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name="searchtype"><option value="all">All fields</option><option value="title">Title</option><option selected value="author">Author(s)</option><option value="abstract">Abstract</option><option value="comments">Comments</option><option value="journal_ref">Journal reference</option><option value="acm_class">ACM classification</option><option value="msc_class">MSC classification</option><option value="report_num">Report number</option><option value="paper_id">arXiv identifier</option><option value="doi">DOI</option><option value="orcid">ORCID</option><option value="license">License (URI)</option><option value="author_id">arXiv author ID</option><option value="help">Help pages</option><option value="full_text">Full text</option></select> <input id="query" name="query" type="text" value="Yao, X"> <ul id="abstracts"><li><input checked id="abstracts-0" name="abstracts" type="radio" value="show"> <label for="abstracts-0">Show abstracts</label></li><li><input id="abstracts-1" name="abstracts" type="radio" value="hide"> <label for="abstracts-1">Hide abstracts</label></li></ul> </div> <div class="box field is-grouped is-grouped-multiline level-item"> <div class="control"> <span class="select is-small"> <select id="size" name="size"><option value="25">25</option><option selected value="50">50</option><option value="100">100</option><option value="200">200</option></select> </span> <label for="size">results per page</label>. </div> <div class="control"> <label for="order">Sort results by</label> <span class="select is-small"> <select id="order" name="order"><option selected value="-announced_date_first">Announcement date (newest first)</option><option value="announced_date_first">Announcement date (oldest first)</option><option value="-submitted_date">Submission date (newest first)</option><option value="submitted_date">Submission date (oldest first)</option><option value="">Relevance</option></select> </span> </div> <div class="control"> <button class="button is-small is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2409.11710">arXiv:2409.11710</a> <span> [<a href="https://arxiv.org/pdf/2409.11710">pdf</a>, <a href="https://arxiv.org/ps/2409.11710">ps</a>, <a href="https://arxiv.org/format/2409.11710">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Solar and Stellar Astrophysics">astro-ph.SR</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.3847/1538-4357/ad7b26">10.3847/1538-4357/ad7b26 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Photo-nuclear reaction rates of $^{157,159}$Ho and $^{163,165}$Tm and their impact in the $纬$--process </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&query=Cheng%2C+H">Hao Cheng</a>, <a href="/search/nucl-ex?searchtype=author&query=Sun%2C+B">Bao-Hua Sun</a>, <a href="/search/nucl-ex?searchtype=author&query=Zhu%2C+L">Li-Hua Zhu</a>, <a href="/search/nucl-ex?searchtype=author&query=Kusakabe%2C+M">Motohiko Kusakabe</a>, <a href="/search/nucl-ex?searchtype=author&query=Luo%2C+Y">Yudong Luo</a>, <a href="/search/nucl-ex?searchtype=author&query=Kajino%2C+T">Toshitaka Kajino</a>, <a href="/search/nucl-ex?searchtype=author&query=Wang%2C+C">Chang-Jian Wang</a>, <a href="/search/nucl-ex?searchtype=author&query=Yao%2C+X">Xing-Qun Yao</a>, <a href="/search/nucl-ex?searchtype=author&query=He%2C+C">Chuang-Ye He</a>, <a href="/search/nucl-ex?searchtype=author&query=Liu%2C+F">Fu-Long Liu</a>, <a href="/search/nucl-ex?searchtype=author&query=Guo%2C+B">Bing Guo</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="2409.11710v1-abstract-short" style="display: inline;"> Reliable photo-nuclear reaction rates at the stellar conditions are essential to understand the origin of the heavy stable neutron-deficient isotopes between $^{74}$Se and $^{196}$Hg-p-nuclei, however, many reaction rates of relevance still have to rely on the Hauser-Feshbach model due to rare experimental progress. One such case is in the mass range of 160 for Dy, Er, Ho and Tm isotopes. In this… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2409.11710v1-abstract-full').style.display = 'inline'; document.getElementById('2409.11710v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2409.11710v1-abstract-full" style="display: none;"> Reliable photo-nuclear reaction rates at the stellar conditions are essential to understand the origin of the heavy stable neutron-deficient isotopes between $^{74}$Se and $^{196}$Hg-p-nuclei, however, many reaction rates of relevance still have to rely on the Hauser-Feshbach model due to rare experimental progress. One such case is in the mass range of 160 for Dy, Er, Ho and Tm isotopes. In this work we attempt to constrain the Hauser-Feshbach model in the TALYS package by reproducing the available experimental data of $^{160}$Dy($p,纬$)$^{161}$Ho and $^{162}$Er($p,纬$)$^{163}$Tm in the $A\sim 160$ mass region, and examine the effects of level density, gamma strength function and the optical model potential. The constrained model then allows us to calculate the reaction rates of $^{157, 159}$Ho($纬$, $p$) and $^{163,165}$Tm($纬$, $p$) for the $纬$-process nucleosynthesis in carbon-deflagration SNe Ia model. Our recommended rates differ from the JINA REACLIB by more than 1 order of magnitude in the temperature range of 2-3 GK. This results in the changes of final abundance of $p$-nuclei in the $A\sim 160$ mass range by -5.5-3\% from those with JINA, which means that the ($纬$, $p$) reactions uncertainty is not predominant for the synthesis of these nuclei. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2409.11710v1-abstract-full').style.display = 'none'; document.getElementById('2409.11710v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 September, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">12 pages,7 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Astrophysics Journal 975(2024)161 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2409.03691">arXiv:2409.03691</a> <span> [<a href="https://arxiv.org/pdf/2409.03691">pdf</a>, <a href="https://arxiv.org/format/2409.03691">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> </div> <p class="title is-5 mathjax"> Physics case for quarkonium studies at the Electron Ion Collider </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&query=Boer%2C+D">Dani毛l Boer</a>, <a href="/search/nucl-ex?searchtype=author&query=Flett%2C+C+A">Chris A. Flett</a>, <a href="/search/nucl-ex?searchtype=author&query=Flore%2C+C">Carlo Flore</a>, <a href="/search/nucl-ex?searchtype=author&query=Kiko%C5%82a%2C+D">Daniel Kiko艂a</a>, <a href="/search/nucl-ex?searchtype=author&query=Lansberg%2C+J">Jean-Philippe Lansberg</a>, <a href="/search/nucl-ex?searchtype=author&query=Nefedov%2C+M">Maxim Nefedov</a>, <a href="/search/nucl-ex?searchtype=author&query=Van+Hulse%2C+C">Charlotte Van Hulse</a>, <a href="/search/nucl-ex?searchtype=author&query=Bhattacharya%2C+S">Shohini Bhattacharya</a>, <a href="/search/nucl-ex?searchtype=author&query=Bor%2C+J">Jelle Bor</a>, <a href="/search/nucl-ex?searchtype=author&query=Butenschoen%2C+M">Mathias Butenschoen</a>, <a href="/search/nucl-ex?searchtype=author&query=Ceccopieri%2C+F">Federico Ceccopieri</a>, <a href="/search/nucl-ex?searchtype=author&query=Chen%2C+L">Longjie Chen</a>, <a href="/search/nucl-ex?searchtype=author&query=Cheung%2C+V">Vincent Cheung</a>, <a href="/search/nucl-ex?searchtype=author&query=D%27Alesio%2C+U">Umberto D'Alesio</a>, <a href="/search/nucl-ex?searchtype=author&query=Echevarria%2C+M">Miguel Echevarria</a>, <a href="/search/nucl-ex?searchtype=author&query=Hatta%2C+Y">Yoshitaka Hatta</a>, <a href="/search/nucl-ex?searchtype=author&query=Hyde%2C+C+E">Charles E. Hyde</a>, <a href="/search/nucl-ex?searchtype=author&query=Kishore%2C+R">Raj Kishore</a>, <a href="/search/nucl-ex?searchtype=author&query=Kosarzewski%2C+L">Leszek Kosarzewski</a>, <a href="/search/nucl-ex?searchtype=author&query=Lorc%C3%A9%2C+C">C茅dric Lorc茅</a>, <a href="/search/nucl-ex?searchtype=author&query=Li%2C+W">Wenliang Li</a>, <a href="/search/nucl-ex?searchtype=author&query=Li%2C+X">Xuan Li</a>, <a href="/search/nucl-ex?searchtype=author&query=Maxia%2C+L">Luca Maxia</a>, <a href="/search/nucl-ex?searchtype=author&query=Metz%2C+A">Andreas Metz</a>, <a href="/search/nucl-ex?searchtype=author&query=Mukherjee%2C+A">Asmita Mukherjee</a> , et al. (19 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="2409.03691v1-abstract-short" style="display: inline;"> The physics case for quarkonium-production studies accessible at the US Electron Ion Collider is described. </span> <span class="abstract-full has-text-grey-dark mathjax" id="2409.03691v1-abstract-full" style="display: none;"> The physics case for quarkonium-production studies accessible at the US Electron Ion Collider is described. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2409.03691v1-abstract-full').style.display = 'none'; document.getElementById('2409.03691v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 September, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Latex, 84 pages. Review prepared for Progress in Particle and Nuclear Physics</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2303.17254">arXiv:2303.17254</a> <span> [<a href="https://arxiv.org/pdf/2303.17254">pdf</a>, <a href="https://arxiv.org/format/2303.17254">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> </div> <p class="title is-5 mathjax"> Hot QCD White Paper </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&query=Arslandok%2C+M">M. Arslandok</a>, <a href="/search/nucl-ex?searchtype=author&query=Bass%2C+S+A">S. A. Bass</a>, <a href="/search/nucl-ex?searchtype=author&query=Baty%2C+A+A">A. A. Baty</a>, <a href="/search/nucl-ex?searchtype=author&query=Bautista%2C+I">I. Bautista</a>, <a href="/search/nucl-ex?searchtype=author&query=Beattie%2C+C">C. Beattie</a>, <a href="/search/nucl-ex?searchtype=author&query=Becattini%2C+F">F. Becattini</a>, <a href="/search/nucl-ex?searchtype=author&query=Bellwied%2C+R">R. Bellwied</a>, <a href="/search/nucl-ex?searchtype=author&query=Berdnikov%2C+Y">Y. Berdnikov</a>, <a href="/search/nucl-ex?searchtype=author&query=Berdnikov%2C+A">A. Berdnikov</a>, <a href="/search/nucl-ex?searchtype=author&query=Bielcik%2C+J">J. Bielcik</a>, <a href="/search/nucl-ex?searchtype=author&query=Blair%2C+J+T">J. T. Blair</a>, <a href="/search/nucl-ex?searchtype=author&query=Bock%2C+F">F. Bock</a>, <a href="/search/nucl-ex?searchtype=author&query=Boimska%2C+B">B. Boimska</a>, <a href="/search/nucl-ex?searchtype=author&query=Bossi%2C+H">H. Bossi</a>, <a href="/search/nucl-ex?searchtype=author&query=Caines%2C+H">H. Caines</a>, <a href="/search/nucl-ex?searchtype=author&query=Chen%2C+Y">Y. Chen</a>, <a href="/search/nucl-ex?searchtype=author&query=Chien%2C+Y+-">Y. -T. Chien</a>, <a href="/search/nucl-ex?searchtype=author&query=Chiu%2C+M">M. Chiu</a>, <a href="/search/nucl-ex?searchtype=author&query=Connors%2C+M+E">M. E. Connors</a>, <a href="/search/nucl-ex?searchtype=author&query=Csan%C3%A1d%2C+M">M. Csan谩d</a>, <a href="/search/nucl-ex?searchtype=author&query=da+Silva%2C+C+L">C. L. da Silva</a>, <a href="/search/nucl-ex?searchtype=author&query=Dash%2C+A+P">A. P. Dash</a>, <a href="/search/nucl-ex?searchtype=author&query=David%2C+G">G. David</a>, <a href="/search/nucl-ex?searchtype=author&query=Dehmelt%2C+K">K. Dehmelt</a>, <a href="/search/nucl-ex?searchtype=author&query=Dexheimer%2C+V">V. Dexheimer</a> , et al. (149 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="2303.17254v1-abstract-short" style="display: inline;"> Hot QCD physics studies the nuclear strong force under extreme temperature and densities. Experimentally these conditions are achieved via high-energy collisions of heavy ions at the Relativistic Heavy Ion Collider (RHIC) and the Large Hadron Collider (LHC). In the past decade, a unique and substantial suite of data was collected at RHIC and the LHC, probing hydrodynamics at the nucleon scale, the… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2303.17254v1-abstract-full').style.display = 'inline'; document.getElementById('2303.17254v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2303.17254v1-abstract-full" style="display: none;"> Hot QCD physics studies the nuclear strong force under extreme temperature and densities. Experimentally these conditions are achieved via high-energy collisions of heavy ions at the Relativistic Heavy Ion Collider (RHIC) and the Large Hadron Collider (LHC). In the past decade, a unique and substantial suite of data was collected at RHIC and the LHC, probing hydrodynamics at the nucleon scale, the temperature dependence of the transport properties of quark-gluon plasma, the phase diagram of nuclear matter, the interaction of quarks and gluons at different scales and much more. This document, as part of the 2023 nuclear science long range planning process, was written to review the progress in hot QCD since the 2015 Long Range Plan for Nuclear Science, as well as highlight the realization of previous recommendations, and present opportunities for the next decade, building on the accomplishments and investments made in theoretical developments and the construction of new detectors. Furthermore, this document provides additional context to support the recommendations voted on at the Joint Hot and Cold QCD Town Hall Meeting, which are reported in a separate document. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2303.17254v1-abstract-full').style.display = 'none'; document.getElementById('2303.17254v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 March, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 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">190 pages, 69 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/2303.02579">arXiv:2303.02579</a> <span> [<a href="https://arxiv.org/pdf/2303.02579">pdf</a>, <a href="https://arxiv.org/format/2303.02579">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nuclphysa.2024.122874">10.1016/j.nuclphysa.2024.122874 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The Present and Future of QCD </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&query=Achenbach%2C+P">P. Achenbach</a>, <a href="/search/nucl-ex?searchtype=author&query=Adhikari%2C+D">D. Adhikari</a>, <a href="/search/nucl-ex?searchtype=author&query=Afanasev%2C+A">A. Afanasev</a>, <a href="/search/nucl-ex?searchtype=author&query=Afzal%2C+F">F. Afzal</a>, <a href="/search/nucl-ex?searchtype=author&query=Aidala%2C+C+A">C. A. Aidala</a>, <a href="/search/nucl-ex?searchtype=author&query=Al-bataineh%2C+A">A. Al-bataineh</a>, <a href="/search/nucl-ex?searchtype=author&query=Almaalol%2C+D+K">D. K. Almaalol</a>, <a href="/search/nucl-ex?searchtype=author&query=Amaryan%2C+M">M. Amaryan</a>, <a href="/search/nucl-ex?searchtype=author&query=Androi%C4%87%2C+D">D. Androi膰</a>, <a href="/search/nucl-ex?searchtype=author&query=Armstrong%2C+W+R">W. R. Armstrong</a>, <a href="/search/nucl-ex?searchtype=author&query=Arratia%2C+M">M. Arratia</a>, <a href="/search/nucl-ex?searchtype=author&query=Arrington%2C+J">J. Arrington</a>, <a href="/search/nucl-ex?searchtype=author&query=Asaturyan%2C+A">A. Asaturyan</a>, <a href="/search/nucl-ex?searchtype=author&query=Aschenauer%2C+E+C">E. C. Aschenauer</a>, <a href="/search/nucl-ex?searchtype=author&query=Atac%2C+H">H. Atac</a>, <a href="/search/nucl-ex?searchtype=author&query=Avakian%2C+H">H. Avakian</a>, <a href="/search/nucl-ex?searchtype=author&query=Averett%2C+T">T. Averett</a>, <a href="/search/nucl-ex?searchtype=author&query=Gayoso%2C+C+A">C. Ayerbe Gayoso</a>, <a href="/search/nucl-ex?searchtype=author&query=Bai%2C+X">X. Bai</a>, <a href="/search/nucl-ex?searchtype=author&query=Barish%2C+K+N">K. N. Barish</a>, <a href="/search/nucl-ex?searchtype=author&query=Barnea%2C+N">N. Barnea</a>, <a href="/search/nucl-ex?searchtype=author&query=Basar%2C+G">G. Basar</a>, <a href="/search/nucl-ex?searchtype=author&query=Battaglieri%2C+M">M. Battaglieri</a>, <a href="/search/nucl-ex?searchtype=author&query=Baty%2C+A+A">A. A. Baty</a>, <a href="/search/nucl-ex?searchtype=author&query=Bautista%2C+I">I. Bautista</a> , et al. (378 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="2303.02579v1-abstract-short" style="display: inline;"> This White Paper presents the community inputs and scientific conclusions from the Hot and Cold QCD Town Meeting that took place September 23-25, 2022 at MIT, as part of the Nuclear Science Advisory Committee (NSAC) 2023 Long Range Planning process. A total of 424 physicists registered for the meeting. The meeting highlighted progress in Quantum Chromodynamics (QCD) nuclear physics since the 2015… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2303.02579v1-abstract-full').style.display = 'inline'; document.getElementById('2303.02579v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2303.02579v1-abstract-full" style="display: none;"> This White Paper presents the community inputs and scientific conclusions from the Hot and Cold QCD Town Meeting that took place September 23-25, 2022 at MIT, as part of the Nuclear Science Advisory Committee (NSAC) 2023 Long Range Planning process. A total of 424 physicists registered for the meeting. The meeting highlighted progress in Quantum