CINXE.COM

Search | arXiv e-print repository

<!DOCTYPE html> <html lang="en"> <head> <meta charset="utf-8"/> <meta name="viewport" content="width=device-width, initial-scale=1"/> <!-- new favicon config and versions by realfavicongenerator.net --> <link rel="apple-touch-icon" sizes="180x180" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/apple-touch-icon.png"> <link rel="icon" type="image/png" sizes="32x32" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/favicon-32x32.png"> <link rel="icon" type="image/png" sizes="16x16" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/favicon-16x16.png"> <link rel="manifest" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/site.webmanifest"> <link rel="mask-icon" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/safari-pinned-tab.svg" color="#b31b1b"> <link rel="shortcut icon" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/favicon.ico"> <meta name="msapplication-TileColor" content="#b31b1b"> <meta name="msapplication-config" content="images/icons/browserconfig.xml"> <meta name="theme-color" content="#b31b1b"> <!-- end favicon config --> <title>Search | arXiv e-print repository</title> <script defer src="https://static.arxiv.org/static/base/1.0.0a5/fontawesome-free-5.11.2-web/js/all.js"></script> <link rel="stylesheet" href="https://static.arxiv.org/static/base/1.0.0a5/css/arxivstyle.css" /> <script type="text/x-mathjax-config"> MathJax.Hub.Config({ messageStyle: "none", extensions: ["tex2jax.js"], jax: ["input/TeX", "output/HTML-CSS"], tex2jax: { inlineMath: [ ['$','$'], ["\\(","\\)"] ], displayMath: [ ['$$','$$'], ["\\[","\\]"] ], processEscapes: true, ignoreClass: '.*', processClass: 'mathjax.*' }, TeX: { extensions: ["AMSmath.js", "AMSsymbols.js", "noErrors.js"], noErrors: { inlineDelimiters: ["$","$"], multiLine: false, style: { "font-size": "normal", "border": "" } } }, "HTML-CSS": { availableFonts: ["TeX"] } }); </script> <script src='//static.arxiv.org/MathJax-2.7.3/MathJax.js'></script> <script src="https://static.arxiv.org/static/base/1.0.0a5/js/notification.js"></script> <link rel="stylesheet" href="https://static.arxiv.org/static/search/0.5.6/css/bulma-tooltip.min.css" /> <link rel="stylesheet" href="https://static.arxiv.org/static/search/0.5.6/css/search.css" /> <script src="https://code.jquery.com/jquery-3.2.1.slim.min.js" integrity="sha256-k2WSCIexGzOj3Euiig+TlR8gA0EmPjuc79OEeY5L45g=" crossorigin="anonymous"></script> <script src="https://static.arxiv.org/static/search/0.5.6/js/fieldset.js"></script> <style> radio#cf-customfield_11400 { display: none; } </style> </head> <body> <header><a href="#main-container" class="is-sr-only">Skip to main content</a> <!-- contains Cornell logo and sponsor statement --> <div class="attribution level is-marginless" role="banner"> <div class="level-left"> <a class="level-item" href="https://cornell.edu/"><img src="https://static.arxiv.org/static/base/1.0.0a5/images/cornell-reduced-white-SMALL.svg" alt="Cornell University" width="200" aria-label="logo" /></a> </div> <div class="level-right is-marginless"><p class="sponsors level-item is-marginless"><span id="support-ack-url">We gratefully acknowledge support from<br /> the Simons Foundation, <a href="https://info.arxiv.org/about/ourmembers.html">member institutions</a>, and all contributors. <a href="https://info.arxiv.org/about/donate.html">Donate</a></span></p></div> </div> <!-- contains arXiv identity and search bar --> <div class="identity level is-marginless"> <div class="level-left"> <div class="level-item"> <a class="arxiv" href="https://arxiv.org/" aria-label="arxiv-logo"> <img src="https://static.arxiv.org/static/base/1.0.0a5/images/arxiv-logo-one-color-white.svg" aria-label="logo" alt="arxiv logo" width="85" style="width:85px;"/> </a> </div> </div> <div class="search-block level-right"> <form class="level-item mini-search" method="GET" action="https://arxiv.org/search"> <div class="field has-addons"> <div class="control"> <input class="input is-small" type="text" name="query" placeholder="Search..." aria-label="Search term or terms" /> <p class="help"><a href="https://info.arxiv.org/help">Help</a> | <a href="https://arxiv.org/search/advanced">Advanced Search</a></p> </div> <div class="control"> <div class="select is-small"> <select name="searchtype" aria-label="Field to search"> <option value="all" selected="selected">All fields</option> <option value="title">Title</option> <option value="author">Author</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="author_id">arXiv author ID</option> <option value="help">Help pages</option> <option value="full_text">Full text</option> </select> </div> </div> <input type="hidden" name="source" value="header"> <button class="button is-small is-cul-darker">Search</button> </div> </form> </div> </div> <!-- closes identity --> <div class="container"> <div class="user-tools is-size-7 has-text-right has-text-weight-bold" role="navigation" aria-label="User menu"> <a href="https://arxiv.org/login">Login</a> </div> </div> </header> <main class="container" id="main-container"> <div class="level is-marginless"> <div class="level-left"> <h1 class="title is-clearfix"> Showing 1&ndash;37 of 37 results for author: <span class="mathjax">Marini, P</span> </h1> </div> <div class="level-right is-hidden-mobile"> <!-- feedback for mobile is moved to footer --> <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>&nbsp;&nbsp;</span> </div> </div> <div class="content"> <form method="GET" action="/search/nucl-ex" aria-role="search"> Searching in archive <strong>nucl-ex</strong>. <a href="/search/?searchtype=author&amp;query=Marini%2C+P">Search in all archives.</a> <div class="field has-addons-tablet"> <div class="control is-expanded"> <label for="query" class="hidden-label">Search term or terms</label> <input class="input is-medium" id="query" name="query" placeholder="Search term..." type="text" value="Marini, P"> </div> <div class="select control is-medium"> <label class="is-hidden" for="searchtype">Field</label> <select class="is-medium" id="searchtype" 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> </div> <div class="control"> <button class="button is-link is-medium">Search</button> </div> </div> <div class="field"> <div class="control is-size-7"> <label class="radio"> <input checked id="abstracts-0" name="abstracts" type="radio" value="show"> Show abstracts </label> <label class="radio"> <input id="abstracts-1" name="abstracts" type="radio" value="hide"> Hide abstracts </label> </div> </div> <div class="is-clearfix" style="height: 2.5em"> <div class="is-pulled-right"> <a href="/search/advanced?terms-0-term=Marini%2C+P&amp;terms-0-field=author&amp;size=50&amp;order=-announced_date_first">Advanced Search</a> </div> </div> <input type="hidden" name="order" value="-announced_date_first"> <input type="hidden" name="size" value="50"> </form> <div class="level breathe-horizontal"> <div class="level-left"> <form method="GET" action="/search/"> <div style="display: none;"> <select id="searchtype" 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="Marini, P"> <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/2312.01763">arXiv:2312.01763</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2312.01763">pdf</a>, <a href="https://arxiv.org/format/2312.01763">other</a>]&nbsp;</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> </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.109.064605">10.1103/PhysRevC.109.064605 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Isospin diffusion from $^{40,48}$Ca$+^{40,48}$Ca experimental data at Fermi energies: Direct comparisons with transport model calculations </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Fable%2C+Q">Q. Fable</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baldesi%2C+L">L. Baldesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barlini%2C+S">S. Barlini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">Eric Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">Bernard Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">Remi Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camaiani%2C+A">A. Camaiani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casini%2C+G">G. Casini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ciampi%2C+C">Caterina Ciampi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Due%C3%B1as%2C+J+A">J. A. Due帽as</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Genard%2C+T">T. Genard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D+D">Diego D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henri%2C+M">Maxime Henri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hong%2C+B">Byungsik Hong</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kim%2C+S">S. Kim</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kordyasz%2C+A+J">A. J. Kordyasz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kozik%2C+T">T. Kozik</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=F%C3%A8vre%2C+A+L">Arnaud Le F猫vre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">Nicolas Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">Ivano Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">Olivier Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marchi%2C+T">T. Marchi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">Paola Marini</a> , et al. (8 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="2312.01763v2-abstract-short" style="display: inline;"> This article presents an investigation of isospin equilibration in cross-bombarding $^{40,48}$Ca$+^{40,48}$Ca reactions at 35 MeV/nucleon, by comparing experimental data with filtered transport model calculations. Isospin diffusion is studied using the evolution of the isospin transport ratio with centrality. The asymmetry parameter $未=(N-Z)/A$ of the quasiprojectile (QP) residue is used as isospi&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2312.01763v2-abstract-full').style.display = 'inline'; document.getElementById('2312.01763v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2312.01763v2-abstract-full" style="display: none;"> This article presents an investigation of isospin equilibration in cross-bombarding $^{40,48}$Ca$+^{40,48}$Ca reactions at 35 MeV/nucleon, by comparing experimental data with filtered transport model calculations. Isospin diffusion is studied using the evolution of the isospin transport ratio with centrality. The asymmetry parameter $未=(N-Z)/A$ of the quasiprojectile (QP) residue is used as isospin-sensitive observable, while a recent method for impact parameter reconstruction is used for centrality sorting. A benchmark of global observables is proposed to assess the relevance of the antisymmetrized molecular dynamics (AMD) model, coupled to GEMINI++, in the study of dissipative collisions. Our results demonstrate the importance of considering cluster formation to reproduce observables used for isospin transport and centrality studies. Within the AMD model, we prove the applicability of the impact parameter reconstruction method, enabling a direct comparison to the experimental data for the investigation of isospin diffusion. For both, we evidence a tendency to isospin equilibration with an impact parameter decreasing from 9 to 3 fm, while the full equilibration is not reached. A weak sensitivity to the stiffness of the equation of state employed in the model is also observed, with a better reproduction of the experimental trend for the neutron-rich reactions. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2312.01763v2-abstract-full').style.display = 'none'; document.getElementById('2312.01763v2-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 June, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 4 December, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2023. