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class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Towards a new generation of solid total-energy detectors for neutron-capture time-of-flight experiments with intense neutron beams </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Balibrea-Correa%2C+J">J. Balibrea-Correa</a>, <a href="/search/physics?searchtype=author&amp;query=Babiano-Suarez%2C+V">V. Babiano-Suarez</a>, <a href="/search/physics?searchtype=author&amp;query=Lerendegui-Marco%2C+J">J. Lerendegui-Marco</a>, <a href="/search/physics?searchtype=author&amp;query=Domingo-Pardo%2C+C">C. Domingo-Pardo</a>, <a href="/search/physics?searchtype=author&amp;query=Ladarescu%2C+I">I. Ladarescu</a>, <a href="/search/physics?searchtype=author&amp;query=Tarife%C3%B1o-Saldivia%2C+A">A. Tarife帽o-Saldivia</a>, <a href="/search/physics?searchtype=author&amp;query=de+la+Fuente-Rosales%2C+G">G. de la Fuente-Rosales</a>, <a href="/search/physics?searchtype=author&amp;query=Gameiro%2C+B">B. Gameiro</a>, <a href="/search/physics?searchtype=author&amp;query=Zaitseva%2C+N">N. Zaitseva</a>, <a href="/search/physics?searchtype=author&amp;query=Alcayne%2C+V">V. Alcayne</a>, <a href="/search/physics?searchtype=author&amp;query=Cano-Ott%2C+D">D. Cano-Ott</a>, <a href="/search/physics?searchtype=author&amp;query=Gonz%C3%A1lez-Romero%2C+E">E. Gonz谩lez-Romero</a>, <a href="/search/physics?searchtype=author&amp;query=Mart%C3%ADnez%2C+T">T. Mart铆nez</a>, <a href="/search/physics?searchtype=author&amp;query=Mendoza%2C+E">E. Mendoza</a>, <a href="/search/physics?searchtype=author&amp;query=de+Rada%2C+A+P">A. P茅rez de Rada</a>, <a href="/search/physics?searchtype=author&amp;query=del+Olmo%2C+J+P">J. Plaza del Olmo</a>, <a href="/search/physics?searchtype=author&amp;query=S%C3%A1nchez-Caballero%2C+A">A. S谩nchez-Caballero</a>, <a href="/search/physics?searchtype=author&amp;query=Casanovas%2C+A">A. Casanovas</a>, <a href="/search/physics?searchtype=author&amp;query=Calvi%C3%B1o%2C+F">F. Calvi帽o</a>, <a href="/search/physics?searchtype=author&amp;query=Valenta%2C+S">S. Valenta</a>, <a href="/search/physics?searchtype=author&amp;query=Aberle%2C+O">O. Aberle</a>, <a href="/search/physics?searchtype=author&amp;query=Altieri%2C+S">S. Altieri</a>, <a href="/search/physics?searchtype=author&amp;query=Amaducci%2C+S">S. Amaducci</a>, <a href="/search/physics?searchtype=author&amp;query=Andrzejewski%2C+J">J. Andrzejewski</a>, <a href="/search/physics?searchtype=author&amp;query=Bacak%2C+M">M. Bacak</a> , et al. (112 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="2411.18969v1-abstract-short" style="display: inline;"> Challenging neutron-capture cross-section measurements of small cross sections and samples with a very limited number of atoms require high-flux time-of-flight facilities. In turn, such facilities need innovative detection setups that are fast, have low sensitivity to neutrons, can quickly recover from the so-called $纬$-flash, and offer the highest possible detection sensitivity. In this paper, we&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.18969v1-abstract-full').style.display = 'inline'; document.getElementById('2411.18969v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.18969v1-abstract-full" style="display: none;"> Challenging neutron-capture cross-section measurements of small cross sections and samples with a very limited number of atoms require high-flux time-of-flight facilities. In turn, such facilities need innovative detection setups that are fast, have low sensitivity to neutrons, can quickly recover from the so-called $纬$-flash, and offer the highest possible detection sensitivity. In this paper, we present several steps toward such advanced systems. Specifically, we describe the performance of a high-sensitivity experimental setup at CERN n\_TOF EAR2. It consists of nine sTED detector modules in a compact cylindrical configuration, two conventional used large-volume C$_{6}$D$_{6}$ detectors, and one LaCl$_{3}$(Ce) detector. The performance of these detection systems is compared using $^{93}$Nb($n$,$纬$) data. We also developed a detailed \textsc{Geant4} Monte Carlo model of the experimental EAR2 setup, which allows for a better understanding of the detector features, including their efficiency determination. This Monte Carlo model has been used for further optimization, thus leading to a new conceptual design of a $纬$ detector array, STAR, based on a deuterated-stilbene crystal array. Finally, the suitability of deuterated-stilbene crystals for the future STAR array is investigaged experimentally utilizing a small stilbene-d12 prototype. The results suggest a similar or superior performance of STAR with respect to other setups based on liquid-scintillators, and allow for additional features such as neutron-gamma discrimination and a higher level of customization capability. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.18969v1-abstract-full').style.display = 'none'; document.getElementById('2411.18969v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 28 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/2411.01900">arXiv:2411.01900</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2411.01900">pdf</a>]&nbsp;</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"> Exploring Different Search Approaches to Discover Donor Molecules for Organic Solar Cells </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Azzouzi%2C+M">Mohammed Azzouzi</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S">Steven Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Posligua%2C+V">Victor Posligua</a>, <a href="/search/physics?searchtype=author&amp;query=Bondesan%2C+R">Roberto Bondesan</a>, <a href="/search/physics?searchtype=author&amp;query=Zwijnenburg%2C+M+A">Martijn A. Zwijnenburg</a>, <a href="/search/physics?searchtype=author&amp;query=Jelfs%2C+K+E">Kim E. Jelfs</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="2411.01900v2-abstract-short" style="display: inline;"> Identifying organic molecules with desirable properties from the extensive chemical space can be challenging, particularly when property evaluation methods are time-consuming and resource intensive. In this study, we illustrate this challenge by exploring the chemical space of large oligomers, constructed from monomeric building blocks, for potential use in organic photovoltaics (OPV). For this pu&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.01900v2-abstract-full').style.display = 'inline'; document.getElementById('2411.01900v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2411.01900v2-abstract-full" style="display: none;"> Identifying organic molecules with desirable properties from the extensive chemical space can be challenging, particularly when property evaluation methods are time-consuming and resource intensive. In this study, we illustrate this challenge by exploring the chemical space of large oligomers, constructed from monomeric building blocks, for potential use in organic photovoltaics (OPV). For this purpose, we developed a python package to search the chemical space using a building block approach: stk-search. We use stk-search (GitHub link) to compare a variety of search algorithms, including those based upon Bayesian optimization and evolutionary approaches. Initially, we evaluated and compared the performance of different search algorithms within a precomputed search space. We then extended our investigation to the vast chemical space of molecules formed of 6 building blocks (6-mers), comprising over $10^{14}$ molecules. Notably, while some algorithms show only marginal improvements over a random search approach in a relatively small, precomputed, search space, their performance in the larger chemical space is orders of magnitude better. Specifically, Bayesian optimization identified a thousand times more promising molecules with the desired properties compared to random search, using the same computational resources. