=Cho%2C+K">K. Cho</a> , et al. (118 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.16181v1-abstract-short" style="display: inline;"> In the bottomonium sector, the hindered magnetic dipole (M1) transitions between P-wave states $h_b(2P) \rightarrow 蠂_{bJ}(1P) 纬$, $J=0, \, 1, \, 2$, are expected to be severely suppressed according to the Relativized Quark Model, due to the spin flip of the $b$ quark. Nevertheless, a recent model following the coupled-channel approach predicts the corresponding branching fractions to be enhanced… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.16181v1-abstract-full').style.display = 'inline'; document.getElementById('2410.16181v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.16181v1-abstract-full" style="display: none;"> In the bottomonium sector, the hindered magnetic dipole (M1) transitions between P-wave states $h_b(2P) \rightarrow 蠂_{bJ}(1P) 纬$, $J=0, \, 1, \, 2$, are expected to be severely suppressed according to the Relativized Quark Model, due to the spin flip of the $b$ quark. Nevertheless, a recent model following the coupled-channel approach predicts the corresponding branching fractions to be enhanced by orders of magnitude. In this Letter, we report the first search for such transitions. We find no significant signals and set upper limits at 90% CL on the corresponding branching fractions: $\mathcal{B}[h_b(2P)\to纬蠂_{b0}(1P)] < 2.7 \times 10^{-1}$, $\mathcal{B}[h_b(2P)\to纬蠂_{b1}(1P)] < 5.4 \times 10^{-3}$ and $\mathcal{B}[h_b(2P)\to纬蠂_{b2}(1P)] < 1.3 \times 10^{-2}$. These values help to constrain the parameters of the coupled-channel models. The results are obtained using a $121.4 \, fb^{-1}$ data sample taken around $\sqrt{s}= 10.860 \, GeV$ with the Belle detector at the KEKB asymmetric-energy $e^+e^-$ collider. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.16181v1-abstract-full').style.display = 'none'; document.getElementById('2410.16181v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> Belle Preprint 2024-07; KEK Preprint 2024-19 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.16078">arXiv:2410.16078</a> <span> [<a href="https://arxiv.org/pdf/2410.16078">pdf</a>, <a href="https://arxiv.org/format/2410.16078">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> The $螞_c^+\to畏蟺^+螞$ reaction and the $螞a_0^+(980)$ and $蟺^+螞(1670)$ contributions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Duan%2C+M">Man-Yu Duan</a>, <a href="/search/?searchtype=author&query=Lyu%2C+W">Wen-Tao Lyu</a>, <a href="/search/?searchtype=author&query=Xiao%2C+C">Chu-Wen Xiao</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">En Wang</a>, <a href="/search/?searchtype=author&query=Xie%2C+J">Ju-Jun Xie</a>, <a href="/search/?searchtype=author&query=Chen%2C+D">Dian-Yong Chen</a>, <a href="/search/?searchtype=author&query=Oset%2C+E">Eulogio Oset</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.16078v2-abstract-short" style="display: inline;"> We study from the theoretical point of view the $螞_c^+\to 蟺^+ 畏螞$ reaction, recently measured by the Belle and BESIII Collaborations, where clear signals are observed for $a_0(980)$, $螞(1670)$, and $危(1385)$ excitation. By considering the $a_0(980)$ and $螞(1670)$ as dynamically generated resonances from the meson meson and meson baryon interaction, respectively, we are able to determine their rela… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.16078v2-abstract-full').style.display = 'inline'; document.getElementById('2410.16078v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.16078v2-abstract-full" style="display: none;"> We study from the theoretical point of view the $螞_c^+\to 蟺^+ 畏螞$ reaction, recently measured by the Belle and BESIII Collaborations, where clear signals are observed for $a_0(980)$, $螞(1670)$, and $危(1385)$ excitation. By considering the $a_0(980)$ and $螞(1670)$ as dynamically generated resonances from the meson meson and meson baryon interaction, respectively, we are able to determine their relative production strength in the reaction, which is also tied to the strength of the $蟺^+ 畏螞$ tree level contribution. We observe that this latter strength is very big and there are large destructive interferences between the tree level and the rescattering terms where the $a_0(980)$ and $螞(1670)$ are generated. The $危(1385)$ contribution is included by means of a free parameter, the only one of the theory, up to a global normalization, when one considers only external emission, and we observe that the spin flip part of this term, usually ignored in theoretical and experimental works, plays an important role determining the shape of the mass distributions. Internal emission is also considered and it is found to play a minor role. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.16078v2-abstract-full').style.display = 'none'; document.getElementById('2410.16078v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 22 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 21 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.15449">arXiv:2410.15449</a> <span> [<a href="https://arxiv.org/pdf/2410.15449">pdf</a>, <a href="https://arxiv.org/format/2410.15449">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> </div> </div> <p class="title is-5 mathjax"> Heterogeneous Graph Reinforcement Learning for Dependency-aware Multi-task Allocation in Spatial Crowdsourcing </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Zhao%2C+Y">Yong Zhao</a>, <a href="/search/?searchtype=author&query=Zhu%2C+Z">Zhengqiu Zhu</a>, <a href="/search/?searchtype=author&query=Gao%2C+C">Chen Gao</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">En Wang</a>, <a href="/search/?searchtype=author&query=Huang%2C+J">Jincai Huang</a>, <a href="/search/?searchtype=author&query=Wang%2C+F">Fei-Yue Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.15449v1-abstract-short" style="display: inline;"> Spatial Crowdsourcing (SC) is gaining traction in both academia and industry, with tasks on SC platforms becoming increasingly complex and requiring collaboration among workers with diverse skills. Recent research works address complex tasks by dividing them into subtasks with dependencies and assigning them to suitable workers. However, the dependencies among subtasks and their heterogeneous skil… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.15449v1-abstract-full').style.display = 'inline'; document.getElementById('2410.15449v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.15449v1-abstract-full" style="display: none;"> Spatial Crowdsourcing (SC) is gaining traction in both academia and industry, with tasks on SC platforms becoming increasingly complex and requiring collaboration among workers with diverse skills. Recent research works address complex tasks by dividing them into subtasks with dependencies and assigning them to suitable workers. However, the dependencies among subtasks and their heterogeneous skill requirements, as well as the need for efficient utilization of workers' limited work time in the multi-task allocation mode, pose challenges in achieving an optimal task allocation scheme. Therefore, this paper formally investigates the problem of Dependency-aware Multi-task Allocation (DMA) and presents a well-designed framework to solve it, known as Heterogeneous Graph Reinforcement Learning-based Task Allocation (HGRL-TA). To address the challenges associated with representing and embedding diverse problem instances to ensure robust generalization, we propose a multi-relation graph model and a Compound-path-based Heterogeneous Graph Attention Network (CHANet) for effectively representing and capturing intricate relations among tasks and workers, as well as providing embedding of problem state. The task allocation decision is determined sequentially by a policy network, which undergoes simultaneous training with CHANet using the proximal policy optimization algorithm. Extensive experiment results demonstrate the effectiveness and generality of the proposed HGRL-TA in solving the DMA problem, leading to average profits that is 21.78% higher than those achieved using the metaheuristic methods. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.15449v1-abstract-full').style.display = 'none'; document.getElementById('2410.15449v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.14979">arXiv:2410.14979</a> <span> [<a href="https://arxiv.org/pdf/2410.14979">pdf</a>, <a href="https://arxiv.org/format/2410.14979">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Machine Learning">cs.LG</span> </div> </div> <p class="title is-5 mathjax"> Do Large Language Models Truly Grasp Mathematics? An Empirical Exploration From Cognitive Psychology </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Xie%2C+W">Wei Xie</a>, <a href="/search/?searchtype=author&query=Ma%2C+S">Shuoyoucheng Ma</a>, <a href="/search/?searchtype=author&query=Wang%2C+Z">Zhenhua Wang</a>, <a href="/search/?searchtype=author&query=Wang%2C+E">Enze Wang</a>, <a href="/search/?searchtype=author&query=Chen%2C+K">Kai Chen</a>, <a href="/search/?searchtype=author&query=Sun%2C+X">Xiaobing Sun</a>, <a href="/search/?searchtype=author&query=Wang%2C+B">Baosheng Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.14979v5-abstract-short" style="display: inline;"> The cognitive mechanism by which Large Language Models (LLMs) solve mathematical problems remains a widely debated and unresolved issue. Currently, there is little interpretable experimental evidence that connects LLMs' problem-solving with human cognitive psychology.To determine if LLMs possess human-like mathematical reasoning, we modified the problems used in the human Cognitive Reflection Test… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.14979v5-abstract-full').style.display = 'inline'; document.getElementById('2410.14979v5-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.14979v5-abstract-full" style="display: none;"> The cognitive mechanism by which Large Language Models (LLMs) solve mathematical problems remains a widely debated and unresolved issue. Currently, there is little interpretable experimental evidence that connects LLMs' problem-solving with human cognitive psychology.To determine if LLMs possess human-like mathematical reasoning, we modified the problems used in the human Cognitive Reflection Test (CRT). Our results show that, even with the use of Chains of Thought (CoT) prompts, mainstream LLMs, including the latest o1 model (noted for its reasoning capabilities), have a high error rate when solving these modified CRT problems. Specifically, the average accuracy rate dropped by up to 50% compared to the original questions.Further analysis of LLMs' incorrect answers suggests that they primarily rely on pattern matching from their training data, which aligns more with human intuition (System 1 thinking) rather than with human-like reasoning (System 2 thinking). This finding challenges the belief that LLMs have genuine mathematical reasoning abilities comparable to humans. As a result, this work may adjust overly optimistic views on LLMs' progress towards artificial general intelligence. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.14979v5-abstract-full').style.display = 'none'; document.getElementById('2410.14979v5-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 15 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 19 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.12836">arXiv:2410.12836</a> <span> [<a href="https://arxiv.org/pdf/2410.12836">pdf</a>, <a href="https://arxiv.org/format/2410.12836">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Graphics">cs.GR</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computer Vision and Pattern Recognition">cs.CV</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Human-Computer Interaction">cs.HC</span> </div> </div> <p class="title is-5 mathjax"> EditRoom: LLM-parameterized Graph Diffusion for Composable 3D Room Layout Editing </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Zheng%2C+K">Kaizhi Zheng</a>, <a href="/search/?searchtype=author&query=Chen%2C+X">Xiaotong Chen</a>, <a href="/search/?searchtype=author&query=He%2C+X">Xuehai He</a>, <a href="/search/?searchtype=author&query=Gu%2C+J">Jing Gu</a>, <a href="/search/?searchtype=author&query=Li%2C+L">Linjie Li</a>, <a href="/search/?searchtype=author&query=Yang%2C+Z">Zhengyuan Yang</a>, <a href="/search/?searchtype=author&query=Lin%2C+K">Kevin Lin</a>, <a href="/search/?searchtype=author&query=Wang%2C+J">Jianfeng Wang</a>, <a href="/search/?searchtype=author&query=Wang%2C+L">Lijuan Wang</a>, <a href="/search/?searchtype=author&query=Wang%2C+X+E">Xin Eric Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.12836v1-abstract-short" style="display: inline;"> Given the steep learning curve of professional 3D software and the time-consuming process of managing large 3D assets, language-guided 3D scene editing has significant potential in fields such as virtual reality, augmented reality, and gaming. However, recent approaches to language-guided 3D scene editing either require manual interventions or focus only on appearance modifications without support… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.12836v1-abstract-full').style.display = 'inline'; document.getElementById('2410.12836v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.12836v1-abstract-full" style="display: none;"> Given the steep learning curve of professional 3D software and the time-consuming process of managing large 3D assets, language-guided 3D scene editing has significant potential in fields such as virtual reality, augmented reality, and gaming. However, recent approaches to language-guided 3D scene editing either require manual interventions or focus only on appearance modifications without supporting comprehensive scene layout changes. In response, we propose Edit-Room, a unified framework capable of executing a variety of layout edits through natural language commands, without requiring manual intervention. Specifically, EditRoom leverages Large Language Models (LLMs) for command planning and generates target scenes using a diffusion-based method, enabling six types of edits: rotate, translate, scale, replace, add, and remove. To address the lack of data for language-guided 3D scene editing, we have developed an automatic pipeline to augment existing 3D scene synthesis datasets and introduced EditRoom-DB, a large-scale dataset with 83k editing pairs, for training and evaluation. Our experiments demonstrate that our approach consistently outperforms other baselines across all metrics, indicating higher accuracy and coherence in language-guided scene layout editing. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.12836v1-abstract-full').style.display = 'none'; document.getElementById('2410.12836v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 3 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.09988">arXiv:2410.09988</a> <span> [<a href="https://arxiv.org/pdf/2410.09988">pdf</a>, <a href="https://arxiv.org/format/2410.09988">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Machine Learning">cs.LG</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> </div> </div> <p class="title is-5 mathjax"> HARDMath: A Benchmark Dataset for Challenging Problems in Applied Mathematics </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Fan%2C+J">Jingxuan Fan</a>, <a href="/search/?searchtype=author&query=Martinson%2C+S">Sarah Martinson</a>, <a href="/search/?searchtype=author&query=Wang%2C+E+Y">Erik Y. Wang</a>, <a href="/search/?searchtype=author&query=Hausknecht%2C+K">Kaylie Hausknecht</a>, <a href="/search/?searchtype=author&query=Brenner%2C+J">Jonah Brenner</a>, <a href="/search/?searchtype=author&query=Liu%2C+D">Danxian Liu</a>, <a href="/search/?searchtype=author&query=Peng%2C+N">Nianli