Chromodynamics (QCD) nuclear physics since the 2015 LRP (LRP15) and identified key questions and plausible paths to obtaining answers to those questions, defining priorities for our research over the coming decade. In defining the priority of outstanding physics opportunities for the future, both prospects for the short (~ 5 years) and longer term (5-10 years and beyond) are identified together with the facilities, personnel and other resources needed to maximize the discovery potential and maintain United States leadership in QCD physics worldwide. This White Paper is organized as follows: In the Executive Summary, we detail the Recommendations and Initiatives that were presented and discussed at the Town Meeting, and their supporting rationales. Section 2 highlights major progress and accomplishments of the past seven years. It is followed, in Section 3, by an overview of the physics opportunities for the immediate future, and in relation with the next QCD frontier: the EIC. Section 4 provides an overview of the physics motivations and goals associated with the EIC. Section 5 is devoted to the workforce development and support of diversity, equity and inclusion. This is followed by a dedicated section on computing in Section 6. Section 7 describes the national need for nuclear data science and the relevance to QCD research. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2303.02579v1-abstract-full').style.display = 'none'; document.getElementById('2303.02579v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 4 March, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 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">QCD Town Meeting White Paper, as submitted to 2023 NSAC LRP committee on Feb. 28, 2023</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nucl.Phys.A 1047 (2024) 122874 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2303.00113">arXiv:2303.00113</a> <span> [<a href="https://arxiv.org/pdf/2303.00113">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</span> </div> </div> <p class="title is-5 mathjax"> Quantum Information Science and Technology for Nuclear Physics. Input into U.S. Long-Range Planning, 2023 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&query=Beck%2C+D">Douglas Beck</a>, <a href="/search/nucl-ex?searchtype=author&query=Carlson%2C+J">Joseph Carlson</a>, <a href="/search/nucl-ex?searchtype=author&query=Davoudi%2C+Z">Zohreh Davoudi</a>, <a href="/search/nucl-ex?searchtype=author&query=Formaggio%2C+J">Joseph Formaggio</a>, <a href="/search/nucl-ex?searchtype=author&query=Quaglioni%2C+S">Sofia Quaglioni</a>, <a href="/search/nucl-ex?searchtype=author&query=Savage%2C+M">Martin Savage</a>, <a href="/search/nucl-ex?searchtype=author&query=Barata%2C+J">Joao Barata</a>, <a href="/search/nucl-ex?searchtype=author&query=Bhattacharya%2C+T">Tanmoy Bhattacharya</a>, <a href="/search/nucl-ex?searchtype=author&query=Bishof%2C+M">Michael Bishof</a>, <a href="/search/nucl-ex?searchtype=author&query=Cloet%2C+I">Ian Cloet</a>, <a href="/search/nucl-ex?searchtype=author&query=Delgado%2C+A">Andrea Delgado</a>, <a href="/search/nucl-ex?searchtype=author&query=DeMarco%2C+M">Michael DeMarco</a>, <a href="/search/nucl-ex?searchtype=author&query=Fink%2C+C">Caleb Fink</a>, <a href="/search/nucl-ex?searchtype=author&query=Florio%2C+A">Adrien Florio</a>, <a href="/search/nucl-ex?searchtype=author&query=Francois%2C+M">Marianne Francois</a>, <a href="/search/nucl-ex?searchtype=author&query=Grabowska%2C+D">Dorota Grabowska</a>, <a href="/search/nucl-ex?searchtype=author&query=Hoogerheide%2C+S">Shannon Hoogerheide</a>, <a href="/search/nucl-ex?searchtype=author&query=Huang%2C+M">Mengyao Huang</a>, <a href="/search/nucl-ex?searchtype=author&query=Ikeda%2C+K">Kazuki Ikeda</a>, <a href="/search/nucl-ex?searchtype=author&query=Illa%2C+M">Marc Illa</a>, <a href="/search/nucl-ex?searchtype=author&query=Joo%2C+K">Kyungseon Joo</a>, <a href="/search/nucl-ex?searchtype=author&query=Kharzeev%2C+D">Dmitri Kharzeev</a>, <a href="/search/nucl-ex?searchtype=author&query=Kowalski%2C+K">Karol Kowalski</a>, <a href="/search/nucl-ex?searchtype=author&query=Lai%2C+W+K">Wai Kin Lai</a>, <a href="/search/nucl-ex?searchtype=author&query=Leach%2C+K">Kyle Leach</a> , et al. (76 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="2303.00113v1-abstract-short" style="display: inline;"> In preparation for the 2023 NSAC Long Range Plan (LRP), members of the Nuclear Science community gathered to discuss the current state of, and plans for further leveraging opportunities in, QIST in NP research at the Quantum Information Science for U.S. Nuclear Physics Long Range Planning workshop, held in Santa Fe, New Mexico on January 31 - February 1, 2023. The workshop included 45 in-person pa… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2303.00113v1-abstract-full').style.display = 'inline'; document.getElementById('2303.00113v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2303.00113v1-abstract-full" style="display: none;"> In preparation for the 2023 NSAC Long Range Plan (LRP), members of the Nuclear Science community gathered to discuss the current state of, and plans for further leveraging opportunities in, QIST in NP research at the Quantum Information Science for U.S. Nuclear Physics Long Range Planning workshop, held in Santa Fe, New Mexico on January 31 - February 1, 2023. The workshop included 45 in-person participants and 53 remote attendees. The outcome of the workshop identified strategic plans and requirements for the next 5-10 years to advance quantum sensing and quantum simulations within NP, and to develop a diverse quantum-ready workforce. The plans include resolutions endorsed by the participants to address the compelling scientific opportunities at the intersections of NP and QIST. These endorsements are aligned with similar affirmations by the LRP Computational Nuclear Physics and AI/ML Workshop, the Nuclear Structure, Reactions, and Astrophysics LRP Town Hall, and the Fundamental Symmetries, Neutrons, and Neutrinos LRP Town Hall communities. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2303.00113v1-abstract-full').style.display = 'none'; document.getElementById('2303.00113v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 28 February, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 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">A white paper for the 2023 nuclear physics long-range planning activity, emerging from the workshop "Quantum Information Science for U.S. Nuclear Physics Long Range Planning'', held in Santa Fe, New Mexico on January 31 - February 1, 2023. 26 pages with 7 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/2108.06245">arXiv:2108.06245</a> <span> [<a href="https://arxiv.org/pdf/2108.06245">pdf</a>, <a href="https://arxiv.org/format/2108.06245">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Alpha-decay-correlated mass measurement of 206,207Ra using an $伪$-TOF detector equipped MRTOF-MS system </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&query=Niwase%2C+T">T. Niwase</a>, <a href="/search/nucl-ex?searchtype=author&query=Wada%2C+M">M. Wada</a>, <a href="/search/nucl-ex?searchtype=author&query=Schury%2C+P">P Schury</a>, <a href="/search/nucl-ex?searchtype=author&query=Brionnet%2C+P">P. Brionnet</a>, <a href="/search/nucl-ex?searchtype=author&query=Chen%2C+S+D">S. D. Chen</a>, <a href="/search/nucl-ex?searchtype=author&query=Hashimoto%2C+T">T. Hashimoto</a>, <a href="/search/nucl-ex?searchtype=author&query=Haba%2C+H">H. Haba</a>, <a href="/search/nucl-ex?searchtype=author&query=Hirayama%2C+Y">Y. Hirayama</a>, <a href="/search/nucl-ex?searchtype=author&query=Hou%2C+D+S">D. S. Hou</a>, <a href="/search/nucl-ex?searchtype=author&query=Iimura%2C+S">S. Iimura</a>, <a href="/search/nucl-ex?searchtype=author&query=Ishiyama%2C+H">H. Ishiyama</a>, <a href="/search/nucl-ex?searchtype=author&query=Ishizawa%2C+S">S. Ishizawa</a>, <a href="/search/nucl-ex?searchtype=author&query=Ito%2C+Y">Y. Ito</a>, <a href="/search/nucl-ex?searchtype=author&query=Kaji%2C+D">D. Kaji</a>, <a href="/search/nucl-ex?searchtype=author&query=Kimura%2C+S">S. Kimura</a>, <a href="/search/nucl-ex?searchtype=author&query=Liu%2C+J">J. Liu</a>, <a href="/search/nucl-ex?searchtype=author&query=Miyatake%2C+H">H. Miyatake</a>, <a href="/search/nucl-ex?searchtype=author&query=Moon%2C+J+Y">J. Y. Moon</a>, <a href="/search/nucl-ex?searchtype=author&query=Morimoto%2C+K">K. Morimoto</a>, <a href="/search/nucl-ex?searchtype=author&query=Morita%2C+K">K. Morita</a>, <a href="/search/nucl-ex?searchtype=author&query=Nagae%2C+D">D. Nagae</a>, <a href="/search/nucl-ex?searchtype=author&query=Rosenbusch%2C+M">M. Rosenbusch</a>, <a href="/search/nucl-ex?searchtype=author&query=Takamine%2C+A">A. Takamine</a>, <a href="/search/nucl-ex?searchtype=author&query=Tanaka%2C+T">T. Tanaka</a>, <a href="/search/nucl-ex?searchtype=author&query=Watanabe%2C+Y+X">Y. X. Watanabe</a> , et al. (3 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="2108.06245v2-abstract-short" style="display: inline;"> The atomic masses of the isotopes $^{206,207}$Ra have been measured via decay-correlated mass spectroscopy using a multi-reflection time-of-flight mass spectrograph equipped with an $伪$-TOF detector. The Ra isotopes were produced as fusion-evaporation products in the $^{51}$V+$^{159}$Tb reaction system and delivered by the gas-filled recoil ion separator GARIS-II at RIKEN. The $伪$-TOF detector pro… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2108.06245v2-abstract-full').style.display = 'inline'; document.getElementById('2108.06245v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2108.06245v2-abstract-full" style="display: none;"> The atomic masses of the isotopes $^{206,207}$Ra have been measured via decay-correlated mass spectroscopy using a multi-reflection time-of-flight mass spectrograph equipped with an $伪$-TOF detector. The Ra isotopes were produced as fusion-evaporation products in the $^{51}$V+$^{159}$Tb reaction system and delivered by the gas-filled recoil ion separator GARIS-II at RIKEN. The $伪$-TOF detector provides for high-accuracy mass measurements by correlating time-of-flight signals with subsequent $伪$-decay events. The masses of $^{206}$Ra and $^{207g,m}$Ra were directly measured using a multi-reflection time-of-flight mass spectrograph equipped with an $伪$-TOF detector. A mass excess of ME = 3538(15) keV/c$^2$ and an excitation energy of E$_{\rm ex}$ = 552(42) keV were determined. The $伪$-decay branching ratio of $^{207m}$Ra, b$伪$ = 0.26(20), was directly determined from decay-correlated time-of-flight signals, and the reduced alpha width of $^{207m}$Ra was calculated to be $未^2$ = 50+62-41 keV from the branching ratio. The spin-parity of $^{207m}$Ra was confirmed to be $J^蟺$ = 13/2$^-$ from decay correlated mass measurement results. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2108.06245v2-abstract-full').style.display = 'none'; document.getElementById('2108.06245v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 October, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 13 August, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2021. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2012.14161">arXiv:2012.14161</a> <span> [<a href="https://arxiv.org/pdf/2012.14161">pdf</a>, <a href="https://arxiv.org/format/2012.14161">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.ppnp.2021.103906">10.1016/j.ppnp.2021.103906 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Prospects for quarkonium studies at the high-luminosity LHC </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&query=Chapon%2C+E">Emilien Chapon</a>, <a href="/search/nucl-ex?searchtype=author&query=d%27Enterria%2C+D">David d'Enterria</a>, <a href="/search/nucl-ex?searchtype=author&query=Ducloue%2C+B">Bertrand Ducloue</a>, <a href="/search/nucl-ex?searchtype=author&query=Echevarria%2C+M+G">Miguel G. Echevarria</a>, <a href="/search/nucl-ex?searchtype=author&query=Gossiaux%2C+P">Pol-Bernard Gossiaux</a>, <a href="/search/nucl-ex?searchtype=author&query=Kartvelishvili%2C+V">Vato Kartvelishvili</a>, <a href="/search/nucl-ex?searchtype=author&query=Kasemets%2C+T">Tomas Kasemets</a>, <a href="/search/nucl-ex?searchtype=author&query=Lansberg%2C+J">Jean-Philippe Lansberg</a>, <a href="/search/nucl-ex?searchtype=author&query=McNulty%2C+R">Ronan McNulty</a>, <a href="/search/nucl-ex?searchtype=author&query=Price%2C+D+D">Darren D. Price</a>, <a href="/search/nucl-ex?searchtype=author&query=Shao%2C+H">Hua-Sheng Shao</a>, <a href="/search/nucl-ex?searchtype=author&query=Van+Hulse%2C+C">Charlotte Van Hulse</a>, <a href="/search/nucl-ex?searchtype=author&query=Winn%2C+M">Michael Winn</a>, <a href="/search/nucl-ex?searchtype=author&query=Adam%2C+J">Jaroslav Adam</a>, <a href="/search/nucl-ex?searchtype=author&query=An%2C+L">Liupan An</a>, <a href="/search/nucl-ex?searchtype=author&query=Villar%2C+D+Y+A">Denys Yen Arrebato Villar</a>, <a href="/search/nucl-ex?searchtype=author&query=Bhattacharya%2C+S">Shohini Bhattacharya</a>, <a href="/search/nucl-ex?searchtype=author&query=Celiberto%2C+F+G">Francesco G. Celiberto</a>, <a href="/search/nucl-ex?searchtype=author&query=Cheshkov%2C+C">Cvetan Cheshkov</a>, <a href="/search/nucl-ex?searchtype=author&query=D%27Alesio%2C+U">Umberto D'Alesio</a>, <a href="/search/nucl-ex?searchtype=author&query=da+Silva%2C+C">Cesar da Silva</a>, <a href="/search/nucl-ex?searchtype=author&query=Ferreiro%2C+E+G">Elena G. Ferreiro</a>, <a href="/search/nucl-ex?searchtype=author&query=Flett%2C+C+A">Chris A. Flett</a>, <a href="/search/nucl-ex?searchtype=author&query=Flore%2C+C">Carlo Flore</a>, <a href="/search/nucl-ex?searchtype=author&query=Garzelli%2C+M+V">Maria Vittoria Garzelli</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="2012.14161v2-abstract-short" style="display: inline;"> Prospects for quarkonium-production studies accessible during the upcoming high-luminosity phases of the CERN Large Hadron Collider operation after 2021 are reviewed. Current experimental and theoretical open issues in the field are assessed together with the potential for future studies in quarkonium-related physics. This will be possible through the exploitation of the huge data samples to be co… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.14161v2-abstract-full').style.display = 'inline'; document.getElementById('2012.14161v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2012.14161v2-abstract-full" style="display: none;"> Prospects for quarkonium-production studies accessible during the upcoming high-luminosity phases of the CERN Large Hadron Collider operation after 2021 are reviewed. Current experimental and theoretical open issues in the field are assessed together with the potential for future studies in quarkonium-related physics. This will be possible through the exploitation of the huge data samples to be collected in proton-proton, proton-nucleus and nucleus-nucleus collisions, both in the collider and fixed-target modes. Such investigations include, among others, those of: (i) J/psi and Upsilon produced in association with other hard particles; (ii) chi(c,b) and eta(c,b) down to small transverse momenta; (iii) the constraints brought in by quarkonia on gluon PDFs, nuclear PDFs, TMDs, GPDs and GTMDs, as well as on the low-x parton dynamics; (iv) the gluon Sivers effect in polarised-nucleon collisions; (v) the properties of the quark-gluon plasma produced in ultra-relativistic heavy-ion collisions and of collective partonic effects in general; and (vi) double and triple parton scatterings. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.14161v2-abstract-full').style.display = 'none'; document.getElementById('2012.14161v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 November, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 28 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">Latex, 115 pages, 55 figures, 4 tables. v2: Review published in Progress in Particle and Nuclear Physics</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> MIT-CTP/5231 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Progress in Particle and Nuclear Physics 122 (2022) 103906 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2010.03571">arXiv:2010.03571</a> <span> [<a href="https://arxiv.org/pdf/2010.03571">pdf</a>, <a href="https://arxiv.org/format/2010.03571">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</span> </div> <div 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/PhysRevD.104.L051501">10.1103/PhysRevD.104.L051501 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Quantum simulation of open quantum systems in heavy-ion collisions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&query=de+Jong%2C+W+A">Wibe A. de Jong</a>, <a href="/search/nucl-ex?searchtype=author&query=Metcalf%2C+M">Mekena Metcalf</a>, <a href="/search/nucl-ex?searchtype=author&query=Mulligan%2C+J">James Mulligan</a>, <a href="/search/nucl-ex?searchtype=author&query=P%C5%82osko%C5%84%2C+M">Mateusz P艂osko艅</a>, <a href="/search/nucl-ex?searchtype=author&query=Ringer%2C+F">Felix Ringer</a>, <a href="/search/nucl-ex?searchtype=author&query=Yao%2C+X">Xiaojun