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2411.01900v2-abstract-full').style.display = 'none'; document.getElementById('2411.01900v2-abstract-short').style.display = 'inline';">&#9651; 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">v1</span> submitted 4 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/2408.00219">arXiv:2408.00219</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2408.00219">pdf</a>, <a href="https://arxiv.org/format/2408.00219">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Optics">physics.optics</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"> Silicon Double-Disk Optomechanical Resonators from Wafer-Scale Double-Layered Silicon-on-Insulator </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Navarathna%2C+A">Amy Navarathna</a>, <a href="/search/physics?searchtype=author&amp;query=Carey%2C+B+J">Benjamin J. Carey</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+J+S">James S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Khademi%2C+S">Soroush Khademi</a>, <a href="/search/physics?searchtype=author&amp;query=Bowen%2C+W+P">Warwick P. Bowen</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="2408.00219v1-abstract-short" style="display: inline;"> Whispering gallery mode (WGM) optomechanical resonators are a promising technology for the simultaneous control and measurement of optical and mechanical degrees of freedom at the nanoscale. They offer potential for use across a wide range of applications such as sensors and quantum transducers. Double-disk WGM resonators, which host strongly interacting mechanical and optical modes co-localized a&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2408.00219v1-abstract-full').style.display = 'inline'; document.getElementById('2408.00219v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2408.00219v1-abstract-full" style="display: none;"> Whispering gallery mode (WGM) optomechanical resonators are a promising technology for the simultaneous control and measurement of optical and mechanical degrees of freedom at the nanoscale. They offer potential for use across a wide range of applications such as sensors and quantum transducers. Double-disk WGM resonators, which host strongly interacting mechanical and optical modes co-localized around their circumference, are particularly attractive due to their high optomechanical coupling. Large-scale integrated fabrication of silicon double-disk WGM resonators has not previously been demonstrated. In this work we present a process for the fabrication of double-layer silicon-on-insulator wafers, which we then use to fabricate functional optomechanical double silicon disk resonators with on-chip optical coupling. The integrated devices present an experimentally observed optical quality factors of the order of 10^5 and a single-photon optomechanical coupling of approximately 15 kHz. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2408.00219v1-abstract-full').style.display = 'none'; document.getElementById('2408.00219v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 31 July, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2311.12378">arXiv:2311.12378</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2311.12378">pdf</a>, <a href="https://arxiv.org/format/2311.12378">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Applied Physics">physics.app-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> </div> <p class="title is-5 mathjax"> Quantitative Profilometric Measurement of Magnetostriction in Thin-Films </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Greenall%2C+H">Hamish Greenall</a>, <a href="/search/physics?searchtype=author&amp;query=Carey%2C+B+J">Benjamin J. Carey</a>, <a href="/search/physics?searchtype=author&amp;query=Bulla%2C+D">Douglas Bulla</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+J+S">James S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Harris%2C+G+I">Glen I. Harris</a>, <a href="/search/physics?searchtype=author&amp;query=Gotardo%2C+F">Fernando Gotardo</a>, <a href="/search/physics?searchtype=author&amp;query=Foster%2C+S">Scott Foster</a>, <a href="/search/physics?searchtype=author&amp;query=Bowen%2C+W+P">Warwick P. Bowen</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="2311.12378v1-abstract-short" style="display: inline;"> A DC non-contact method for measuring the magnetostrictive strain in thin-films is demonstrated, achieving a state-of-the-art sensitivity of 0.1 ppm. In this method, an optical profilometer is used to measure the curvature induced in a magnetostrictively coated coverslip under a DC field through phase-sensitive interferometry. From this the magnetostrictive stress and strain are calculated using S&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2311.12378v1-abstract-full').style.display = 'inline'; document.getElementById('2311.12378v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2311.12378v1-abstract-full" style="display: none;"> A DC non-contact method for measuring the magnetostrictive strain in thin-films is demonstrated, achieving a state-of-the-art sensitivity of 0.1 ppm. In this method, an optical profilometer is used to measure the curvature induced in a magnetostrictively coated coverslip under a DC field through phase-sensitive interferometry. From this the magnetostrictive stress and strain are calculated using Stoney&#39;s formula. This addresses limitations of conventional techniques that measure magnetostriction based on the deflection of a cantilever under an AC field, which require complex dedicated set-ups and are sensitive to vibrational noise. Further, it reveals information about the anisotropy of the film and allows for the possibility of measuring multiple samples simultaneously. The theoretical sensitivity limits are derived, predicting a shot-noise-limit of 0.01 ppm. The method is implemented to measure the magnetostrictive hysteresis and piezomagnetic coupling of thin-film galfenol. Degradation in film performance is observed above a thickness of 206 nm, alongside a change in coercivity. This prompts investigation into the growth and optimization of galfenol films for use in devices. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2311.12378v1-abstract-full').style.display = 'none'; document.getElementById('2311.12378v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 November, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2023. </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">5 figures. Supplementary information included</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2311.01365">arXiv:2311.01365</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2311.01365">pdf</a>, <a href="https://arxiv.org/format/2311.01365">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Pushing the high count rate limits of scintillation detectors for challenging neutron-capture experiments </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Correa%2C+J+B">J. Balibrea Correa</a>, <a href="/search/physics?searchtype=author&amp;query=Lerendegui-Marco%2C+J">J. Lerendegui-Marco</a>, <a href="/search/physics?searchtype=author&amp;query=Babiano-Suarez%2C+V">V. Babiano-Suarez</a>, <a href="/search/physics?searchtype=author&amp;query=Domingo-Pardo%2C+C">C. Domingo-Pardo</a>, <a href="/search/physics?searchtype=author&amp;query=Ladarescu%2C+I">I. Ladarescu</a>, <a href="/search/physics?searchtype=author&amp;query=Tarife%C3%B1o-Saldivia%2C+A">A. Tarife帽o-Saldivia</a>, <a href="/search/physics?searchtype=author&amp;query=Alcayne%2C+V">V. Alcayne</a>, <a href="/search/physics?searchtype=author&amp;query=Cano-Ott%2C+D">D. Cano-Ott</a>, <a href="/search/physics?searchtype=author&amp;query=Gonz%C3%A1lez-Romero%2C+E">E. Gonz谩lez-Romero</a>, <a href="/search/physics?searchtype=author&amp;query=Mart%C3%ADnez%2C+T">T. Mart铆nez</a>, <a href="/search/physics?searchtype=author&amp;query=Mendoza%2C+E">E. Mendoza</a>, <a href="/search/physics?searchtype=author&amp;query=de+Rada%2C+A+P">A. P茅rez de Rada</a>, <a href="/search/physics?searchtype=author&amp;query=del+Olmo%2C+J+P">J. Plaza del Olmo</a>, <a href="/search/physics?searchtype=author&amp;query=S%C3%A1nchez-Caballero%2C+A">A. S谩nchez-Caballero</a>, <a href="/search/physics?searchtype=author&amp;query=Casanovas%2C+A">A. Casanovas</a>, <a href="/search/physics?searchtype=author&amp;query=Calvi%C3%B1o%2C+F">F. Calvi帽o</a>, <a href="/search/physics?searchtype=author&amp;query=Valenta%2C+S">S. Valenta</a>, <a href="/search/physics?searchtype=author&amp;query=Aberle%2C+O">O. Aberle</a>, <a href="/search/physics?searchtype=author&amp;query=Altieri%2C+S">S. Altieri</a>, <a href="/search/physics?searchtype=author&amp;query=Amaducci%2C+S">S. Amaducci</a>, <a href="/search/physics?searchtype=author&amp;query=Andrzejewski%2C+J">J. Andrzejewski</a>, <a href="/search/physics?searchtype=author&amp;query=Bacak%2C+M">M. Bacak</a>, <a href="/search/physics?searchtype=author&amp;query=Beltrami%2C+C">C. Beltrami</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S">S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Bernardes%2C+A+P">A. P. Bernardes</a> , et al. (109 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="2311.01365v1-abstract-short" style="display: inline;"> One of the critical aspects for the accurate determination of neutron capture cross sections when combining time-of-flight and total energy detector techniques is the characterization and control of systematic uncertainties associated to the measuring devices. In this work we explore the most conspicuous effects associated to harsh count rate conditions: dead-time and pile-up effects. Both effects&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2311.01365v1-abstract-full').style.display = 'inline'; document.getElementById('2311.01365v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2311.01365v1-abstract-full" style="display: none;"> One of the critical aspects for the accurate determination of neutron capture cross sections when combining time-of-flight and total energy detector techniques is the characterization and control of systematic uncertainties associated to the measuring devices. In this work we explore the most conspicuous effects associated to harsh count rate conditions: dead-time and pile-up effects. Both effects, when not properly treated, can lead to large systematic uncertainties and bias in the determination of neutron cross sections. In the majority of neutron capture measurements carried out at the CERN n\_TOF facility, the detectors of choice are the C$_{6}$D$_{6}$ liquid-based either in form of large-volume cells or recently commissioned sTED detector array, consisting of much smaller-volume modules. To account for the aforementioned effects, we introduce a Monte Carlo model for these detectors mimicking harsh count rate conditions similar to those happening at the CERN n\_TOF 20~m fligth path vertical measuring station. The model parameters are extracted by comparison with the experimental data taken at the same facility during 2022 experimental campaign. We propose a novel methodology to consider both, dead-time and pile-up effects simultaneously for these fast detectors and check the applicability to experimental data from $^{197}$Au($n$,$纬$), including the saturated 4.9~eV resonance which is an important component of normalization for neutron cross section measurements. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2311.01365v1-abstract-full').style.display = 'none'; document.getElementById('2311.01365v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 2 November, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2023. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2307.15229">arXiv:2307.15229</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2307.15229">pdf</a>, <a href="https://arxiv.org/format/2307.15229">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Optics">physics.optics</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Applied Physics">physics.app-ph</span> </div> </div> <p class="title is-5 mathjax"> Waveguide-integrated and portable optomechanical magnetometer </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Gotardo%2C+F">Fernando Gotardo</a>, <a href="/search/physics?searchtype=author&amp;query=Carey%2C+B+J">Benjamin J. Carey</a>, <a href="/search/physics?searchtype=author&amp;query=Greenall%2C+H">Hamish Greenall</a>, <a href="/search/physics?searchtype=author&amp;query=Harris%2C+G+I">Glen I. Harris</a>, <a href="/search/physics?searchtype=author&amp;query=Romero%2C+E">Erick Romero</a>, <a href="/search/physics?searchtype=author&amp;query=Bulla%2C+D">Douglas Bulla</a>, <a href="/search/physics?searchtype=author&amp;query=Bridge%2C+E+M">Elizabeth M. Bridge</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+J+S">James S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Foster%2C+S">Scott Foster</a>, <a href="/search/physics?searchtype=author&amp;query=Bowen%2C+W+P">Warwick P. Bowen</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="2307.15229v1-abstract-short" style="display: inline;"> Optomechanical magnetometers enable highly sensitive magnetic field sensing. However, all such magnetometers to date have been optically excited and read-out either via free space or a tapered optical fiber. This limits their scalability and integrability, and ultimately their range of applications. Here, we present an optomechanical magnetometer that is excited and read out via a suspended optica&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2307.15229v1-abstract-full').style.display = 'inline'; document.getElementById('2307.15229v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2307.15229v1-abstract-full" style="display: none;"> Optomechanical magnetometers enable highly sensitive magnetic field sensing. However, all such magnetometers to date have been optically excited and read-out either via free space or a tapered optical fiber. This limits their scalability and integrability, and ultimately their range of applications. Here, we present an optomechanical magnetometer that is excited and read out via a suspended optical waveguide fabricated on the same silicon chip as the magnetometer. Moreover, we demonstrate that thermomechanical noise limited sensitivity is possible using portable electronics and laser. The magnetometer employs a silica microdisk resonator selectively sputtered with a magnetostrictive film of galfenol (FeGa) which induces a resonant frequency shift in response to an external magnetic field. Experimental results reveal the retention of high quality-factor optical whispering gallery mode resonances whilst also demonstrating high sensitivity and dynamic range in ambient conditions. The use of off-the-shelf portable electronics without compromising sensor performance demonstrates promise for applications. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2307.15229v1-abstract-full').style.display = 'none'; document.getElementById('2307.15229v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 27 July, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2023. </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, 4 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/2301.03855">arXiv:2301.03855</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2301.03855">pdf</a>, <a href="https://arxiv.org/format/2301.03855">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Mesoscale and Nanoscale Physics">cond-mat.mes-hall</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Optics">physics.optics</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/PhysRevLett.130.263603">10.1103/PhysRevLett.130.263603 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Continuous optical-to-mechanical quantum state transfer in the unresolved sideband regime </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Navarathna%2C+A">Amy Navarathna</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+J+S">James S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Bowen%2C+W+P">Warwick P. Bowen</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="2301.03855v1-abstract-short" style="display: inline;"> Optical-to-mechanical quantum state transfer is an important capability for future quantum networks, quantum communication, and distributed quantum sensing. However, existing continuous state transfer protocols operate in the resolved sideband regime, necessitating a high-quality optical cavity and a high mechanical resonance frequency. Here, we propose a continuous protocol that operates in the u&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2301.03855v1-abstract-full').style.display = 'inline'; document.getElementById('2301.03855v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2301.03855v1-abstract-full" style="display: none;"> Optical-to-mechanical quantum state transfer is an important capability for future quantum networks, quantum communication, and distributed quantum sensing. However, existing continuous state transfer protocols operate in the resolved sideband regime, necessitating a high-quality optical cavity and a high mechanical resonance frequency. Here, we propose a continuous protocol that operates in the unresolved sideband regime. The protocol is based on feedback cooling, can be implemented with current technology, and is able to transfer non-Gaussian quantum states with high fidelity. Our protocol significantly expands the kinds of optomechanical devices for which continuous optical-to-mechanical state transfer is possible, paving the way towards quantum technological applications and the preparation of macroscopic superpositions to test the fundamentals of quantum science. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2301.03855v1-abstract-full').style.display = 'none'; document.getElementById('2301.03855v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 January, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2023. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2209.04443">arXiv:2209.04443</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2209.04443">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> The CERN n TOF NEAR station for astrophysics- and application-related neutron activation measurements </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Patronis%2C+N">N. Patronis</a>, <a href="/search/physics?searchtype=author&amp;query=Mengoni%2C+A">A. Mengoni</a>, <a href="/search/physics?searchtype=author&amp;query=Colonna%2C+N">N. Colonna</a>, <a href="/search/physics?searchtype=author&amp;query=Cecchetto%2C+M">M. Cecchetto</a>, <a href="/search/physics?searchtype=author&amp;query=Domingo-Pardo%2C+C">C. Domingo-Pardo</a>, <a href="/search/physics?searchtype=author&amp;query=Aberle%2C+O">O. Aberle</a>, <a href="/search/physics?searchtype=author&amp;query=Lerendegui-Marco%2C+J">J. Lerendegui-Marco</a>, <a href="/search/physics?searchtype=author&amp;query=Gervino%2C+G">G. Gervino</a>, <a href="/search/physics?searchtype=author&amp;query=Stamati%2C+M+E">M. E. Stamati</a>, <a href="/search/physics?searchtype=author&amp;query=Goula%2C+S">S. Goula</a>, <a href="/search/physics?searchtype=author&amp;query=Bernardes%2C+A+P">A. P. Bernardes</a>, <a href="/search/physics?searchtype=author&amp;query=Mastromarco%2C+M">M. Mastromarco</a>, <a href="/search/physics?searchtype=author&amp;query=Manna%2C+A">A. Manna</a>, <a href="/search/physics?searchtype=author&amp;query=Vlastou%2C+R">R. Vlastou</a>, <a href="/search/physics?searchtype=author&amp;query=Massimi%2C+C">C. Massimi</a>, <a href="/search/physics?searchtype=author&amp;query=Calviani%2C+M">M. Calviani</a>, <a href="/search/physics?searchtype=author&amp;query=Alcayne%2C+V">V. Alcayne</a>, <a href="/search/physics?searchtype=author&amp;query=Altieri%2C+S">S. Altieri</a>, <a href="/search/physics?searchtype=author&amp;query=Amaducci%2C+S">S. Amaducci</a>, <a href="/search/physics?searchtype=author&amp;query=Andrzejewski%2C+J">J. Andrzejewski</a>, <a href="/search/physics?searchtype=author&amp;query=Babiano-Suarez%2C+V">V. Babiano-Suarez</a>, <a href="/search/physics?searchtype=author&amp;query=Bacak%2C+M">M. Bacak</a>, <a