Peng</a>, <a href="/search/?searchtype=author&query=Wang%2C+C">Corey Wang</a>, <a href="/search/?searchtype=author&query=Brenner%2C+M+P">Michael P. Brenner</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.09988v2-abstract-short" style="display: inline;"> Advanced applied mathematics problems are underrepresented in existing Large Language Model (LLM) benchmark datasets. To address this, we introduce HARDMath, a dataset inspired by a graduate course on asymptotic methods, featuring challenging applied mathematics problems that require analytical approximation techniques. These problems demand a combination of mathematical reasoning, computational t… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.09988v2-abstract-full').style.display = 'inline'; document.getElementById('2410.09988v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.09988v2-abstract-full" style="display: none;"> Advanced applied mathematics problems are underrepresented in existing Large Language Model (LLM) benchmark datasets. To address this, we introduce HARDMath, a dataset inspired by a graduate course on asymptotic methods, featuring challenging applied mathematics problems that require analytical approximation techniques. These problems demand a combination of mathematical reasoning, computational tools, and subjective judgment, making them difficult for LLMs. Our framework auto-generates a large number of problems with solutions validated against numerical ground truths. We evaluate both open- and closed-source LLMs on HARDMath-mini, a sub-sampled test set of 366 problems, as well as on 40 word problems formulated in applied science contexts. Even leading closed-source models like GPT-4 achieve only 43.8% overall accuracy with few-shot Chain-of-Thought prompting, and all models demonstrate significantly lower performance compared to results on existing mathematics benchmark datasets. We additionally conduct a detailed error analysis to gain insights into the failure cases of LLMs. These results demonstrate limitations of current LLM performance on advanced graduate-level applied math problems and underscore the importance of datasets like HARDMath to advance mathematical abilities of LLMs. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.09988v2-abstract-full').style.display = 'none'; document.getElementById('2410.09988v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 13 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 13 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Code and the HARDMath dataset is available at https://github.com/sarahmart/HARDMath</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.09377">arXiv:2410.09377</a> <span> [<a href="https://arxiv.org/pdf/2410.09377">pdf</a>, <a href="https://arxiv.org/format/2410.09377">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Computer Vision and Pattern Recognition">cs.CV</span> </div> </div> <p class="title is-5 mathjax"> GEM-VPC: A dual Graph-Enhanced Multimodal integration for Video Paragraph Captioning </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Wang%2C+E">Eileen Wang</a>, <a href="/search/?searchtype=author&query=Han%2C+C">Caren Han</a>, <a href="/search/?searchtype=author&query=Poon%2C+J">Josiah Poon</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.09377v1-abstract-short" style="display: inline;"> Video Paragraph Captioning (VPC) aims to generate paragraph captions that summarises key events within a video. Despite recent advancements, challenges persist, notably in effectively utilising multimodal signals inherent in videos and addressing the long-tail distribution of words. The paper introduces a novel multimodal integrated caption generation framework for VPC that leverages information f… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.09377v1-abstract-full').style.display = 'inline'; document.getElementById('2410.09377v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.09377v1-abstract-full" style="display: none;"> Video Paragraph Captioning (VPC) aims to generate paragraph captions that summarises key events within a video. Despite recent advancements, challenges persist, notably in effectively utilising multimodal signals inherent in videos and addressing the long-tail distribution of words. The paper introduces a novel multimodal integrated caption generation framework for VPC that leverages information from various modalities and external knowledge bases. Our framework constructs two graphs: a 'video-specific' temporal graph capturing major events and interactions between multimodal information and commonsense knowledge, and a 'theme graph' representing correlations between words of a specific theme. These graphs serve as input for a transformer network with a shared encoder-decoder architecture. We also introduce a node selection module to enhance decoding efficiency by selecting the most relevant nodes from the graphs. Our results demonstrate superior performance across benchmark datasets. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.09377v1-abstract-full').style.display = 'none'; document.getElementById('2410.09377v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 12 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.08164">arXiv:2410.08164</a> <span> [<a href="https://arxiv.org/pdf/2410.08164">pdf</a>, <a href="https://arxiv.org/format/2410.08164">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computer Vision and Pattern Recognition">cs.CV</span> </div> </div> <p class="title is-5 mathjax"> Agent S: An Open Agentic Framework that Uses Computers Like a Human </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Agashe%2C+S">Saaket Agashe</a>, <a href="/search/?searchtype=author&query=Han%2C+J">Jiuzhou Han</a>, <a href="/search/?searchtype=author&query=Gan%2C+S">Shuyu Gan</a>, <a href="/search/?searchtype=author&query=Yang%2C+J">Jiachen Yang</a>, <a href="/search/?searchtype=author&query=Li%2C+A">Ang Li</a>, <a href="/search/?searchtype=author&query=Wang%2C+X+E">Xin Eric Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.08164v1-abstract-short" style="display: inline;"> We present Agent S, an open agentic framework that enables autonomous interaction with computers through a Graphical User Interface (GUI), aimed at transforming human-computer interaction by automating complex, multi-step tasks. Agent S aims to address three key challenges in automating computer tasks: acquiring domain-specific knowledge, planning over long task horizons, and handling dynamic, non… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.08164v1-abstract-full').style.display = 'inline'; document.getElementById('2410.08164v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.08164v1-abstract-full" style="display: none;"> We present Agent S, an open agentic framework that enables autonomous interaction with computers through a Graphical User Interface (GUI), aimed at transforming human-computer interaction by automating complex, multi-step tasks. Agent S aims to address three key challenges in automating computer tasks: acquiring domain-specific knowledge, planning over long task horizons, and handling dynamic, non-uniform interfaces. To this end, Agent S introduces experience-augmented hierarchical planning, which learns from external knowledge search and internal experience retrieval at multiple levels, facilitating efficient task planning and subtask execution. In addition, it employs an Agent-Computer Interface (ACI) to better elicit the reasoning and control capabilities of GUI agents based on Multimodal Large Language Models (MLLMs). Evaluation on the OSWorld benchmark shows that Agent S outperforms the baseline by 9.37% on success rate (an 83.6% relative improvement) and achieves a new state-of-the-art. Comprehensive analysis highlights the effectiveness of individual components and provides insights for future improvements. Furthermore, Agent S demonstrates broad generalizability to different operating systems on a newly-released WindowsAgentArena benchmark. Code available at https://github.com/simular-ai/Agent-S. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.08164v1-abstract-full').style.display = 'none'; document.getElementById('2410.08164v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">23 pages, 16 figures, 9 tables</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.07000">arXiv:2410.07000</a> <span> [<a href="https://arxiv.org/pdf/2410.07000">pdf</a>, <a href="https://arxiv.org/format/2410.07000">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Mesoscale and Nanoscale Physics">cond-mat.mes-hall</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevB.111.075114">10.1103/PhysRevB.111.075114 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Higher-Order Van Hove Singularities in Kagome Topological Bands </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Wang%2C+E">Edrick Wang</a>, <a href="/search/?searchtype=author&query=Pullasseri%2C+L">Lakshmi Pullasseri</a>, <a href="/search/?searchtype=author&query=Santos%2C+L+H">Luiz H. Santos</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.07000v3-abstract-short" style="display: inline;"> Motivated by the growing interest in band structures featuring higher-order Van Hove singularities (HOVHS), we investigate a spinless fermion kagome system characterized by nearest-neighbor (NN) and next-nearest-neighbor (NNN) hopping amplitudes. While NN hopping preserves time-reversal symmetry, NNN hopping, akin to chiral hopping on the Haldane lattice, breaks time-reversal symmetry and leads to… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.07000v3-abstract-full').style.display = 'inline'; document.getElementById('2410.07000v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.07000v3-abstract-full" style="display: none;"> Motivated by the growing interest in band structures featuring higher-order Van Hove singularities (HOVHS), we investigate a spinless fermion kagome system characterized by nearest-neighbor (NN) and next-nearest-neighbor (NNN) hopping amplitudes. While NN hopping preserves time-reversal symmetry, NNN hopping, akin to chiral hopping on the Haldane lattice, breaks time-reversal symmetry and leads to the formation of topological bands with Chern numbers ranging from $C = \pm 1$ to $ \pm 4$. We perform analytical and numerical analysis of the energy bands near the high-symmetry points $\boldsymbol螕$, $\pm \boldsymbol{K}$, and $\boldsymbol{M_i}$ ($i=1,2,$ and $3$), which uncover a rich and complex landscape of HOVHS, controlled by the magnitude and phase of the NNN hopping. We observe power-law divergences in the density of states (DOS), $蟻(蔚) \sim |蔚|^{-谓}$, with exponents $谓= 1/2, 1/3, 1/4$, which can significantly affect the anomalous Hall response at low temperatures when the Fermi level crosses the HOVHS. Additionally, the NNN hopping induces the formation of higher Chern number bands $C = \pm 2, \pm 4$ in the middle of the spectrum obeying a sublattice interference whereupon electronic states are maximally localized in each of the sublattices when the momentum approaches the three high-symmetry points $\boldsymbol{M_i}$ ($i=1,2,$ and $3$) on the Brillouin zone boundary. This classification of HOVHS in kagome systems provides a platform to explore unconventional electronic orders induced by electronic correlations. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.07000v3-abstract-full').style.display = 'none'; document.getElementById('2410.07000v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 8 February, 2025; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 9 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">11 pages, 7 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> E. Wang, L. Pullasseri, and L. H. Santos, Higher-order Van-Hove singularities in kagome topological bands, Phys. Rev. B 111, 075114 (2025) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2410.06172">arXiv:2410.06172</a> <span> [<a href="https://arxiv.org/pdf/2410.06172">pdf</a>, <a href="https://arxiv.org/format/2410.06172">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Artificial Intelligence">cs.AI</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computation and Language">cs.CL</span> </div> </div> <p class="title is-5 mathjax"> Multimodal Situational Safety </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/?searchtype=author&query=Zhou%2C+K">Kaiwen Zhou</a>, <a href="/search/?searchtype=author&query=Liu%2C+C">Chengzhi Liu</a>, <a href="/search/?searchtype=author&query=Zhao%2C+X">Xuandong Zhao</a>, <a href="/search/?searchtype=author&query=Compalas%2C+A">Anderson Compalas</a>, <a href="/search/?searchtype=author&query=Song%2C+D">Dawn Song</a>, <a href="/search/?searchtype=author&query=Wang%2C+X+E">Xin Eric Wang</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2410.06172v1-abstract-short" style="display: inline;"> Multimodal Large Language Models (MLLMs) are rapidly evolving, demonstrating impressive capabilities as multimodal assistants that interact with both humans and their environments. However, this increased sophistication introduces significant safety concerns. In this paper, we present the first evaluation and analysis of a novel safety challenge termed Multimodal Situational Safety, which explores… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.06172v1-abstract-full').style.display = 'inline'; document.getElementById('2410.06172v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2410.06172v1-abstract-full" style="display: none;"> Multimodal Large Language Models (MLLMs) are rapidly evolving, demonstrating impressive capabilities as multimodal assistants that interact with both humans and their environments. However, this increased sophistication introduces significant safety concerns. In this paper, we present the first evaluation and analysis of a novel safety challenge termed Multimodal Situational Safety, which explores how safety considerations vary based on the specific situation in which the user or agent is engaged. We argue that for an MLLM to respond safely, whether through language or action, it often needs to assess the safety implications of a language query within its corresponding visual context. To evaluate this capability, we develop the Multimodal Situational Safety benchmark (MSSBench) to assess the situational safety performance of current MLLMs. The dataset comprises 1,820 language query-image pairs, half of which the image context is safe, and the other half is unsafe. We also develop an evaluation framework that analyzes key safety aspects, including explicit safety reasoning, visual understanding, and, crucially, situational safety reasoning. Our findings reveal that current MLLMs struggle with this nuanced safety problem in the instruction-following setting and struggle to tackle these situational safety challenges all at once, highlighting a key area for future research. Furthermore, we develop multi-agent pipelines to coordinately solve safety challenges, which shows consistent improvement in safety over the original MLLM response. Code and data: mssbench.github.io. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2410.06172v1-abstract-full').style.display = 'none'; document.getElementById('2410.06172v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 8 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2024. </p> </li> </ol> <nav class="pagination is-small is-centered breathe-horizontal" role="navigation" aria-label="pagination"> <a href="" class="pagination-previous is-invisible">Previous </a> <a href="/search/?searchtype=author&query=Wang%2C+E&start=50" class="pagination-next" >Next </a> <ul class="pagination-list"> <li> <a href="/search/?searchtype=author&query=Wang%2C+E&start=0" class="pagination-link is-current" aria-label="Goto page 1">1 </a> </li> <li> <a 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