Yao</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="2010.03571v2-abstract-short" style="display: inline;"> We present a framework to simulate the dynamics of hard probes such as heavy quarks or jets in a hot, strongly-coupled quark-gluon plasma (QGP) on a quantum computer. Hard probes in the QGP can be treated as open quantum systems governed in the Markovian limit by the Lindblad equation. However, due to large computational costs, most current phenomenological calculations of hard probes evolving in… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2010.03571v2-abstract-full').style.display = 'inline'; document.getElementById('2010.03571v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2010.03571v2-abstract-full" style="display: none;"> We present a framework to simulate the dynamics of hard probes such as heavy quarks or jets in a hot, strongly-coupled quark-gluon plasma (QGP) on a quantum computer. Hard probes in the QGP can be treated as open quantum systems governed in the Markovian limit by the Lindblad equation. However, due to large computational costs, most current phenomenological calculations of hard probes evolving in the QGP use semiclassical approximations of the quantum evolution. Quantum computation can mitigate these costs, and offers the potential for a fully quantum treatment with exponential speedup over classical techniques. We report a simplified demonstration of our framework on IBM Q quantum devices, and apply the Random Identity Insertion Method (RIIM) to account for CNOT depolarization noise, in addition to measurement error mitigation. Our work demonstrates the feasibility of simulating open quantum systems on current and near-term quantum devices, which is of broad relevance to applications in nuclear physics, quantum information, and other fields. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2010.03571v2-abstract-full').style.display = 'none'; document.getElementById('2010.03571v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 7 September, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 7 October, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 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">Published in Phys Rev D</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> MIT-CTP/5247 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 104, 051501 (2021) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1801.02652">arXiv:1801.02652</a> <span> [<a href="https://arxiv.org/pdf/1801.02652">pdf</a>, <a href="https://arxiv.org/format/1801.02652">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.97.074003">10.1103/PhysRevD.97.074003 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Doubly charmed baryon production in heavy ion collisions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&query=Yao%2C+X">Xiaojun Yao</a>, <a href="/search/nucl-ex?searchtype=author&query=M%C3%BCller%2C+B">Berndt M眉ller</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="1801.02652v6-abstract-short" style="display: inline;"> We give an estimate of $螢_{cc}^{++}$ production rate and transverse momentum spectra in relativistic heavy ion collisions. We use Boltzmann transport equations to describe the dynamical evolution of charm quarks and diquarks inside quark-gluon plasma. In-medium formation and dissociation rates of charm diquarks are calculated from potential non-relativistic QCD for the diquark sector. We solve the… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1801.02652v6-abstract-full').style.display = 'inline'; document.getElementById('1801.02652v6-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1801.02652v6-abstract-full" style="display: none;"> We give an estimate of $螢_{cc}^{++}$ production rate and transverse momentum spectra in relativistic heavy ion collisions. We use Boltzmann transport equations to describe the dynamical evolution of charm quarks and diquarks inside quark-gluon plasma. In-medium formation and dissociation rates of charm diquarks are calculated from potential non-relativistic QCD for the diquark sector. We solve the transport equations by Monte Carlo simulations. For $2.76$ TeV Pb-Pb collisions with $0-10\%$ centrality, the number of $螢_{cc}^{++}$ produced in the transverse momentum range $0-5$ GeV and rapidity from $-1$ to $1$ is roughly $0.02$ per collision. We repeat the calculation with a melting temperature $250$ MeV above which no diquarks can be formed. The number of $螢_{cc}^{++}$ produced in the same kinematic region is about $0.0125$ per collision. We discuss how to study diquarks at finite temperature on a lattice and construct the anti-triplet free energy in a gauge invariant but path dependent way. We also comment on extensions of the calculation to other doubly heavy baryons and doubly heavy tetraquarks and the feasibility of experimental measurements. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1801.02652v6-abstract-full').style.display = 'none'; document.getElementById('1801.02652v6-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 3 April, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 8 January, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2018. </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, 3 figures, add a discussion of productions of other doubly heavy baryons and doubly heavy tetraquarks; add a discussion on diquark free energy on the lattice; add a comment on experimental feasibility; published version</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 97, 074003 (2018) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1709.03529">arXiv:1709.03529</a> <span> [<a href="https://arxiv.org/pdf/1709.03529">pdf</a>, <a href="https://arxiv.org/format/1709.03529">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.97.014908">10.1103/PhysRevC.97.014908 