href="/search/physics?searchtype=author&amp;query=Balibrea%2C+J">J. Balibrea</a>, <a href="/search/physics?searchtype=author&amp;query=Beltrami%2C+C">C. Beltrami</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S">S. Bennett</a> , et al. (108 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="2209.04443v1-abstract-short" style="display: inline;"> A new experimental area, the NEAR station, has recently been built at the CERN n TOF facility, at a short distance from the spallation target (1.5 m). The new area, characterized by a neutron beam of very high flux, has been designed with the purpose of performing activation measurements of interest for astrophysics and various applications. The beam is transported from the spallation target to th&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2209.04443v1-abstract-full').style.display = 'inline'; document.getElementById('2209.04443v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2209.04443v1-abstract-full" style="display: none;"> A new experimental area, the NEAR station, has recently been built at the CERN n TOF facility, at a short distance from the spallation target (1.5 m). The new area, characterized by a neutron beam of very high flux, has been designed with the purpose of performing activation measurements of interest for astrophysics and various applications. The beam is transported from the spallation target to the NEAR station through a hole in the shielding wall of the target, inside which a collimator is inserted. The new area is complemented with a 纬-ray spectroscopy laboratory, the GEAR station, equipped with a high efficiency HPGe detector, for the measurement of the activity resulting from irradiation of a sample in the NEAR station. The use of a moderator/filter assembly is envisaged, in order to produce a neutron beam of Maxwellian shape at different thermal energies, necessary for the measurement of Maxwellian Averaged Cross Sections of astrophysical interest. A new fast-cycling activation technique is also being investigated, for measurements of reactions leading to isotopes of very short half life. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2209.04443v1-abstract-full').style.display = 'none'; document.getElementById('2209.04443v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 September, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2022. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2107.08545">arXiv:2107.08545</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2107.08545">pdf</a>, <a href="https://arxiv.org/format/2107.08545">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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/10.1007/s00190-022-01659-0">10.1007/s00190-022-01659-0 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A Simplified Gravitational Reference Sensor for Satellite Geodesy </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Alvarez%2C+A+D">Anthony Davila Alvarez</a>, <a href="/search/physics?searchtype=author&amp;query=Knudtson%2C+A">Aaron Knudtson</a>, <a href="/search/physics?searchtype=author&amp;query=Patel%2C+U">Unmil Patel</a>, <a href="/search/physics?searchtype=author&amp;query=Gleason%2C+J">Joseph Gleason</a>, <a href="/search/physics?searchtype=author&amp;query=Hollis%2C+H">Harold Hollis</a>, <a href="/search/physics?searchtype=author&amp;query=Sanjuan%2C+J">Jose Sanjuan</a>, <a href="/search/physics?searchtype=author&amp;query=Doughty%2C+N">Neil Doughty</a>, <a href="/search/physics?searchtype=author&amp;query=McDaniel%2C+G">Glenn McDaniel</a>, <a href="/search/physics?searchtype=author&amp;query=Lee%2C+J">Jennifer Lee</a>, <a href="/search/physics?searchtype=author&amp;query=Leitch%2C+J">James Leitch</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S">Stephen Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Bevilacqua%2C+R">Riccardo Bevilacqua</a>, <a href="/search/physics?searchtype=author&amp;query=Mueller%2C+G">Guido Mueller</a>, <a href="/search/physics?searchtype=author&amp;query=Spero%2C+R">Robert Spero</a>, <a href="/search/physics?searchtype=author&amp;query=Ware%2C+B">Brent Ware</a>, <a href="/search/physics?searchtype=author&amp;query=Wass%2C+P">Peter Wass</a>, <a href="/search/physics?searchtype=author&amp;query=Wiese%2C+D">David Wiese</a>, <a href="/search/physics?searchtype=author&amp;query=Ziemer%2C+J">John Ziemer</a>, <a href="/search/physics?searchtype=author&amp;query=Conklin%2C+J+W">John W. Conklin</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="2107.08545v4-abstract-short" style="display: inline;"> We describe a Simplified Gravitational Reference Sensor (S-GRS), an ultra-precise inertial sensor for future Earth geodesy missions. These sensors are used to measure or compensate for all non-gravitational accelerations of the host spacecraft so that they can be removed in the data analysis to recover spacecraft motion due to Earth&#39;s gravity field, which is the main science observable. Low-low sa&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2107.08545v4-abstract-full').style.display = 'inline'; document.getElementById('2107.08545v4-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2107.08545v4-abstract-full" style="display: none;"> We describe a Simplified Gravitational Reference Sensor (S-GRS), an ultra-precise inertial sensor for future Earth geodesy missions. These sensors are used to measure or compensate for all non-gravitational accelerations of the host spacecraft so that they can be removed in the data analysis to recover spacecraft motion due to Earth&#39;s gravity field, which is the main science observable. Low-low satellite-to-satellite tracking missions like GRACE-FO that utilize laser ranging interferometers are technologically limited by the acceleration noise performance of their electrostatic accelerometers, in addition to temporal aliasing associated with Earth&#39;s dynamic gravity field. The S-GRS is estimated to be at least 40 times more sensitive than the GRACE accelerometers and more than 500 times more sensitive if operated on a drag-compensated platform. The improved performance is enabled by increasing the mass of the sensor&#39;s test mass, increasing the gap between the test mass and its electrode housing, removing the small grounding wire used in the GRACE accelerometers and replacing them with a UV LED-based charge management system. This level of improvement allows future missions to fully take advantage of the sensitivity of the GRACE-FO laser Ranging Interferometer in the gravity recovery analysis. The S-GRS concept is a simplified version of the flight-proven LISA Pathfinder GRS. Our performance estimates are based on models vetted during the LISA Pathfinder flight and the expected Earth orbiting spacecraft environment based on flight data from GRACE-FO. The relatively low volume, mass, and a power consumption enables use of the S-GRS on ESPA-class microsatellites, reducing launch costs or enabling larger numbers of satellite pairs to be utilized to improve the temporal resolution of Earth gravity field maps. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2107.08545v4-abstract-full').style.display = 'none'; document.getElementById('2107.08545v4-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 12 January, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 18 July, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2021. </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">Corrected typos, clarified some sentences, and added references</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2106.15843">arXiv:2106.15843</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2106.15843">pdf</a>, <a href="https://arxiv.org/format/2106.15843">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Applied Physics">physics.app-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Space Physics">physics.space-ph</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/10.3390/s21165568">10.3390/s21165568 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Precision Magnetometers for Aerospace Applications </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+J+S">James S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Vyhnalek%2C+B+E">Brian E. Vyhnalek</a>, <a href="/search/physics?searchtype=author&amp;query=Greenall%2C+H">Hamish Greenall</a>, <a href="/search/physics?searchtype=author&amp;query=Bridge%2C+E+M">Elizabeth M. Bridge</a>, <a href="/search/physics?searchtype=author&amp;query=Gotardo%2C+F">Fernando Gotardo</a>, <a href="/search/physics?searchtype=author&amp;query=Forstner%2C+S">Stefan Forstner</a>, <a href="/search/physics?searchtype=author&amp;query=Harris%2C+G+I">Glen I. Harris</a>, <a href="/search/physics?searchtype=author&amp;query=Miranda%2C+F+A">F茅lix A. Miranda</a>, <a href="/search/physics?searchtype=author&amp;query=Bowen%2C+W+P">Warwick P. Bowen</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="2106.15843v1-abstract-short" style="display: inline;"> Aerospace technologies are crucial for modern civilization; space-based infrastructure underpins weather forecasting, communications, terrestrial navigation and logistics, planetary observations, solar monitoring, and other indispensable capabilities. Extraplanetary exploration -- including orbital surveys and (more recently) roving, flying, or submersible unmanned vehicles -- is also a key