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Approach to equilibrium of quarkonium in quark-gluon plasma </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&query=Yao%2C+X">Xiaojun Yao</a>, <a href="/search/nucl-ex?searchtype=author&query=M%C3%BCller%2C+B">Berndt M眉ller</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="1709.03529v4-abstract-short" style="display: inline;"> We calculate the dissociation and recombination rates of $违(1S)$ in quark-gluon plasma by using potential non-relativistic QCD. We then study the dynamical in-medium evolution of the $b\bar{b}-违$ system in a periodic box via the Boltzmann equation and explore how the system reaches equilibrium. We find that interactions between the free heavy quarks and the medium are necessary for the system to r… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1709.03529v4-abstract-full').style.display = 'inline'; document.getElementById('1709.03529v4-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1709.03529v4-abstract-full" style="display: none;"> We calculate the dissociation and recombination rates of $违(1S)$ in quark-gluon plasma by using potential non-relativistic QCD. We then study the dynamical in-medium evolution of the $b\bar{b}-违$ system in a periodic box via the Boltzmann equation and explore how the system reaches equilibrium. We find that interactions between the free heavy quarks and the medium are necessary for the system to reach equilibrium. We find that the angular distribution of $违(1S)$ probes the stages at which recombination occurs. Finally, we study the system under a longitudinal expansion and show that different initial conditions evolve to distinct final ratios of hidden and open $b$ flavors. We argue that experimental measurements of the ratio could address open questions in the quarkonium production in heavy ion collisions. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1709.03529v4-abstract-full').style.display = 'none'; document.getElementById('1709.03529v4-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 April, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 11 September, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2017. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 5 figures, accepted version; a missing factor in Eq.(6) is added</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C 97, 014908 (2018) </p> </li> </ol> <div class="is-hidden-tablet">  <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a>  </span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary">  <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/about">About</a></li> <li><a href="https://info.arxiv.org/help">Help</a></li> </ul> </div> <div class="column"> <ul class="nav-spaced"> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>contact arXiv</title><desc>Click here to contact arXiv</desc><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg> <a href="https://info.arxiv.org/help/contact.html"> Contact</a> </li> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>subscribe to arXiv mailings</title><desc>Click here to subscribe</desc><path d="M476 3.2L12.5 270.6c-18.1 10.4-15.8 35.6 2.2 43.2L121 358.4l287.3-253.2c5.5-4.9 13.3 2.6 8.6 8.3L176 407v80.5c0 23.6 28.5 32.9 42.5 15.8L282 426l124.6 52.2c14.2 6 30.4-2.9 33-18.2l72-432C515 7.8 493.3-6.8 476 3.2z"/></svg> <a href="https://info.arxiv.org/help/subscribe"> Subscribe</a> </li> </ul> </div> </div> </div>   <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/license/index.html">Copyright</a></li> <li><a href="https://info.arxiv.org/help/policies/privacy_policy.html">Privacy Policy</a></li> </ul> </div> <div class="column sorry-app-links"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/web_accessibility.html">Web Accessibility Assistance</a></li> <li> <p class="help"> <a class="a11y-main-link" href="https://status.arxiv.org" target="_blank">arXiv Operational Status <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 256 512" class="icon filter-dark_grey" role="presentation"><path d="M224.3 273l-136 136c-9.4 9.4-24.6 9.4-33.9 0l-22.6-22.6c-9.4-9.4-9.4-24.6 0-33.9l96.4-96.4-96.4-96.4c-9.4-9.4-9.4-24.6 0-33.9L54.3 103c9.4-9.4 24.6-9.4 33.9 0l136 136c9.5 9.4 9.5 24.6.1 34z"/></svg></a><br> Get status notifications via <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/email/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg>email</a> or <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/slack/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 448 512" class="icon filter-black" role="presentation"><path d="M94.12 315.1c0 25.9-21.16 47.06-47.06 47.06S0 341 0 315.1c0-25.9 21.16-47.06 47.06-47.06h47.06v47.06zm23.72 0c0-25.9 21.16-47.06 47.06-47.06s47.06 21.16 47.06 47.06v117.84c0 25.9-21.16 47.06-47.06 47.06s-47.06-21.16-47.06-47.06V315.1zm47.06-188.98c-25.9 0-47.06-21.16-47.06-47.06S139 32 164.9 32s47.06 21.16 47.06 47.06v47.06H164.9zm0 23.72c25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06H47.06C21.16 243.96 0 222.8 0 196.9s21.16-47.06 47.06-47.06H164.9zm188.98 47.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06h-47.06V196.9zm-23.72 0c0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06V79.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06V196.9zM283.1 385.88c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06v-47.06h47.06zm0-23.72c-25.9 0-47.06-21.16-47.06-47.06 0-25.9 21.16-47.06 47.06-47.06h117.84c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06H283.1z"/></svg>slack</a> </p> </li> </ul> </div> </div> </div>  </div> </footer> <script src="https://static.arxiv.org/static/base/1.0.0a5/js/member_acknowledgement.js"></script> </body> </html>

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