scient&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2106.15843v1-abstract-full').style.display = 'inline'; document.getElementById('2106.15843v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2106.15843v1-abstract-full" style="display: none;"> Aerospace technologies are crucial for modern civilization; space-based infrastructure underpins weather forecasting, communications, terrestrial navigation and logistics, planetary observations, solar monitoring, and other indispensable capabilities. Extraplanetary exploration -- including orbital surveys and (more recently) roving, flying, or submersible unmanned vehicles -- is also a key scientific and technological frontier, believed by many to be paramount to the long-term survival and prosperity of humanity. All of these aerospace applications require reliable control of the craft and the ability to record high-precision measurements of physical quantities. Magnetometers deliver on both of these aspects, and have been vital to the success of numerous missions. In this review paper, we provide an introduction to the relevant instruments and their applications. We consider past and present magnetometers, their proven aerospace applications, and emerging uses. We then look to the future, reviewing recent progress in magnetometer technology. We particularly focus on magnetometers that use optical readout, including atomic magnetometers, magnetometers based on quantum defects in diamond, and optomechanical magnetometers. These optical magnetometers offer a combination of field sensitivity, size, weight, and power consumption that allows them to reach performance regimes that are inaccessible with existing techniques. This promises to enable new applications in areas ranging from unmanned vehicles to navigation and exploration. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2106.15843v1-abstract-full').style.display = 'none'; document.getElementById('2106.15843v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 June, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2021. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2012.10374">arXiv:2012.10374</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2012.10374">pdf</a>, <a href="https://arxiv.org/format/2012.10374">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</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/10.1140/epja/s10050-021-00507-7">10.1140/epja/s10050-021-00507-7 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Imaging neutron capture cross sections: i-TED proof-of-concept and future prospects based on Machine-Learning techniques </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Babiano-Su%C3%A1rez%2C+V">V. Babiano-Su谩rez</a>, <a href="/search/physics?searchtype=author&amp;query=Lerendegui-Marco%2C+J">J. Lerendegui-Marco</a>, <a href="/search/physics?searchtype=author&amp;query=Balibrea-Correa%2C+J">J. Balibrea-Correa</a>, <a href="/search/physics?searchtype=author&amp;query=Caballero%2C+L">L. Caballero</a>, <a href="/search/physics?searchtype=author&amp;query=Calvo%2C+D">D. Calvo</a>, <a href="/search/physics?searchtype=author&amp;query=Ladarescu%2C+I">I. Ladarescu</a>, <a href="/search/physics?searchtype=author&amp;query=Domingo-Pardo%2C+C">C. Domingo-Pardo</a>, <a href="/search/physics?searchtype=author&amp;query=Calvi%C3%B1o%2C+F">F. Calvi帽o</a>, <a href="/search/physics?searchtype=author&amp;query=Casanovas%2C+A">A. Casanovas</a>, <a href="/search/physics?searchtype=author&amp;query=Tarife%C3%B1o-Saldivia%2C+A">A. Tarife帽o-Saldivia</a>, <a href="/search/physics?searchtype=author&amp;query=Alcayne%2C+V">V. Alcayne</a>, <a href="/search/physics?searchtype=author&amp;query=Guerrero%2C+C">C. Guerrero</a>, <a href="/search/physics?searchtype=author&amp;query=Mill%C3%A1n-Callado%2C+M+A">M. A. Mill谩n-Callado</a>, <a href="/search/physics?searchtype=author&amp;query=Gonz%C3%A1lez%2C+M+T+R">M. T. Rodr铆guez Gonz谩lez</a>, <a href="/search/physics?searchtype=author&amp;query=Barbagallo%2C+M">M. Barbagallo</a>, <a href="/search/physics?searchtype=author&amp;query=Aberle%2C+O">O. Aberle</a>, <a href="/search/physics?searchtype=author&amp;query=Amaducci%2C+S">S. Amaducci</a>, <a href="/search/physics?searchtype=author&amp;query=Andrzejewski%2C+J">J. Andrzejewski</a>, <a href="/search/physics?searchtype=author&amp;query=Audouin%2C+L">L. Audouin</a>, <a href="/search/physics?searchtype=author&amp;query=Bacak%2C+M">M. Bacak</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S">S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Berthoumieux%2C+E">E. Berthoumieux</a>, <a href="/search/physics?searchtype=author&amp;query=Billowes%2C+J">J. Billowes</a>, <a href="/search/physics?searchtype=author&amp;query=Bosnar%2C+D">D. Bosnar</a>, <a href="/search/physics?searchtype=author&amp;query=Brown%2C+A">A. Brown</a> , et al. (110 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="2012.10374v1-abstract-short" style="display: inline;"> i-TED is an innovative detection system which exploits Compton imaging techniques to achieve a superior signal-to-background ratio in ($n,纬$) cross-section measurements using time-of-flight technique. This work presents the first experimental validation of the i-TED apparatus for high-resolution time-of-flight experiments and demonstrates for the first time the concept proposed for background reje&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.10374v1-abstract-full').style.display = 'inline'; document.getElementById('2012.10374v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2012.10374v1-abstract-full" style="display: none;"> i-TED is an innovative detection system which exploits Compton imaging techniques to achieve a superior signal-to-background ratio in ($n,纬$) cross-section measurements using time-of-flight technique. This work presents the first experimental validation of the i-TED apparatus for high-resolution time-of-flight experiments and demonstrates for the first time the concept proposed for background rejection. To this aim both $^{197}$Au($n,纬$) and $^{56}$Fe($n, 纬$) reactions were measured at CERN n\_TOF using an i-TED demonstrator based on only three position-sensitive detectors. Two \cds detectors were also used to benchmark the performance of i-TED. The i-TED prototype built for this study shows a factor of $\sim$3 higher detection sensitivity than state-of-the-art \cds detectors in the $\sim$10~keV neutron energy range of astrophysical interest. This paper explores also the perspectives of further enhancement in performance attainable with the final i-TED array consisting of twenty position-sensitive detectors and new analysis methodologies based on Machine-Learning techniques. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.10374v1-abstract-full').style.display = 'none'; document.getElementById('2012.10374v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 December, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2020. </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, 16 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/2006.01653">arXiv:2006.01653</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2006.01653">pdf</a>, <a href="https://arxiv.org/format/2006.01653">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Image and Video Processing">eess.IV</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Optics">physics.optics</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/10.1364/AO.399227">10.1364/AO.399227 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Compact Multi-Spectral Pushframe Camera for Nano-Satellites </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Noblet%2C+Y">Yoann Noblet</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S">Stuart Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Griffin%2C+P+F">Paul F. Griffin</a>, <a href="/search/physics?searchtype=author&amp;query=Murray%2C+P">Paul Murray</a>, <a href="/search/physics?searchtype=author&amp;query=Marshall%2C+S">Stephen Marshall</a>, <a href="/search/physics?searchtype=author&amp;query=Roga%2C+W">Wojciech Roga</a>, <a href="/search/physics?searchtype=author&amp;query=Jeffers%2C+J">John Jeffers</a>, <a href="/search/physics?searchtype=author&amp;query=Oi%2C+D">Daniel Oi</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="2006.01653v1-abstract-short" style="display: inline;"> In this paper we present an evolution of the single-pixel camera architecture, called &#39;pushframe&#39;, which addresses the limitations of pushbroom cameras in space-based applications. In particular, it is well-suited to observing fast moving scenes while retaining high spatial resolution and sensitivity. We show that the system is capable of producing colour images with good fidelity and scalable res&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2006.01653v1-abstract-full').style.display = 'inline'; document.getElementById('2006.01653v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2006.01653v1-abstract-full" style="display: none;"> In this paper we present an evolution of the single-pixel camera architecture, called &#39;pushframe&#39;, which addresses the limitations of pushbroom cameras in space-based applications. In particular, it is well-suited to observing fast moving scenes while retaining high spatial resolution and sensitivity. We show that the system is capable of producing colour images with good fidelity and scalable resolution performance. The principle of our design places no restriction on the spectral range to be captured, making it suitable for wide infrared imaging. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2006.01653v1-abstract-full').style.display = 'none'; document.getElementById('2006.01653v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 1 June, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Appl. Opt. 59, 8511-8518 (2020) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1911.06972">arXiv:1911.06972</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1911.06972">pdf</a>, <a href="https://arxiv.org/format/1911.06972">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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/10.1088/1742-6596/1668/1/012013">10.1088/1742-6596/1668/1/012013 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Review and new concepts for neutron-capture measurements of astrophysical interest </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Domingo-Pardo%2C+C">C. Domingo-Pardo</a>, <a href="/search/physics?searchtype=author&amp;query=Babiano-Suarez%2C+V">V. Babiano-Suarez</a>, <a href="/search/physics?searchtype=author&amp;query=Balibrea-Correa%2C+J">J. Balibrea-Correa</a>, <a href="/search/physics?searchtype=author&amp;query=Caballero%2C+L">L. Caballero</a>, <a href="/search/physics?searchtype=author&amp;query=Ladarescu%2C+I">I. Ladarescu</a>, <a href="/search/physics?searchtype=author&amp;query=Lerendegui-Marco%2C+J">J. Lerendegui-Marco</a>, <a href="/search/physics?searchtype=author&amp;query=Tain%2C+J+L">J. L. Tain</a>, <a href="/search/physics?searchtype=author&amp;query=Calvi%C3%B1o%2C+F">F. Calvi帽o</a>, <a href="/search/physics?searchtype=author&amp;query=Casanovas%2C+A">A. Casanovas</a>, <a href="/search/physics?searchtype=author&amp;query=Segarra%2C+A">A. Segarra</a>, <a href="/search/physics?searchtype=author&amp;query=Tarife%C3%B1o-Saldivia%2C+A+E">A. E. Tarife帽o-Saldivia</a>, <a href="/search/physics?searchtype=author&amp;query=Guerrero%2C+C">C. Guerrero</a>, <a href="/search/physics?searchtype=author&amp;query=Mill%C3%A1n-Callado%2C+M+A">M. A. Mill谩n-Callado</a>, <a href="/search/physics?searchtype=author&amp;query=Quesada%2C+J+M">J. M. Quesada</a>, <a href="/search/physics?searchtype=author&amp;query=Rodr%C3%ADguez-Gonz%C3%A1lez%2C+M+T">M. T. Rodr铆guez-Gonz谩lez</a>, <a href="/search/physics?searchtype=author&amp;query=Aberle%2C+O">O. Aberle</a>, <a href="/search/physics?searchtype=author&amp;query=Alcayne%2C+V">V. Alcayne</a>, <a href="/search/physics?searchtype=author&amp;query=Amaducci%2C+S">S. Amaducci</a>, <a href="/search/physics?searchtype=author&amp;query=Andrzejewski%2C+J">J. Andrzejewski</a>, <a href="/search/physics?searchtype=author&amp;query=Audouin%2C+L">L. Audouin</a>, <a href="/search/physics?searchtype=author&amp;query=Bacak%2C+M">M. Bacak</a>, <a href="/search/physics?searchtype=author&amp;query=Barbagallo%2C+M">M. Barbagallo</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S">S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Berthoumieux%2C+E">E. Berthoumieux</a>, <a href="/search/physics?searchtype=author&amp;query=Bosnar%2C+D">D. Bosnar</a> , et al. (106 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="1911.06972v1-abstract-short" style="display: inline;"> The idea of slow-neutron capture nucleosynthesis formulated in 1957 triggered a tremendous experimental effort in different laboratories worldwide to measure the relevant nuclear physics input quantities, namely ($n,纬$) cross sections over the stellar temperature range (from few eV up to several hundred keV) for most of the isotopes involved from Fe up to Bi. A brief historical review focused on t&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1911.06972v1-abstract-full').style.display = 'inline'; document.getElementById('1911.06972v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1911.06972v1-abstract-full" style="display: none;"> The idea of slow-neutron capture nucleosynthesis formulated in 1957 triggered a tremendous experimental effort in different laboratories worldwide to measure the relevant nuclear physics input quantities, namely ($n,纬$) cross sections over the stellar temperature range (from few eV up to several hundred keV) for most of the isotopes involved from Fe up to Bi. A brief historical review focused on total energy detectors will be presented to illustrate how, advances in instrumentation have led, over the years, to the assessment and discovery of many new aspects of $s$-process nucleosynthesis and to the progressive refinement of theoretical models of stellar evolution. A summary will be presented on current efforts to develop new detection concepts, such as the Total-Energy Detector with $纬$-ray imaging capability (i-TED). The latter is based on the simultaneous combination of Compton imaging with neutron time-of-flight (TOF) techniques, in order to achieve a superior level of sensitivity and selectivity in the measurement of stellar neutron capture rates. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1911.06972v1-abstract-full').style.display = 'none'; document.getElementById('1911.06972v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 16 November, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2019. </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">Nuclear Physics in Astrophysics IX - Conference Proceedings</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1911.06412">arXiv:1911.06412</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1911.06412">pdf</a>, <a href="https://arxiv.org/format/1911.06412">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Mesoscale and Nanoscale Physics">cond-mat.mes-hall</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Optics">physics.optics</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/PhysRevLett.125.043604">10.1103/PhysRevLett.125.043604 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Mechanical squeezing via fast continuous measurement </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Meng%2C+C">Chao Meng</a>, <a href="/search/physics?searchtype=author&amp;query=Brawley%2C+G+A">George A. Brawley</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+J+S">James S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Vanner%2C+M+R">Michael R. Vanner</a>, <a href="/search/physics?searchtype=author&amp;query=Bowen%2C+W+P">Warwick P. Bowen</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="1911.06412v3-abstract-short" style="display: inline;"> We revisit quantum state preparation of an oscillator by continuous linear position measurement. Quite general analytical expressions are derived for the conditioned state of the oscillator. Remarkably, we predict that quantum squeezing is possible outside of both the backaction dominated and quantum coherent oscillation regimes, relaxing experimental requirements even compared to ground-state coo&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1911.06412v3-abstract-full').style.display = 'inline'; document.getElementById('1911.06412v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1911.06412v3-abstract-full" style="display: none;"> We revisit quantum state preparation of an oscillator by continuous linear position measurement. Quite general analytical expressions are derived for the conditioned state of the oscillator. Remarkably, we predict that quantum squeezing is possible outside of both the backaction dominated and quantum coherent oscillation regimes, relaxing experimental requirements even compared to ground-state cooling. This provides a new way to generate non-classical states of macroscopic mechanical oscillators, and opens the door to quantum sensing and tests of quantum macroscopicity at room temperature. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1911.06412v3-abstract-full').style.display = 'none'; document.getElementById('1911.06412v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 24 July, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 14 November, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 125, 043604 (2020) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1902.08501">arXiv:1902.08501</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1902.08501">pdf</a>, <a href="https://arxiv.org/format/1902.08501">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Applied Physics">physics.app-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</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/10.1088/2058-9565/ab0ca8">10.1088/2058-9565/ab0ca8 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Development of transmon qubits solely from optical lithography on 300mm wafers </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Foroozani%2C+N">N. Foroozani</a>, <a href="/search/physics?searchtype=author&amp;query=Hobbs%2C+C">C. Hobbs</a>, <a href="/search/physics?searchtype=author&amp;query=Hung%2C+C+C">C. C. Hung</a>, <a href="/search/physics?searchtype=author&amp;query=Olson%2C+S">S. Olson</a>, <a href="/search/physics?searchtype=author&amp;query=Ashworth%2C+D">D. Ashworth</a>, <a href="/search/physics?searchtype=author&amp;query=Holland%2C+E">E. Holland</a>, <a href="/search/physics?searchtype=author&amp;query=Malloy%2C+M">M. Malloy</a>, <a href="/search/physics?searchtype=author&amp;query=Kearney%2C+P">P. Kearney</a>, <a href="/search/physics?searchtype=author&amp;query=O%27Brien%2C+B">B. O&#39;Brien</a>, <a href="/search/physics?searchtype=author&amp;query=Bunday%2C+B">B. Bunday</a>, <a href="/search/physics?searchtype=author&amp;query=DiPaola%2C+D">D. DiPaola</a>, <a href="/search/physics?searchtype=author&amp;query=Advocate%2C+W">W. Advocate</a>, <a href="/search/physics?searchtype=author&amp;query=Murray%2C+T">T. Murray</a>, <a href="/search/physics?searchtype=author&amp;query=Hansen%2C+P">P. Hansen</a>, <a href="/search/physics?searchtype=author&amp;query=Novak%2C+S">S. Novak</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S">S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Rodgers%2C+M">M. Rodgers</a>, <a href="/search/physics?searchtype=author&amp;query=Baker-O%27Neal%2C+B">B. Baker-O&#39;Neal</a>, <a href="/search/physics?searchtype=author&amp;query=Sapp%2C+B">B. Sapp</a>, <a href="/search/physics?searchtype=author&amp;query=Barth%2C+E">E. Barth</a>, <a href="/search/physics?searchtype=author&amp;query=Hedrick%2C+J">J. Hedrick</a>, <a href="/search/physics?searchtype=author&amp;query=Goldblatt%2C+R">R. Goldblatt</a>, <a href="/search/physics?searchtype=author&amp;query=Rao%2C+S+S+P">S. S. Papa Rao</a>, <a href="/search/physics?searchtype=author&amp;query=Osborn%2C+K+D">K. D. Osborn</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="1902.08501v1-abstract-short" style="display: inline;"> Qubit information processors are increasing in footprint but currently rely on e-beam lithography for patterning the required Josephson junctions (JJs). Advanced optical lithography is an alternative patterning method, and we report on the development of transmon qubits patterned solely with optical lithography. The lithography uses 193 nm wavelength exposure and 300-mm large silicon wafers. Qubit&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1902.08501v1-abstract-full').style.display = 'inline'; document.getElementById('1902.08501v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1902.08501v1-abstract-full" style="display: none;"> Qubit information processors are increasing in footprint but currently rely on e-beam lithography for patterning the required Josephson junctions (JJs). Advanced optical lithography is an alternative patterning method, and we report on the development of transmon qubits patterned solely with optical lithography. The lithography uses 193 nm wavelength exposure and 300-mm large silicon wafers. Qubits and arrays of evaluation JJs were patterned with process control which resulted in narrow feature distributions: a standard deviation of 0:78% for a 220 nm linewidth pattern realized across over half the width of the wafers. Room temperature evaluation found a 2.8-3.6% standard deviation in JJ resistance in completed chips. The qubits used aluminum and titanium nitride films on silicon substrates without substantial silicon etching. T1 times of the qubits were extracted at 26 - 27 microseconds, indicating a low level of material-based qubit defects. This study shows that large wafer optical lithography on silicon is adequate for high-quality transmon qubits, and shows a promising path for improving many-qubit processors. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1902.08501v1-abstract-full').style.display = 'none'; document.getElementById('1902.08501v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 22 February, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2019. </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">7 pages, 4 figures, submitted to Quantum Science and Technology</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Journal of Quantum Science and Technology, 2019 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1509.00070">arXiv:1509.00070</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1509.00070">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Emerging Technologies">cs.ET</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Materials Science">cond-mat.mtrl-sci</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Data Analysis, Statistics and Probability">physics.data-an</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/10.1109/IMW.2015.7150290">10.1109/IMW.2015.7150290 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> In-Line-Test of Variability and Bit-Error-Rate of HfOx-Based Resistive Memory </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Ji%2C+B+L">B. L. Ji</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+H">H. Li</a>, <a href="/search/physics?searchtype=author&amp;query=Ye%2C+Q">Q. Ye</a>, <a href="/search/physics?searchtype=author&amp;query=Gausepohl%2C+S">S. Gausepohl</a>, <a href="/search/physics?searchtype=author&amp;query=Deora%2C+S">S. Deora</a>, <a href="/search/physics?searchtype=author&amp;query=Veksler%2C+D">D. Veksler</a>, <a href="/search/physics?searchtype=author&amp;query=Vivekanand%2C+S">S. Vivekanand</a>, <a href="/search/physics?searchtype=author&amp;query=Chong%2C+H">H. Chong</a>, <a href="/search/physics?searchtype=author&amp;query=Stamper%2C+H">H. Stamper</a>, <a href="/search/physics?searchtype=author&amp;query=Burroughs%2C+T">T. Burroughs</a>, <a href="/search/physics?searchtype=author&amp;query=Johnson%2C+C">C. Johnson</a>, <a href="/search/physics?searchtype=author&amp;query=Smalley%2C+M">M. Smalley</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S">S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Kaushik%2C+V">V. Kaushik</a>, <a href="/search/physics?searchtype=author&amp;query=Piccirillo%2C+J">J. Piccirillo</a>, <a href="/search/physics?searchtype=author&amp;query=Rodgers%2C+M">M. Rodgers</a>, <a href="/search/physics?searchtype=author&amp;query=Passaro%2C+M">M. Passaro</a>, <a href="/search/physics?searchtype=author&amp;query=Liehr%2C+M">M. Liehr</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="1509.00070v1-abstract-short" style="display: inline;"> Spatial and temporal variability of HfOx-based resistive random access memory (RRAM) are investigated for manufacturing and product designs. Manufacturing variability is characterized at different levels including lots, wafers, and chips. Bit-error-rate (BER) is proposed as a holistic parameter for the write cycle resistance statistics. Using the electrical in-line-test cycle data, a method is dev&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1509.00070v1-abstract-full').style.display = 'inline'; document.getElementById('1509.00070v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1509.00070v1-abstract-full" style="display: none;"> Spatial and temporal variability of HfOx-based resistive random access memory (RRAM) are investigated for manufacturing and product designs. Manufacturing variability is characterized at different levels including lots, wafers, and chips. Bit-error-rate (BER) is proposed as a holistic parameter for the write cycle resistance statistics. Using the electrical in-line-test cycle data, a method is developed to derive BERs as functions of the design margin, to provide guidance for technology evaluation and product design. The proposed BER calculation can also be used in the off-line bench test and build-in-self-test (BIST) for adaptive error correction and for the other types of random access memories. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1509.00070v1-abstract-full').style.display = 'none'; document.getElementById('1509.00070v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 31 August, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2015. </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">4 pages. Memory Workshop (IMW), 2015 IEEE International</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> 2015 IEEE International Memory Workshop(IMW), 17-20 May 2015 URL: http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&amp;arnumber=7150290&amp;isnumber=7150256 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1311.1801">arXiv:1311.1801</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1311.1801">pdf</a>, <a href="https://arxiv.org/ps/1311.1801">ps</a>, <a href="https://arxiv.org/format/1311.1801">other</a>]&nbsp;</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> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Atomic Physics">physics.atom-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Biological Physics">physics.bio-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</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/10.1021/nl502988n">10.1021/nl502988n <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> All-optical sensing of a single-molecule electron spin </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Sushkov%2C+A+O">A. O. Sushkov</a>, <a href="/search/physics?searchtype=author&amp;query=Chisholm%2C+N">N. Chisholm</a>, <a href="/search/physics?searchtype=author&amp;query=Lovchinsky%2C+I">I. Lovchinsky</a>, <a href="/search/physics?searchtype=author&amp;query=Kubo%2C+M">M. Kubo</a>, <a href="/search/physics?searchtype=author&amp;query=Lo%2C+P+K">P. K. Lo</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S+D">S. D. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Hunger%2C+D">D. Hunger</a>, <a href="/search/physics?searchtype=author&amp;query=Akimov%2C+A">A. Akimov</a>, <a href="/search/physics?searchtype=author&amp;query=Walsworth%2C+R+L">R. L. Walsworth</a>, <a href="/search/physics?searchtype=author&amp;query=Park%2C+H">H. Park</a>, <a href="/search/physics?searchtype=author&amp;query=Lukin%2C+M+D">M. D. Lukin</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="1311.1801v1-abstract-short" style="display: inline;"> We demonstrate an all-optical method for magnetic sensing of individual molecules in ambient conditions at room temperature. Our approach is based on shallow nitrogen-vacancy (NV) centers near the surface of a diamond crystal, which we use to detect single paramagnetic molecules covalently attached to the diamond surface. The manipulation and readout of the NV centers is all-optical and provides a&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1311.1801v1-abstract-full').style.display = 'inline'; document.getElementById('1311.1801v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1311.1801v1-abstract-full" style="display: none;"> We demonstrate an all-optical method for magnetic sensing of individual molecules in ambient conditions at room temperature. Our approach is based on shallow nitrogen-vacancy (NV) centers near the surface of a diamond crystal, which we use to detect single paramagnetic molecules covalently attached to the diamond surface. The manipulation and readout of the NV centers is all-optical and provides a sensitive probe of the magnetic field fluctuations stemming from the dynamics of the electronic spins of the attached molecules. As a specific example, we demonstrate detection of a single paramagnetic molecule containing a gadolinium (Gd$^{3+}$) ion. We confirm single-molecule resolution using optical fluorescence and atomic force microscopy to co-localize one NV center and one Gd$^{3+}$-containing molecule. Possible applications include nanoscale and in vivo magnetic spectroscopy and imaging of individual molecules. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1311.1801v1-abstract-full').style.display = 'none'; document.getElementById('1311.1801v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 7 November, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2013. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1307.1130">arXiv:1307.1130</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1307.1130">pdf</a>, <a href="https://arxiv.org/format/1307.1130">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Quantum Gases">cond-mat.quant-gas</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Atomic Physics">physics.atom-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Chemical Physics">physics.chem-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</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.88.014426">10.1103/PhysRevB.88.014426 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Controllable quantum spin glasses with magnetic impurities embedded in quantum solids </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Lemeshko%2C+M">Mikhail Lemeshko</a>, <a href="/search/physics?searchtype=author&amp;query=Yao%2C+N+Y">Norman Y. Yao</a>, <a href="/search/physics?searchtype=author&amp;query=Gorshkov%2C+A+V">Alexey V. Gorshkov</a>, <a href="/search/physics?searchtype=author&amp;query=Weimer%2C+H">Hendrik Weimer</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S+D">Steven D. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Momose%2C+T">Takamasa Momose</a>, <a href="/search/physics?searchtype=author&amp;query=Gopalakrishnan%2C+S">Sarang Gopalakrishnan</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="1307.1130v1-abstract-short" style="display: inline;"> Magnetic impurities embedded in inert solids can exhibit long coherence times and interact with one another via their intrinsic anisotropic dipolar interaction. We argue that, as a consequence of these properties, disordered ensembles of magnetic impurities provide an effective platform for realizing a controllable, tunable version of the dipolar quantum spin glass seen in LiHo$_x$Y$_{1-x}$F$_4$.&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1307.1130v1-abstract-full').style.display = 'inline'; document.getElementById('1307.1130v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1307.1130v1-abstract-full" style="display: none;"> Magnetic impurities embedded in inert solids can exhibit long coherence times and interact with one another via their intrinsic anisotropic dipolar interaction. We argue that, as a consequence of these properties, disordered ensembles of magnetic impurities provide an effective platform for realizing a controllable, tunable version of the dipolar quantum spin glass seen in LiHo$_x$Y$_{1-x}$F$_4$. Specifically, we propose and analyze a system composed of dysprosium atoms embedded in solid helium. We describe the phase diagram of the system and discuss the realizability and detectability of the quantum spin glass and antiglass phases. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1307.1130v1-abstract-full').style.display = 'none'; document.getElementById('1307.1130v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 3 July, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2013. </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, 3 figures, 1 table</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. B 88, 014426 (2013) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/9702008">arXiv:physics/9702008</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/physics/9702008">pdf</a>, <a href="https://arxiv.org/ps/physics/9702008">ps</a>, <a href="https://arxiv.org/format/physics/9702008">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</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/PhysRevLett.78.2916">10.1103/PhysRevLett.78.2916 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Two-pion correlations in Au+Au collisions at 10.8 GeV/c per nucleon </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=E877+Collaboration"> E877 Collaboration</a>, <a href="/search/physics?searchtype=author&amp;query=Barrette%2C+J">J. Barrette</a>, <a href="/search/physics?searchtype=author&amp;query=Bellwied%2C+R">R. Bellwied</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+S">S. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Bersch%2C+R">R. Bersch</a>, <a href="/search/physics?searchtype=author&amp;query=Braun-Munzinger%2C+P">P. Braun-Munzinger</a>, <a href="/search/physics?searchtype=author&amp;query=Chang%2C+W+C">W. C. Chang</a>, <a href="/search/physics?searchtype=author&amp;query=Cleland%2C+W+E">W. E. Cleland</a>, <a href="/search/physics?searchtype=author&amp;query=Cole%2C+J+D">J. D. Cole</a>, <a href="/search/physics?searchtype=author&amp;query=Cormier%2C+T+M">T. M. Cormier</a>, <a href="/search/physics?searchtype=author&amp;query=David%2C+G">G. David</a>, <a href="/search/physics?searchtype=author&amp;query=Dee%2C+J">J. Dee</a>, <a href="/search/physics?searchtype=author&amp;query=Dietzsch%2C+O">O. Dietzsch</a>, <a href="/search/physics?searchtype=author&amp;query=Drigert%2C+M+W">M. W. Drigert</a>, <a href="/search/physics?searchtype=author&amp;query=Gilbert%2C+S">S. Gilbert</a>, <a href="/search/physics?searchtype=author&amp;query=Hall%2C+J+R">J. R. Hall</a>, <a href="/search/physics?searchtype=author&amp;query=Hemmick%2C+T+K">T. K. Hemmick</a>, <a href="/search/physics?searchtype=author&amp;query=Herrmann%2C+N">N. Herrmann</a>, <a href="/search/physics?searchtype=author&amp;query=Hong%2C+B">B. Hong</a>, <a href="/search/physics?searchtype=author&amp;query=Jiang%2C+C+L">C. L. Jiang</a>, <a href="/search/physics?searchtype=author&amp;query=Johnson%2C+S+C">S. C. Johnson</a>, <a href="/search/physics?searchtype=author&amp;query=Kwon%2C+Y">Y. Kwon</a>, <a href="/search/physics?searchtype=author&amp;query=Lacasse%2C+R">R. Lacasse</a>, <a href="/search/physics?searchtype=author&amp;query=Lukaszew%2C+A">A. Lukaszew</a>, <a href="/search/physics?searchtype=author&amp;query=Li%2C+Q">Q. Li</a> , et al. (26 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="physics/9702008v1-abstract-short" style="display: inline;"> Two-particle correlation functions for positive and negative pions have been measured in Au+Au collisions at 10.8~GeV/c per nucleon. The data were analyzed using one- and three-dimensional correlation functions. From the results of the three-dimensional fit the phase space density of pions was calculated. It is consistent with local thermal equilibrium. </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/9702008v1-abstract-full" style="display: none;"> Two-particle correlation functions for positive and negative pions have been measured in Au+Au collisions at 10.8~GeV/c per nucleon. The data were analyzed using one- and three-dimensional correlation functions. From the results of the three-dimensional fit the phase space density of pions was calculated. It is consistent with local thermal equilibrium. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/9702008v1-abstract-full').style.display = 'none'; document.getElementById('physics/9702008v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 7 February, 1997; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 1997. </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">5 pages RevTeX (including 3 Figures)</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.Lett.78:2916-2919,1997 </p> </li> </ol> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <span class="help" style="display: inline-block;"><a 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