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Physical Review C, 109 (064605) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2311.07103">arXiv:2311.07103</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2311.07103">pdf</a>, <a href="https://arxiv.org/format/2311.07103">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 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.nimb.2023.05.053">10.1016/j.nimb.2023.05.053 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Particle Identification at VAMOS++ with Machine Learning Techniques </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Cho%2C+Y">Y. Cho</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kim%2C+Y+H">Y. H. Kim</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Choi%2C+S">S. Choi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Park%2C+J">J. Park</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bae%2C+S">S. Bae</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hahn%2C+K+I">K. I. Hahn</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Son%2C+Y">Y. Son</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Navin%2C+A">A. Navin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lemasson%2C+A">A. Lemasson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rejmund%2C+M">M. Rejmund</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ramos%2C+D">D. Ramos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ackermann%2C+D">D. Ackermann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Utepov%2C+A">A. Utepov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fourgeres%2C+C">C. Fourgeres</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Thomas%2C+J+C">J. C. Thomas</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Goupil%2C+J">J. Goupil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fremont%2C+G">G. Fremont</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=de+France%2C+G">G. de France</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Watanabe%2C+Y+X">Y. X. Watanabe</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hirayama%2C+Y">Y. Hirayama</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Jeong%2C+S">S. Jeong</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Niwase%2C+T">T. Niwase</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Miyatake%2C+H">H. Miyatake</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schury%2C+P">P. Schury</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosenbusch%2C+M">M. Rosenbusch</a> , et al. (23 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="2311.07103v2-abstract-short" style="display: inline;"> Multi-nucleon transfer reaction between 136Xe beam and 198Pt target was performed using the VAMOS++ spectrometer at GANIL to study the structure of n-rich nuclei around N=126. Unambiguous charge state identification was obtained by combining two supervised machine learning methods, deep neural network (DNN) and positional correction using a gradient-boosting decision tree (GBDT). The new method re&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2311.07103v2-abstract-full').style.display = 'inline'; document.getElementById('2311.07103v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2311.07103v2-abstract-full" style="display: none;"> Multi-nucleon transfer reaction between 136Xe beam and 198Pt target was performed using the VAMOS++ spectrometer at GANIL to study the structure of n-rich nuclei around N=126. Unambiguous charge state identification was obtained by combining two supervised machine learning methods, deep neural network (DNN) and positional correction using a gradient-boosting decision tree (GBDT). The new method reduced the complexity of the kinetic energy calibration and outperformed the conventional method, improving the charge state resolution by 8% <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2311.07103v2-abstract-full').style.display = 'none'; document.getElementById('2311.07103v2-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> 14 November, 2023; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 13 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">Journal ref:</span> Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, Volume 541, August 2023, Pages 240-242 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2202.13850">arXiv:2202.13850</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2202.13850">pdf</a>, <a href="https://arxiv.org/format/2202.13850">other</a>]&nbsp;</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="Atomic Physics">physics.atom-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/PhysRevC.106.024605">10.1103/PhysRevC.106.024605 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Experimental study of the $^{40,48}$Ca+ $^{40,48}$Ca reactions at 35 MeV/nucleon </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Fable%2C+Q">Q. Fable</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boisjoli%2C+M">M. Boisjoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=F%C3%A8vre%2C+A+L">A. Le F猫vre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Verde%2C+G">G. Verde</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ademard%2C+G">G. Ademard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bardelli%2C+L">L. Bardelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bhattacharya%2C+C">C. Bhattacharya</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bhattacharya%2C+S">S. Bhattacharya</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casini%2C+G">G. Casini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Commara%2C+M">M. Commara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dayras%2C+R">R. Dayras</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ducret%2C+J+E">J. E. Ducret</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Farget%2C+F">F. Farget</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=G%C3%A9nard%2C+T">T. G茅nard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gramegna%2C+F">F. Gramegna</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henri%2C+M">M. Henri</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="2202.13850v2-abstract-short" style="display: inline;"> In this article we investigate $^{40,48}$Ca+$^{40,48}$Ca peripheral and semi-peripheral reactions at 35 MeV/nucleon. Data were obtained using the unique coupling of the VAMOS high acceptance spectrometer and the INDRA charged particle multidetector.The spectrometer allowed high resolution measurement of charge, mass and velocity of the cold projectile-like fragment (PLF), while the INDRA detector&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2202.13850v2-abstract-full').style.display = 'inline'; document.getElementById('2202.13850v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2202.13850v2-abstract-full" style="display: none;"> In this article we investigate $^{40,48}$Ca+$^{40,48}$Ca peripheral and semi-peripheral reactions at 35 MeV/nucleon. Data were obtained using the unique coupling of the VAMOS high acceptance spectrometer and the INDRA charged particle multidetector.The spectrometer allowed high resolution measurement of charge, mass and velocity of the cold projectile-like fragment (PLF), while the INDRA detector recorded coincident charged particles with nearly $4蟺$ acceptance.The measured isotopic composition of the PLF identified in VAMOS and the average light charged particle (LCP) multiplicities are promising observables to study the isospin diffusion.The detection of the PLF in coincidence with LCP allows the reconstruction of the mass, charge and excitation energy of the associated initial quasi-projectile nuclei (QP), as well as the extraction of apparent temperatures.We investigate the suitability of the isoscaling method with the PLF and the experimental reconstructed QP.The extracted $伪$ and $螖$ isoscaling parameters present a dependence on the considered system combination that could justify their use as a surrogate for isospin asymmetry in isospin transport studies.The reconstruction of the QP allows to observe an evolution of the $伪/螖$ with the size of the QP, the latter being consistent with a strong surface contribution to the symmetry energy term in finite nuclei. This leads to the conclusion that the reconstruction of the primary source is mandatory for the study of the symmetry energy term based on the isoscaling method for such reactions. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2202.13850v2-abstract-full').style.display = 'none'; document.getElementById('2202.13850v2-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 August, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 28 February, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Physical Review C, American Physical Society, 2022, 106 (2), pp.024605 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2109.14330">arXiv:2109.14330</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2109.14330">pdf</a>, <a href="https://arxiv.org/ps/2109.14330">ps</a>, <a href="https://arxiv.org/format/2109.14330">other</a>]&nbsp;</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"> Energy Dependence of Prompt Fission Neutron Multiplicity in the $^{239}$Pu($n,f$) Reaction </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Taieb%2C+J">J. Taieb</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neudecker%2C+D">D. Neudecker</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=B%C3%A9lier%2C+G">G. B茅lier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatillon%2C+A">A. Chatillon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Etasse%2C+D">D. Etasse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Laurent%2C+B">B. Laurent</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Morfouace%2C+P">P. Morfouace</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Morillon%2C+B">B. Morillon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Devlin%2C+M">M. Devlin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gomez%2C+J+A">J. A. Gomez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Haight%2C+R+C">R. C. Haight</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kelly%2C+K+J">K. J. Kelly</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=O%27Donnell%2C+J+M">J. M. O&#39;Donnell</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="2109.14330v1-abstract-short" style="display: inline;"> Accurate multiplicities of prompt fission neutrons emitted in neutron-induced fission on a large energy range are essential for fundamental and applied nuclear physics. Measuring them to high precision for radioactive fissioning nuclides remains, however, an experimental challenge. In this work, the average prompt-neutron multiplicity emitted in the 239Pu(n,f) reaction was extracted as a function&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2109.14330v1-abstract-full').style.display = 'inline'; document.getElementById('2109.14330v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2109.14330v1-abstract-full" style="display: none;"> Accurate multiplicities of prompt fission neutrons emitted in neutron-induced fission on a large energy range are essential for fundamental and applied nuclear physics. Measuring them to high precision for radioactive fissioning nuclides remains, however, an experimental challenge. In this work, the average prompt-neutron multiplicity emitted in the 239Pu(n,f) reaction was extracted as a function of the incident-neutron energy, over the range 1-700~MeV, with a novel technique, which allowed to minimize and correct for the main sources of bias and thus achieve unprecedented precision. At low energies, our data validate for the first time the ENDF/B-VIII.0 nuclear data evaluation with an independent measurement and reduce the evaluated uncertainty by up to $60\%$. This work opens up the possibility of precisely measuring prompt fission neutron multiplicities on highly radioactive nuclei relevant for an essential component of energy production world-wide. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2109.14330v1-abstract-full').style.display = 'none'; document.getElementById('2109.14330v1-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> 29 September, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 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">6 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/2002.05439">arXiv:2002.05439</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2002.05439">pdf</a>]&nbsp;</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 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.125.122502">10.1103/PhysRevLett.125.122502 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Simultaneous determination of neutron-induced fission and radiative-capture cross sections from decay probabilities obtained with a surrogate reaction </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Sanchez%2C+R+P">R. Perez Sanchez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Jurado%2C+B">B. Jurado</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Meot%2C+V">V. Meot</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roig%2C+O">O. Roig</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dupuis%2C+M">M. Dupuis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bouland%2C+O">O. Bouland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Denis-Petit%2C+D">D. Denis-Petit</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mathieu%2C+L">L. Mathieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tsekhanovich%2C+I">I. Tsekhanovich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aiche%2C+M">M. Aiche</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Audouin%2C+L">L. Audouin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cannes%2C+C">C. Cannes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czajkowski%2C+S">S. Czajkowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Delpech%2C+S">S. Delpech</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorgen%2C+A">A. Gorgen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guttormsen%2C+M">M. Guttormsen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henriques%2C+A">A. Henriques</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kessedjian%2C+G">G. Kessedjian</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nishio%2C+K">K. Nishio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ramos%2C+D">D. Ramos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Siem%2C+S">S. Siem</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Zeiser%2C+F">F. Zeiser</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="2002.05439v2-abstract-short" style="display: inline;"> Reliable neutron-induced reaction cross sections of unstable nuclei are essential for nuclear astrophysics and applications but their direct measurement is often impossible. The surrogate-reaction method is one of the most promising alternatives to access these cross sections. In this work, we successfully applied the surrogate-reaction method to infer for the first time both the neutron-induced f&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2002.05439v2-abstract-full').style.display = 'inline'; document.getElementById('2002.05439v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2002.05439v2-abstract-full" style="display: none;"> Reliable neutron-induced reaction cross sections of unstable nuclei are essential for nuclear astrophysics and applications but their direct measurement is often impossible. The surrogate-reaction method is one of the most promising alternatives to access these cross sections. In this work, we successfully applied the surrogate-reaction method to infer for the first time both the neutron-induced fission and radiative-capture cross sections of 239Pu in a consistent manner from a single measurement. This was achieved by combining simultaneously-measured fission and gamma-emission probabilities for the 240Pu(4He,4He&#39;) surrogate reaction with a calculation of the angular-momentum and parity distributions populated in this reaction. While other experiments measure the probabilities for some selected gamma-ray transitions, we measure the gamma-emission probability. This enlarges the applicability of the surrogate-reaction method. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2002.05439v2-abstract-full').style.display = 'none'; document.getElementById('2002.05439v2-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 September, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 13 February, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 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">8 pages, 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. 125, 122502 (2020) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1902.07951">arXiv:1902.07951</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1902.07951">pdf</a>, <a href="https://arxiv.org/ps/1902.07951">ps</a>, <a href="https://arxiv.org/format/1902.07951">other</a>]&nbsp;</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 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.101.044614">10.1103/PhysRevC.101.044614 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Prompt Fission Neutrons in the $^{239}$Pu($n,f$) Reaction </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Taieb%2C+J">J. Taieb</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Laurent%2C+B">B. Laurent</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Belier%2C+G">G. Belier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatillon%2C+A">A. Chatillon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Etasse%2C+D">D. Etasse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Morfouace%2C+P">P. Morfouace</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Devlin%2C+M">M. Devlin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gomez%2C+J+A">J. A. Gomez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Haight%2C+R+C">R. C. Haight</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kelly%2C+K+J">K. J. Kelly</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=O%27Donnel%2C+J+M">J. M. O&#39;Donnel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schmitt%2C+K+T">K. T. Schmitt</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="1902.07951v2-abstract-short" style="display: inline;"> Prompt fission neutron spectra from $^{239}$Pu($n,f$) were measured for incident neutron energies from $0.7$ to $700\,$MeV at the Weapons Neutron Research facility (WNR) of the Los Alamos Neutron Science Center. A newly designed high-efficiency fission chamber was coupled to the highly segmented Chi-Nu array to detect neutrons emitted in fission events. The double time-of-flight technique was used&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1902.07951v2-abstract-full').style.display = 'inline'; document.getElementById('1902.07951v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1902.07951v2-abstract-full" style="display: none;"> Prompt fission neutron spectra from $^{239}$Pu($n,f$) were measured for incident neutron energies from $0.7$ to $700\,$MeV at the Weapons Neutron Research facility (WNR) of the Los Alamos Neutron Science Center. A newly designed high-efficiency fission chamber was coupled to the highly segmented Chi-Nu array to detect neutrons emitted in fission events. The double time-of-flight technique was used to deduce the incident-neutron energies from the spallation target and the outgoing-neutron energies from the fission chamber. Prompt fission neutron spectra (PFNS) were measured with respect to $^{252}$Cf spontaneous fission down to $200\,$keV and up to about $12\,$MeV for all the incident neutron energies with typical uncertainties well below $2\%$ up to about $10\,$MeV outgoing-neutron energy. The general trend of PFNS is well reproduced by JEFF3.3 and ENDF-B\VIII.0 evaluations. Discrepancies were however observed for the low-energy part of the spectra, where evaluations overestimate the number of emitted neutrons. Neutron multiplicities and average kinetic energies as a function of incident-neutron energy are obtained experimentally with reported uncertainties below $0.4\%$. Neutron multiplicities disagree with some older datasets above $6\,$ MeV, indicating the need of using a high-efficiency fission detector, which does not bias the data. The measured mean kinetic energies agree with the most recent data. Evaluations fairly reproduce the trend, but fail to reproduce the experimental values within their uncertainties. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1902.07951v2-abstract-full').style.display = 'none'; document.getElementById('1902.07951v2-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 October, 2019; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 21 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">Version 2, 15 pages, 21 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/1901.06185">arXiv:1901.06185</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1901.06185">pdf</a>, <a href="https://arxiv.org/ps/1901.06185">ps</a>, <a href="https://arxiv.org/format/1901.06185">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"> A new gas-based proton-recoil telescope for quasi-absolute neutron flux measurements between 0.2 and 2 MeV neutron energy </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mathieu%2C+L">L. Mathieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=A%C3%AFche%2C+M">M. A茂che</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pedroza%2C+J+-">J. -L. Pedroza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiron%2C+T">T. Chiron</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baron%2C+P">P. Baron</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czajkowski%2C+S">S. Czajkowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Druillole%2C+F">F. Druillole</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellmuth%2C+P">P. Hellmuth</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Jurado%2C+B">B. Jurado</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rebii%2C+A">A. Rebii</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tsekhanovich%2C+I">I. Tsekhanovich</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="1901.06185v1-abstract-short" style="display: inline;"> Absolute measurements of neutron flux are an essential prerequisite of neutron-induced cross section measurements, neutron beam lines characterization and dosimetric investigations. A new gaseous detector has been developed for measurements of 0.2 to 2 MeV neutron flux based on proton-recoil process. The detector, consisting of two segmented ionization chambers read by Micromegas technology, has b&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1901.06185v1-abstract-full').style.display = 'inline'; document.getElementById('1901.06185v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1901.06185v1-abstract-full" style="display: none;"> Absolute measurements of neutron flux are an essential prerequisite of neutron-induced cross section measurements, neutron beam lines characterization and dosimetric investigations. A new gaseous detector has been developed for measurements of 0.2 to 2 MeV neutron flux based on proton-recoil process. The detector, consisting of two segmented ionization chambers read by Micromegas technology, has beed conceived to provide quasi-absolute neutron flux measurements with an accuracy of \simeq3%. The gas pressure flexibility makes the telescope non sensitive to 纬 and electrons background, and therefore advantageous over semi-conductor materials as a neutron flux instrument. The adjustable gas pressure and H-sample thickness, the use of Micromegas technology and the tracking capabilities allows the detection of neutrons on a large dynamical range and down to 200 keV with a good rejection of scattered neutron events and random background <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1901.06185v1-abstract-full').style.display = 'none'; document.getElementById('1901.06185v1-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 January, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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">11 figures, 26 pages</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1901.04874">arXiv:1901.04874</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1901.04874">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="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/10.1016/j.nima.2019.04.084">10.1016/j.nima.2019.04.084 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Experimental set-up for the simultaneous measurement of fission and gamma-emission probabilities induced by transfer or inelastic-scattering reactions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=S%C3%A1nchez%2C+R+P">R. P茅rez S谩nchez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Jurado%2C+B">B. Jurado</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aiche%2C+M">M. Aiche</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czajkowski%2C+S">S. Czajkowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Denis-Petit%2C+D">D. Denis-Petit</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ducasse%2C+Q">Q. Ducasse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mathieu%2C+L">L. Mathieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tsekhanovich%2C+I">I. Tsekhanovich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henriques%2C+A">A. Henriques</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=M%C3%A9ot%2C+V">V. M茅ot</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roig%2C+O">O. Roig</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="1901.04874v2-abstract-short" style="display: inline;"> Fission and gamma-emission probabilities induced by transfer or inelastic scattering reactions with light projectile nuclei are very valuable quantities for constraining the models that describe the de-excitation of heavy nuclei. We have developed an experimental set-up that allows us to simultaneously measure fission and gamma-emission probabilities. The measurement of the gamma-emission probabil&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1901.04874v2-abstract-full').style.display = 'inline'; document.getElementById('1901.04874v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1901.04874v2-abstract-full" style="display: none;"> Fission and gamma-emission probabilities induced by transfer or inelastic scattering reactions with light projectile nuclei are very valuable quantities for constraining the models that describe the de-excitation of heavy nuclei. We have developed an experimental set-up that allows us to simultaneously measure fission and gamma-emission probabilities. The measurement of the gamma-emission probability at excitation energies where the fission channel is open is challenging due to the intense background of gamma rays emitted by the fission fragments. We discuss the procedure to subtract such a background and the constraints that this subtraction and other experimental conditions put on the set up. We show that our set-up complies with these constraints. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1901.04874v2-abstract-full').style.display = 'none'; document.getElementById('1901.04874v2-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> 9 April, 2019; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 11 January, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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">18 pages, 10 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/1811.01005">arXiv:1811.01005</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1811.01005">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="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Development of a gaseous proton-recoil detector for neutron flux measurements between 0.2 and 2 MeV neutron energy </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">Paola Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mathieu%2C+L">Ludovic Mathieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=A%C3%AFche%2C+M">Mourad A茂che</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czajkowski%2C+S">Serge Czajkowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Jurado%2C+B">Beatriz Jurado</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tsekhanovich%2C+I">Igor Tsekhanovich</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="1811.01005v1-abstract-short" style="display: inline;"> Absolute measurements of neutron fluence are an essential prerequisite of neutron-induced cross section measurements, neutron beam lines characterization and dosimetric investigations. The H(n,p) elastic scattering cross section is a very well known standard used to perform precise neutron flux measurements in high precision measurements. The use of this technique, with proton recoil detectors, is&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1811.01005v1-abstract-full').style.display = 'inline'; document.getElementById('1811.01005v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1811.01005v1-abstract-full" style="display: none;"> Absolute measurements of neutron fluence are an essential prerequisite of neutron-induced cross section measurements, neutron beam lines characterization and dosimetric investigations. The H(n,p) elastic scattering cross section is a very well known standard used to perform precise neutron flux measurements in high precision measurements. The use of this technique, with proton recoil detectors, is not straightforward below incident neutron energy of 1 MeV, due to a high background in the detected proton spectrum. Experiments have been carried out at the AIFIRA facility to investigate such background and to determine its origin and components. Based on these investigations, a gaseous proton-recoil detector has been designed with a reduced low energy background. A first test of this detector has been carried out at the AIFIRA facility, and first results will be presented. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1811.01005v1-abstract-full').style.display = 'none'; document.getElementById('1811.01005v1-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, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 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">Submitted</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1804.07552">arXiv:1804.07552</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1804.07552">pdf</a>, <a href="https://arxiv.org/ps/1804.07552">ps</a>, <a href="https://arxiv.org/format/1804.07552">other</a>]&nbsp;</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 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.98.044612">10.1103/PhysRevC.98.044612 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Study and validation of a new &#34;3D Calorimetry&#34; of hot nuclei with the HIPSE event generator </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Vient%2C+E">E. Vient</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manduci%2C+L">L. Manduci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Legou%C3%A9e%2C+E">E. Legou茅e</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augey%2C+L">L. Augey</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dell%27Aquila%2C+D">D. Dell&#39;Aquila</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fable%2C+Q">Q. Fable</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Francalanza%2C+L">L. Francalanza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henri%2C+M">M. Henri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Commara%2C+M">M. La Commara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lehaut%2C+G">G. Lehaut</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Parlog%2C+M">M. Parlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a> , et al. (5 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="1804.07552v1-abstract-short" style="display: inline;"> In nuclear thermodynamics, the determination of the excitation energy of hot nuclei is a fundamental experimental problem. Instrumental physicists have been trying to solve this problem for several years by building the most exhaustive 4Pi detector arrays and perfecting their calorimetry techniques. In a recent paper, a proposal for a new calorimetry, called &#34;3D calorimetry&#34;, was made. It tries to&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1804.07552v1-abstract-full').style.display = 'inline'; document.getElementById('1804.07552v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1804.07552v1-abstract-full" style="display: none;"> In nuclear thermodynamics, the determination of the excitation energy of hot nuclei is a fundamental experimental problem. Instrumental physicists have been trying to solve this problem for several years by building the most exhaustive 4Pi detector arrays and perfecting their calorimetry techniques. In a recent paper, a proposal for a new calorimetry, called &#34;3D calorimetry&#34;, was made. It tries to optimize the separation between the particles and fragments emitted by the Quasi-Projectile and the other possible contributions. This can be achieved by determining the experimental probability for a given nucleus of a nuclear reaction to be emitted by the Quasi-Projectile. It has been developed for the INDRA data. In the present work, we wanted to dissect and validate this new method of characterization of a hot Quasi-Projectile. So we tried to understand and control it completely to determine these limits. Using the HIPSE event generator and a software simulating the functioning of INDRA, we were able to achieve this goal and provide a quantitative estimation of the quality of the QP characterization. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1804.07552v1-abstract-full').style.display = 'none'; document.getElementById('1804.07552v1-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> 20 April, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2018. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C 98, 044612 (2018) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1709.07396">arXiv:1709.07396</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1709.07396">pdf</a>, <a href="https://arxiv.org/format/1709.07396">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Data Analysis, Statistics and Probability">physics.data-an</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/PhysRevC.98.044611">10.1103/PhysRevC.98.044611 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A new &#34;3D Calorimetry&#34; of hot nuclei </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Vient%2C+E">E. Vient</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manduci%2C+L">L. Manduci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Legou%C3%A9e%2C+E">E. Legou茅e</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augey%2C+L">L. Augey</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dell%27Aquila%2C+D">D. Dell&#39;Aquila</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fable%2C+Q">Q. Fable</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Francalanza%2C+L">L. Francalanza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henri%2C+M">M. Henri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Commara%2C+M">M. La Commara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lehaut%2C+G">G. Lehaut</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Parlog%2C+M">M. Parlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a> , et al. (5 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="1709.07396v1-abstract-short" style="display: inline;"> In the domain of Fermi energy, it is extremely complex to isolate experimentally fragments and particles issued from the cooling of a hot nucleus produced during a heavy ion collision. This paper presents a new method to characterize more precisely hot Quasi-Projectiles. It tries to take into account as accurately as possible the distortions generated by all the other potential participants in the&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1709.07396v1-abstract-full').style.display = 'inline'; document.getElementById('1709.07396v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1709.07396v1-abstract-full" style="display: none;"> In the domain of Fermi energy, it is extremely complex to isolate experimentally fragments and particles issued from the cooling of a hot nucleus produced during a heavy ion collision. This paper presents a new method to characterize more precisely hot Quasi-Projectiles. It tries to take into account as accurately as possible the distortions generated by all the other potential participants in the nuclear reaction. It is quantitatively shown that this method is a major improvement respect to classic calorimetries used with a 4$蟺$ detector array. By detailing and deconvolving the different steps of the reconstitution of the hot nucleus, this study shows also the respective role played by the experimental device and the event selection criteria on the quality of the determination of QP characteristics. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1709.07396v1-abstract-full').style.display = 'none'; document.getElementById('1709.07396v1-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 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">11 pages, 13 figures, will be submitted to PRC</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C 98, 044611 (2018) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1707.08863">arXiv:1707.08863</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1707.08863">pdf</a>, <a href="https://arxiv.org/ps/1707.08863">ps</a>, <a href="https://arxiv.org/format/1707.08863">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 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.nima.2017.12.041">10.1016/j.nima.2017.12.041 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Improving isotopic identification with \emph{INDRA} Silicon-CsI(\emph{Tl}) telescopes </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Parlog%2C+M">M. Parlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lehaut%2C+G">G. Lehaut</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tabacaru%2C+G">G. Tabacaru</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tassan-got%2C+L">L. Tassan-got</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pawlowski%2C+P">P. Pawlowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dell%27Aquila%2C+D">D. Dell&#39;Aquila</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Commara%2C+M">M. La Commara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manduci%2C+L">L. Manduci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Steckmeyer%2C+J+C">J. C. Steckmeyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Verde%2C+G">G. Verde</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vient%2C+E">E. Vient</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wieleczko%2C+J+P">J. P. Wieleczko</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="1707.08863v1-abstract-short" style="display: inline;"> Profiting from previous works done with the \emph{INDRA} multidetector on the description of the light response $\mathcal L$ of the CsI(\emph{Tl}) crystals to different impinging nuclei, we propose an improved $螖E - \mathcal L$ identification-calibration procedure for Silicon-Cesium Iodide (Si-CsI) telescopes, namely an Advanced Mass Estimate (\emph{AME}) method. \emph{AME} is compared to the usua&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1707.08863v1-abstract-full').style.display = 'inline'; document.getElementById('1707.08863v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1707.08863v1-abstract-full" style="display: none;"> Profiting from previous works done with the \emph{INDRA} multidetector on the description of the light response $\mathcal L$ of the CsI(\emph{Tl}) crystals to different impinging nuclei, we propose an improved $螖E - \mathcal L$ identification-calibration procedure for Silicon-Cesium Iodide (Si-CsI) telescopes, namely an Advanced Mass Estimate (\emph{AME}) method. \emph{AME} is compared to the usual, %$&#34;螖E - E&#34;$ simple visual analysis of the corresponding two-dimensional map of $螖E - E$ type, by using \emph{INDRA} experimental data from nuclear reactions induced by heavy ions in the Fermi energy regime. We show that the capability of such telescopes to identify both the atomic $Z$ and the mass $A$ numbers of light and heavy reaction products, can be quantitatively improved thanks to the proposed approach. This conclusion opens new possibilities to use \emph{INDRA} for studying these reactions especially with radioactive beams. Indeed, the determination of the mass for charged reaction products becomes of paramount importance to shed light on the role of the isospin degree of freedom in the nuclear equation of state. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1707.08863v1-abstract-full').style.display = 'none'; document.getElementById('1707.08863v1-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, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">19 pages, 10 figures, submitted to NIM A</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1707.01264">arXiv:1707.01264</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1707.01264">pdf</a>, <a href="https://arxiv.org/ps/1707.01264">ps</a>, <a href="https://arxiv.org/format/1707.01264">other</a>]&nbsp;</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 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/i2018-12531-5">10.1140/epja/i2018-12531-5 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Understand the thermometry of hot nuclei from the energy spectra of light charged particles </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Vient%2C+E">E. Vient</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augey%2C+L">L. Augey</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dell%27Aquila%2C+D">D. Dell&#39;Aquila</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fable%2C+Q">Q. Fable</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Francalanza%2C+L">L. Francalanza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henri%2C+M">M. Henri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Commara%2C+M">M. La Commara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Legou%C3%A9e%2C+E">E. Legou茅e</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lehaut%2C+G">G. Lehaut</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manduci%2C+L">L. Manduci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Parlog%2C+M">M. Parlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roy%2C+R">R. Roy</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=St-Onge%2C+P">P. St-Onge</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="1707.01264v1-abstract-short" style="display: inline;"> In the domain of Fermi energy, the hot nucleus temperature can be determined by using the energy spectra of evaporated light charged particles. But this method of measurement is not without difficulties both theoretical and experimental. The presented study aims to disentangle the respective influences of different factors on the quality of this measurement : the physics, the detection (a 4? detec&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1707.01264v1-abstract-full').style.display = 'inline'; document.getElementById('1707.01264v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1707.01264v1-abstract-full" style="display: none;"> In the domain of Fermi energy, the hot nucleus temperature can be determined by using the energy spectra of evaporated light charged particles. But this method of measurement is not without difficulties both theoretical and experimental. The presented study aims to disentangle the respective influences of different factors on the quality of this measurement : the physics, the detection (a 4? detector array as INDRA) and the experimental procedure. This analysis demonstrates the possibility of determining from an energy spectrum, with an accuracy of about 10 %, the true apparent temperature felt by a given type of particle emitted by a hot nucleus. Three conditions are however necessary : have a perfect detector of particles, an important statistics and very few secondary emissions. According to the GEMINI event generator, for hot nuclei of intermediate mass, only deuterons and tritons could fill these conditions. This temperature can allow to trace back to the initial temperature by using an appropriate method. This determination may be better than 15 %. With a real experimental device, an insufficient angular resolution and topological distortions caused by the detection can damage spectra to the point to make very difficult a correct determination of the apparent temperature. The experimental reconstruction of the frame of the hot nucleus may also be responsible for this deterioration <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1707.01264v1-abstract-full').style.display = 'none'; document.getElementById('1707.01264v1-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 July, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">17 pages, 16 figures submitted to PRC</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1703.03694">arXiv:1703.03694</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1703.03694">pdf</a>, <a href="https://arxiv.org/ps/1703.03694">ps</a>, <a href="https://arxiv.org/format/1703.03694">other</a>]&nbsp;</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 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.97.024612">10.1103/PhysRevC.97.024612 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Light charged clusters emitted in 32 MeV/nucleon 136,124Xe+124,112Sn reactions: chemical equilibrium, 3He and 6He production </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dell%27Aquila%2C+D">D. Dell&#39;Aquila</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fable%2C+Q">Q. Fable</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Francalanza%2C+L">L. Francalanza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henri%2C+M">M. Henri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Commara%2C+M">M. La Commara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manduci%2C+L">L. Manduci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Parlog%2C+M">M. Parlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roy%2C+R">R. Roy</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Saint-Onge%2C+P">P. Saint-Onge</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Verde%2C+G">G. Verde</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vient%2C+E">E. Vient</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vigilante%2C+M">M. Vigilante</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="1703.03694v1-abstract-short" style="display: inline;"> Nuclear particle production from peripheral to central events is presented. N/Z gradient between projectile and target is studied using the fact that two reactions have the same projectile+target N/Z and so the same neutron to proton ratio for the combined system. Inclusive data study in the forward part of the center of mass indicates that N/Z equilibration between the projectile-like and the tar&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1703.03694v1-abstract-full').style.display = 'inline'; document.getElementById('1703.03694v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1703.03694v1-abstract-full" style="display: none;"> Nuclear particle production from peripheral to central events is presented. N/Z gradient between projectile and target is studied using the fact that two reactions have the same projectile+target N/Z and so the same neutron to proton ratio for the combined system. Inclusive data study in the forward part of the center of mass indicates that N/Z equilibration between the projectile-like and the target-like is achieved for central collisions. Particles are also produced from mid-rapidity region. 3He mean pre-equilibrium character is evidenced and 6He production at mid-rapidity implies a neutron enrichment phenomenon of the projectile target interacting zone. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1703.03694v1-abstract-full').style.display = 'none'; document.getElementById('1703.03694v1-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 March, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 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">9 pages, 10 figures</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, 024612 (2018) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1608.04332">arXiv:1608.04332</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1608.04332">pdf</a>, <a href="https://arxiv.org/ps/1608.04332">ps</a>, <a href="https://arxiv.org/format/1608.04332">other</a>]&nbsp;</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 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.94.034608">10.1103/PhysRevC.94.034608 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gannon%2C+S">S. Gannon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kupny%2C+S">S. Kupny</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lasko%2C+P">P. Lasko</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Acosta%2C+L">L. Acosta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adamczyk%2C+M">M. Adamczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Ajlan%2C+A">A. Al-Ajlan</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Garawi%2C+M">M. Al-Garawi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Homaidhi%2C+S">S. Al-Homaidhi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ayyad%2C+Y">Y. Ayyad</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Basrak%2C+Z">Z. Basrak</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benlliure%2C+J">J. Benlliure</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boisjoli%2C+M">M. Boisjoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boretzky%2C+K">K. Boretzky</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brzychczyk%2C+J">J. Brzychczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Budzanowski%2C+A">A. Budzanowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caesar%2C+C">C. Caesar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cammarata%2C+P">P. Cammarata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chajecki%2C+Z">Z. Chajecki</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chartier%2C+M">M. Chartier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a> , et al. (67 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="1608.04332v2-abstract-short" style="display: inline;"> Directed and elliptic flows of neutrons and light charged particles were measured for the reaction 197Au+197Au at 400 MeV/nucleon incident energy within the ASY-EOS experimental campaign at the GSI laboratory. The detection system consisted of the Large Area Neutron Detector LAND, combined with parts of the CHIMERA multidetector, of the ALADIN Time-of-flight Wall, and of the Washington-University&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1608.04332v2-abstract-full').style.display = 'inline'; document.getElementById('1608.04332v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1608.04332v2-abstract-full" style="display: none;"> Directed and elliptic flows of neutrons and light charged particles were measured for the reaction 197Au+197Au at 400 MeV/nucleon incident energy within the ASY-EOS experimental campaign at the GSI laboratory. The detection system consisted of the Large Area Neutron Detector LAND, combined with parts of the CHIMERA multidetector, of the ALADIN Time-of-flight Wall, and of the Washington-University Microball detector. The latter three arrays were used for the event characterization and reaction-plane reconstruction. In addition, an array of triple telescopes, KRATTA, was used for complementary measurements of the isotopic composition and flows of light charged particles. From the comparison of the elliptic flow ratio of neutrons with respect to charged particles with UrQMD predictions, a value 纬= 0.72 \pm 0.19 is obtained for the power-law coefficient describing the density dependence of the potential part in the parametrization of the symmetry energy. It represents a new and more stringent constraint for the regime of supra-saturation density and confirms, with a considerably smaller uncertainty, the moderately soft to linear density dependence deduced from the earlier FOPI-LAND data. The densities probed are shown to reach beyond twice saturation. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1608.04332v2-abstract-full').style.display = 'none'; document.getElementById('1608.04332v2-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 September, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 15 August, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">25 pages, 22 figures, accepted for publication in Physical Review C</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C 94, 034608 (2016) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1512.07777">arXiv:1512.07777</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1512.07777">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="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/10.1016/j.nima.2016.04.083">10.1016/j.nima.2016.04.083 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Application of the EXtrapolated Efficiency Method (EXEM) to infer the gamma-cascade detection efficiency in the actinide region </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Ducasse%2C+Q">Q. Ducasse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Jurado%2C+B">B. Jurado</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mathieu%2C+L">L. Mathieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Morillon%2C+B">B. Morillon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aiche%2C+M">M. Aiche</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tsekhanovich%2C+I">I. Tsekhanovich</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="1512.07777v2-abstract-short" style="display: inline;"> The study of transfer-induced gamma-decay probabilities is very useful for understanding the surrogate-reaction method and, more generally, for constraining statistical-model calculations. One of the main difficulties in the measurement of gamma-decay probabilities is the determination of the gamma-cascade detection efficiency. In [Nucl. Instrum. Meth. A 700, 59 (2013)] we developed the Extrapolat&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1512.07777v2-abstract-full').style.display = 'inline'; document.getElementById('1512.07777v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1512.07777v2-abstract-full" style="display: none;"> The study of transfer-induced gamma-decay probabilities is very useful for understanding the surrogate-reaction method and, more generally, for constraining statistical-model calculations. One of the main difficulties in the measurement of gamma-decay probabilities is the determination of the gamma-cascade detection efficiency. In [Nucl. Instrum. Meth. A 700, 59 (2013)] we developed the Extrapolated Efficiency Method (EXEM), a new method to measure this quantity. In this work, we have applied, for the first time, the EXEM to infer the gamma-cascade detection efficiency in the actinide region. In particular, we have considered the 238U(d,p)239U and 238U(3He,d)239Np reactions. We have performed Hauser-Feshbach calculations to interpret our results and to verify the hypothesis on which the EXEM is based. The determination of fission and gamma-decay probabilities of 239Np below the neutron separation energy allowed us to validate the EXEM. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1512.07777v2-abstract-full').style.display = 'none'; document.getElementById('1512.07777v2-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> 19 January, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 24 December, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2015. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nuclear Inst. and Methods in Physics Research, A (2016), pp. 60-64 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1512.06334">arXiv:1512.06334</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1512.06334">pdf</a>]&nbsp;</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 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.94.024614">10.1103/PhysRevC.94.024614 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Study of the 238U(d,p) surrogate reaction via the simultaneous measurement of gamma-decay and fission probabilities </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Ducasse%2C+Q">Q. Ducasse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Jurado%2C+B">B. Jurado</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=A%C3%AFche%2C+M">M. A茂che</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mathieu%2C+L">L. Mathieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=G%C3%B6rgen%2C+A">A. G枚rgen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guttormsen%2C+M">M. Guttormsen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Larsen%2C+A+C">A. C. Larsen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tornyi%2C+T">T. Tornyi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wilson%2C+J+N">J. N. Wilson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barreau%2C+G">G. Barreau</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boutoux%2C+G">G. Boutoux</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czajkowski%2C+S">S. Czajkowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giacoppo%2C+F">F. Giacoppo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gunsing%2C+F">F. Gunsing</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hagen%2C+T+W">T. W. Hagen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lebois%2C+M">M. Lebois</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lei%2C+J">J. Lei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=M%C3%A9ot%2C+V">V. M茅ot</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Morillon%2C+B">B. Morillon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Moro%2C+A">A. Moro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Renstr%C3%B8m%2C+T">T. Renstr酶m</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roig%2C+O">O. Roig</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rose%2C+S+J">S. J. Rose</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=S%C3%A9rot%2C+O">O. S茅rot</a> , et al. (4 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1512.06334v3-abstract-short" style="display: inline;"> We investigated the 238U(d,p) reaction as a surrogate for the n + 238U reaction. For this purpose we measured for the first time the gamma-decay and fission probabilities of 239U* simultaneously and compared them to the corresponding neutron-induced data. We present the details of the procedure to infer the decay probabilities, as well as a thorough uncertainty analysis, including parameter correl&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1512.06334v3-abstract-full').style.display = 'inline'; document.getElementById('1512.06334v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1512.06334v3-abstract-full" style="display: none;"> We investigated the 238U(d,p) reaction as a surrogate for the n + 238U reaction. For this purpose we measured for the first time the gamma-decay and fission probabilities of 239U* simultaneously and compared them to the corresponding neutron-induced data. We present the details of the procedure to infer the decay probabilities, as well as a thorough uncertainty analysis, including parameter correlations. Calculations based on the continuum-discretized coupled-channels and distorted-wave Born approximations were used to correct our data from detected protons originating from elastic and inelastic deuteron breakup. In the region where the fission and gamma-decay probabilities compete, the corrected fission probability is in agreement with neutron-induced data, whereas the gamma-decay probability is much higher than the neutron-induced data. The performed statistical-model calculations are not able to explain these results. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1512.06334v3-abstract-full').style.display = 'none'; document.getElementById('1512.06334v3-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> 23 July, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 20 December, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 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">Includes modifications due to referee remarks</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C. 94, 024614 (2016) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1501.00595">arXiv:1501.00595</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1501.00595">pdf</a>, <a href="https://arxiv.org/ps/1501.00595">ps</a>, <a href="https://arxiv.org/format/1501.00595">other</a>]&nbsp;</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 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.physletb.2016.02.063">10.1016/j.physletb.2016.02.063 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Signals of Bose Einstein condensation and Fermi quenching in the decay of hot nuclear systems </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Zheng%2C+H">H. Zheng</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boisjoli%2C+M">M. Boisjoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Verde%2C+G">G. Verde</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ademard%2C+G">G. Ademard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auger%2C+L">L. Auger</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bhattacharya%2C+C">C. Bhattacharya</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J">J. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kundu%2C+S">S. Kundu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Commara%2C+M">M. La Commara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mukherjee%2C+G">G. Mukherjee</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Napolitani%2C+P">P. Napolitani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Parlog%2C+M">M. Parlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roy%2C+R">R. Roy</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Spadaccini%2C+G">G. Spadaccini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vigilante%2C+M">M. Vigilante</a> , et al. (2 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="1501.00595v1-abstract-short" style="display: inline;"> We report experimental signals of Bose-Einstein condensation in the decay of hot Ca projectile-like sources produced in mid-peripheral collisions at sub-Fermi energies. The experimental setup, constituted by the coupling of the INDRA 4$蟺$ detector array to the forward angle VAMOS magnetic spectrometer, allowed us to reconstruct the mass, charge and excitation energy of the decaying hot projectile-&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.00595v1-abstract-full').style.display = 'inline'; document.getElementById('1501.00595v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1501.00595v1-abstract-full" style="display: none;"> We report experimental signals of Bose-Einstein condensation in the decay of hot Ca projectile-like sources produced in mid-peripheral collisions at sub-Fermi energies. The experimental setup, constituted by the coupling of the INDRA 4$蟺$ detector array to the forward angle VAMOS magnetic spectrometer, allowed us to reconstruct the mass, charge and excitation energy of the decaying hot projectile-like sources. Furthermore, by means of quantum fluctuation analysis techniques, temperatures and mean volumes per particle &#34;as seen by&#34; bosons and fermions separately are correlated to the excitation energy of the reconstructed system. The obtained results are consistent with the production of dilute mixed (bosons/fermions) systems, where bosons experience a smaller volume as compared to the surrounding fermionic gas. Our findings recall similar phenomena observed in the study of boson condensates in atomic traps. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.00595v1-abstract-full').style.display = 'none'; document.getElementById('1501.00595v1-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 January, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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">Submitted to Phys. Rev. Lett. (december 2014)</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1409.0735">arXiv:1409.0735</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1409.0735">pdf</a>, <a href="https://arxiv.org/ps/1409.0735">ps</a>, <a href="https://arxiv.org/format/1409.0735">other</a>]&nbsp;</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> </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.90.064602">10.1103/PhysRevC.90.064602 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> In-medium effects for nuclear matter in the Fermi energy domain </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Durand%2C+D">D. Durand</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lehaut%2C+G">G. Lehaut</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Napolitani%2C+P">P. Napolitani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=P%C3%A2rlog%2C+M">M. P芒rlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Spadaccini%2C+G">G. Spadaccini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vient%2C+E">E. Vient</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vigilante%2C+M">M. Vigilante</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="1409.0735v1-abstract-short" style="display: inline;"> We study nuclear stopping in central collisions for heavy-ion induced reactions in the Fermi energy domain, between $15$ and $100$ A\,\textrm{MeV}. Using the large dataset of exclusive measurements provided by the $4蟺$ array \emph{INDRA}, we determine the relative degree of stopping as a function of system mass and bombarding energy. We show that the stopping can be directly related to the transpo&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1409.0735v1-abstract-full').style.display = 'inline'; document.getElementById('1409.0735v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1409.0735v1-abstract-full" style="display: none;"> We study nuclear stopping in central collisions for heavy-ion induced reactions in the Fermi energy domain, between $15$ and $100$ A\,\textrm{MeV}. Using the large dataset of exclusive measurements provided by the $4蟺$ array \emph{INDRA}, we determine the relative degree of stopping as a function of system mass and bombarding energy. We show that the stopping can be directly related to the transport properties in the nuclear medium. By looking specifically at free nucleons (here protons), we present for the first time a comprehensive body of experimental results concerning the mean free path, the nucleon-nucleon cross-section and in-medium effects in nuclear matter. It is shown that the mean free path exhibits a maximum at $位_{NN}=9.5 \pm 2$ \textrm{fm}, around $E_{inc}=35-40$ A\,\textrm{MeV} incident energy and decreases toward an asymptotic value $位_{NN}= 4.5 \pm 1$ \textrm{fm} at $E_{inc} = 100$ A\,\textrm{MeV}. After accounting for Pauli blocking of elastic nucleon-nucleon collisions, it is shown that the effective in-medium \emph{NN} cross section is further reduced compared to the free value in this energy range. Therefore, in-medium effects cannot be neglected in the Fermi energy range. These results bring new fundamental inputs for microscopic descriptions of nuclear reactions in the Fermi energy domain. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1409.0735v1-abstract-full').style.display = 'none'; document.getElementById('1409.0735v1-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 September, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2014. </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, 10 figures, submitted to PRC</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1310.5000">arXiv:1310.5000</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1310.5000">pdf</a>, <a href="https://arxiv.org/format/1310.5000">other</a>]&nbsp;</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> </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/i2014-14033-x">10.1140/epja/i2014-14033-x <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Isospin effects and symmetry energy studies with INDRA </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Ademard%2C+G">G. Ademard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Napolitani%2C+P">P. Napolitani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boisjoli%2C+M">M. Boisjoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kabtoul%2C+M">M. Kabtoul</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lehaut%2C+G">G. Lehaut</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P. Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Commara%2C+M">M. La Commara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=P%C3%A2rlog%2C+M">M. P芒rlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Paw%C5%82owski%2C+P">P. Paw艂owski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roy%2C+R">R. Roy</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Spadaccini%2C+E">E. Spadaccini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vient%2C+E">E. Vient</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vigilante%2C+M">M. Vigilante</a> , et al. (1 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="1310.5000v1-abstract-short" style="display: inline;"> The equation of state of asymmetric nuclear matter is still controversial, as predictions at subsaturation as well as above normal density widely diverge. We discuss several experimental results measured in heavy-ion collisions with the INDRA array in the incident energy range 5-80 MeV/nucleon. In particular an estimate of the density dependence of the symmetry energy is derived from isospin diffu&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1310.5000v1-abstract-full').style.display = 'inline'; document.getElementById('1310.5000v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1310.5000v1-abstract-full" style="display: none;"> The equation of state of asymmetric nuclear matter is still controversial, as predictions at subsaturation as well as above normal density widely diverge. We discuss several experimental results measured in heavy-ion collisions with the INDRA array in the incident energy range 5-80 MeV/nucleon. In particular an estimate of the density dependence of the symmetry energy is derived from isospin diffusion results compared with a transport code: the potential part of the symmetry energy linearly increases with the density. We demonstrate that isospin equilibrium is reached in mid-central collisions for the two reactions Ni+Au at 52 MeV/nucleon and Xe+Sn at 32 MeV/nucleon. New possible variables and an improved modelization to investigate symmetry energy are discussed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1310.5000v1-abstract-full').style.display = 'none'; document.getElementById('1310.5000v1-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 October, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 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">Review for the special issue of EPJA on symmetry energy. 20 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/1309.7779">arXiv:1309.7779</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1309.7779">pdf</a>, <a href="https://arxiv.org/format/1309.7779">other</a>]&nbsp;</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 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.92.064606">10.1103/PhysRevC.92.064606 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Coulomb chronometry to probe the decay mechanism of hot nuclei </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">Diego Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">Eric Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ademard%2C+G">G Ademard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boisjoli%2C+M">M Boisjoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gauthier%2C+J">J Gauthier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Legou%C3%A9e%2C+E">E Legou茅e</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manduci%2C+L">L Manduci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mazurek%2C+K">K Mazurek</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nadtochy%2C+P">P. Nadtochy</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=P%C3%A2rlog%2C+M">M P芒rlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roy%2C+R">R. Roy</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Spadaccini%2C+G">G Spadaccini</a> , et al. (4 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1309.7779v4-abstract-short" style="display: inline;"> In 129 Xe+ nat Sn central collisions from 8 to 25 MeV/A, the three-fragment exit channel occurs with a significant cross section. We show that these fragments arise from two successive binary splittings of a heavy composite system. The sequence of fragment production is determined. Strong Coulomb proximity effects are observed in the three-fragment final state. A comparison with Coulomb trajec-tor&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1309.7779v4-abstract-full').style.display = 'inline'; document.getElementById('1309.7779v4-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1309.7779v4-abstract-full" style="display: none;"> In 129 Xe+ nat Sn central collisions from 8 to 25 MeV/A, the three-fragment exit channel occurs with a significant cross section. We show that these fragments arise from two successive binary splittings of a heavy composite system. The sequence of fragment production is determined. Strong Coulomb proximity effects are observed in the three-fragment final state. A comparison with Coulomb trajec-tory calculations shows that the time scale between the consecutive break-ups decreases with increasing bombarding energy, becoming quasi-simultaneous above excitation energy E * = 4.0$\pm$0.5 MeV/A. This transition from sequential to simultaneous break-up was interpreted as the signature of the onset of multifragmentation for the three-fragment exit channel in this system. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1309.7779v4-abstract-full').style.display = 'none'; document.getElementById('1309.7779v4-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> 19 November, 2015; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 30 September, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 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">12 pages; 13 Figures; 4 Table; Accepted for publication in Physical Review C</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C 92, 064606 (2015) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1309.1336">arXiv:1309.1336</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1309.1336">pdf</a>, <a href="https://arxiv.org/format/1309.1336">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 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/10.1051/epjconf/20146611006">10.1051/epjconf/20146611006 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The european FAZIA initiative: a high-performance digital telescope array for heavy-ion studies </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Casini%2C+G">G. Casini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barlini%2C+S">S. Barlini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pasquali%2C+G">G. Pasquali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pastore%2C+G">G. Pastore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bini%2C+M">M. Bini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carboni%2C+S">S. Carboni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Olmi%2C+A">A. Olmi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Piantelli%2C+S">S. Piantelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Poggi%2C+G">G. Poggi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Stefanini%2C+A">A. Stefanini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Valdre%27%2C+S">S. Valdre&#39;</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bruno%2C+M">M. Bruno</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cinausero%2C+M">M. Cinausero</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Degerlier%2C+M">M. Degerlier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Edelbruck%2C+P">P. Edelbruck</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gramegna%2C+F">F. Gramegna</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guerzoni%2C+M">M. Guerzoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kordjasz%2C+A">A. Kordjasz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kozik%2C+T">T. Kozik</a> , et al. (14 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="1309.1336v1-abstract-short" style="display: inline;"> The european Fazia collaboration aims at building a new modular array for charged product identification to be employed for heavy-ion studies. The elementary module of the array is a Silicon-Silicon-CsI telescope, optimized for ion identification also via pulse shape analysis. The achievement of top performances imposes specific electronics which has been developed by FAZIA and features high quali&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1309.1336v1-abstract-full').style.display = 'inline'; document.getElementById('1309.1336v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1309.1336v1-abstract-full" style="display: none;"> The european Fazia collaboration aims at building a new modular array for charged product identification to be employed for heavy-ion studies. The elementary module of the array is a Silicon-Silicon-CsI telescope, optimized for ion identification also via pulse shape analysis. The achievement of top performances imposes specific electronics which has been developed by FAZIA and features high quality charge and current preamplifiers, coupled to fully digital front-end. During the initial R&amp;D phase, original and novel solutions have been tested in prototypes, obtaining unprecedented ion identification capabilities. FAZIA is now constructing a demonstrator array consisting of about two hundreds telescopes arranged in a compact and transportable configuration. In this contribution, we mainly summarize some aspects studied by FAZIA to improve the ion identification. Then we will briefly discuss the FAZIA program centered on experiments to be done with the demonstrator. First results on the isospin dynamics obtained with a reduced set-up demonstrate well the performance of the telescope and represent a good starting point towards future investigations with both stable and exotic beams. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1309.1336v1-abstract-full').style.display = 'none'; document.getElementById('1309.1336v1-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, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 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, 2 figures, Contribution to conference proceedings of the 25th International Nuclear Physics Conference (INPC 2013) Journal-ref: 25th International Nuclear Physics Conference (INPC 2013), Firenze : Italy (2013)</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1308.5302">arXiv:1308.5302</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1308.5302">pdf</a>, <a href="https://arxiv.org/format/1308.5302">other</a>]&nbsp;</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 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/10.1051/epjconf/20136207006">10.1051/epjconf/20136207006 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Sequential fissions of heavy nuclear systems </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">Diego Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boisjoli%2C+M">M. Boisjoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manduci%2C+L">L. Manduci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mazurek%2C+K">K. Mazurek</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nadtochy%2C+P+N">P. N. Nadtochy</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="1308.5302v1-abstract-short" style="display: inline;"> In Xe+Sn central collisions from 12 to 20 MeV/A measured with the INDRA 4$蟺$ multidetector, the three-fragment exit channel occurs with a significant cross section. In this contribution, we show that these fragments arise from two successive binary splittings of a heavy composite system. Strong Coulomb proximity effects are observed in the three-fragment final state. By comparison with Coulomb tra&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1308.5302v1-abstract-full').style.display = 'inline'; document.getElementById('1308.5302v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1308.5302v1-abstract-full" style="display: none;"> In Xe+Sn central collisions from 12 to 20 MeV/A measured with the INDRA 4$蟺$ multidetector, the three-fragment exit channel occurs with a significant cross section. In this contribution, we show that these fragments arise from two successive binary splittings of a heavy composite system. Strong Coulomb proximity effects are observed in the three-fragment final state. By comparison with Coulomb trajectory calculations, we show that the time scale between the consecutive break-ups decreases with increasing bombarding energy, becoming compatible with quasi-simultaneous multifragmentation above 18 MeV/A. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1308.5302v1-abstract-full').style.display = 'none'; document.getElementById('1308.5302v1-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 August, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 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">6 pages, 5 figures, contribution to conference proceedings of the Fifth International Workshop on Nuclear fission and Fission-Product Spectroscopy</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1308.5301">arXiv:1308.5301</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1308.5301">pdf</a>, <a href="https://arxiv.org/ps/1308.5301">ps</a>, <a href="https://arxiv.org/format/1308.5301">other</a>]&nbsp;</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 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/10.1088/1742-6596/436/1/012079">10.1088/1742-6596/436/1/012079 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Pseudo-critical clusterization in nuclear multifragmentation </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">Diego Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Botet%2C+R">R. Botet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ploszajczak%2C+M">M. Ploszajczak</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</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="1308.5301v1-abstract-short" style="display: inline;"> In this contribution we show that the biggest fragment charge distribution in central collisions of Xe+Sn leading to multifragmentation is an admixture of two asymptotic distributions observed for the lowest and highest bombarding energies. The evolution of the relative weights of the two components with bombarding energy is shown to be analogous to that observed as a function of time for the larg&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1308.5301v1-abstract-full').style.display = 'inline'; document.getElementById('1308.5301v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1308.5301v1-abstract-full" style="display: none;"> In this contribution we show that the biggest fragment charge distribution in central collisions of Xe+Sn leading to multifragmentation is an admixture of two asymptotic distributions observed for the lowest and highest bombarding energies. The evolution of the relative weights of the two components with bombarding energy is shown to be analogous to that observed as a function of time for the largest cluster produced in irreversible aggregation for a finite system. We infer that the size distribution of the largest fragment in nuclear multifragmentation is also characteristic of the time scale of the process, which is largely determined by the onset of radial expansion in this energy range. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1308.5301v1-abstract-full').style.display = 'none'; document.getElementById('1308.5301v1-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 August, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 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">4 pages, 3 figures, Contribution to conference proceedings of the 25th International Nuclear Physics Conference (INPC 2013)</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> 25th International Nuclear Physics Conference (INPC 2013), Firenze : Italie (2013) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1305.1517">arXiv:1305.1517</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1305.1517">pdf</a>, <a href="https://arxiv.org/ps/1305.1517">ps</a>, <a href="https://arxiv.org/format/1305.1517">other</a>]&nbsp;</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> </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.physletb.2013.05.004">10.1016/j.physletb.2013.05.004 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Constrained caloric curves and phase transition for hot nuclei </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">Bernard Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Piantelli%2C+S">S. Piantelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Raduta%2C+A+R">Ad. R. Raduta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ademard%2C+G">G. Ademard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P. Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Parlog%2C+M">M. Parlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pawlowski%2C+P">P. Pawlowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roy%2C+R">R. Roy</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vigilante%2C+M">M. Vigilante</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="1305.1517v1-abstract-short" style="display: inline;"> Simulations based on experimental data obtained from multifragmenting quasi-fused nuclei produced in central $^{129}$Xe + $^{nat}$Sn collisions have been used to deduce event by event freeze-out properties in the thermal excitation energy range 4-12 AMeV [Nucl. Phys. A809 (2008) 111]. From these properties and the temperatures deduced from proton transverse momentum fluctuations, constrained calor&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1305.1517v1-abstract-full').style.display = 'inline'; document.getElementById('1305.1517v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1305.1517v1-abstract-full" style="display: none;"> Simulations based on experimental data obtained from multifragmenting quasi-fused nuclei produced in central $^{129}$Xe + $^{nat}$Sn collisions have been used to deduce event by event freeze-out properties in the thermal excitation energy range 4-12 AMeV [Nucl. Phys. A809 (2008) 111]. From these properties and the temperatures deduced from proton transverse momentum fluctuations, constrained caloric curves have been built. At constant average volumes caloric curves exhibit a monotonic behaviour whereas for constrained pressures a backbending is observed. Such results support the existence of a first order phase transition for hot nuclei. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1305.1517v1-abstract-full').style.display = 'none'; document.getElementById('1305.1517v1-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 May, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 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">14 pages, 5 figures, accepted in Physics Letters B</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Physics Letters B 723, 1-3 (2013) 140-144 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1301.6805">arXiv:1301.6805</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1301.6805">pdf</a>, <a href="https://arxiv.org/ps/1301.6805">ps</a>, <a href="https://arxiv.org/format/1301.6805">other</a>]&nbsp;</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> </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.87.034617">10.1103/PhysRevC.87.034617 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Using Light Charged Particles to Probe the Asymmetry Dependence of the Nuclear Caloric Curve </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=McIntosh%2C+A+B">Alan B. McIntosh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonasera%2C+A">Aldo Bonasera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kohley%2C+Z">Zachary Kohley</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cammarata%2C+P+J">Paul J. Cammarata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hagel%2C+K">Kris Hagel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heilborn%2C+L">Lauren Heilborn</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mabiala%2C+J">Justin Mabiala</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=May%2C+L+W">Larry W. May</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">Paola Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Raphelt%2C+A">Andrew Raphelt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Souliotis%2C+G+A">George A. Souliotis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wuenschel%2C+S">Sara Wuenschel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Zarrella%2C+A">Andrew Zarrella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Yennello%2C+S+J">Sherry J. Yennello</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="1301.6805v1-abstract-short" style="display: inline;"> Recently, we observed a clear dependence of the nuclear caloric curve on neutron-proton asymmetry $\frac{N-Z}{A}$ through examination of fully reconstructed equilibrated quasi-projectile sources produced in heavy ion collisions at E/A = 35 MeV. In the present work, we extend our analysis using multiple light charged particle probes of the temperature. Temperatures are extracted with five distinct&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1301.6805v1-abstract-full').style.display = 'inline'; document.getElementById('1301.6805v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1301.6805v1-abstract-full" style="display: none;"> Recently, we observed a clear dependence of the nuclear caloric curve on neutron-proton asymmetry $\frac{N-Z}{A}$ through examination of fully reconstructed equilibrated quasi-projectile sources produced in heavy ion collisions at E/A = 35 MeV. In the present work, we extend our analysis using multiple light charged particle probes of the temperature. Temperatures are extracted with five distinct probes using a kinetic thermometer approach. Additionally, temperatures are extracted using two probes within a chemical thermometer approach (Albergo method). All seven measurements show a significant linear dependence of the source temperature on the source asymmetry. For the kinetic thermometer, the strength of the asymmetry dependence varies with the probe particle species in a way which is consistent with an average emission-time ordering. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1301.6805v1-abstract-full').style.display = 'none'; document.getElementById('1301.6805v1-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 January, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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">7 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/1212.3126">arXiv:1212.3126</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1212.3126">pdf</a>, <a href="https://arxiv.org/ps/1212.3126">ps</a>, <a href="https://arxiv.org/format/1212.3126">other</a>]&nbsp;</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"> Systematic study of symmetry energy within the SMM picture of multifragmentation </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonasera%2C+A">A. Bonasera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Souliotis%2C+G+A">G. A. Souliotis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cammarata%2C+P">P. Cammarata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wuenschel%2C+S">S. Wuenschel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tripathi%2C+R">R. Tripathi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kohley%2C+Z">Z. Kohley</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hagel%2C+K">K. Hagel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heilborn%2C+L">L. Heilborn</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mabiala%2C+J">J. Mabiala</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=May%2C+L+W">L. W. May</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=McIntosh%2C+A+B">A. B. McIntosh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Yennello%2C+S+J">S. J. Yennello</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="1212.3126v1-abstract-short" style="display: inline;"> A systematic study on the effect of secondary decay on the symmetry energy coefficient extracted by isoscaling and the recently proposed isobaric yield ratio methods within the Statistical Multifragmentation Model is performed. The correlations between the input symmetry energy coefficients and the calculated ones from both primary and secondary fragment yields are analysed. Results for secondary&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1212.3126v1-abstract-full').style.display = 'inline'; document.getElementById('1212.3126v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1212.3126v1-abstract-full" style="display: none;"> A systematic study on the effect of secondary decay on the symmetry energy coefficient extracted by isoscaling and the recently proposed isobaric yield ratio methods within the Statistical Multifragmentation Model is performed. The correlations between the input symmetry energy coefficients and the calculated ones from both primary and secondary fragment yields are analysed. Results for secondary fragments show that the best estimation of the input symmetry energy coefficient within SMM is obtained by the isoscaling method, using the yields of light fragments. A comparison to experimental results is also presented. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1212.3126v1-abstract-full').style.display = 'none'; document.getElementById('1212.3126v1-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> 13 December, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2012. </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 figures, 6 pages, Submitted to Phys. Rev. C</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1211.2134">arXiv:1211.2134</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1211.2134">pdf</a>, <a href="https://arxiv.org/ps/1211.2134">ps</a>, <a href="https://arxiv.org/format/1211.2134">other</a>]&nbsp;</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 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.nima.2012.12.113">10.1016/j.nima.2012.12.113 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Experimental determination of the quasi-projectile mass with measured neutrons </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Zarrella%2C+A">A. Zarrella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonasera%2C+A">A. Bonasera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonasera%2C+G">G. Bonasera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cammarata%2C+P">P. Cammarata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heilborn%2C+L">L. Heilborn</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kohley%2C+Z">Z. Kohley</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mabiala%2C+J">J. Mabiala</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=May%2C+L+W">L. W. May</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=McIntosh%2C+A+B">A. B. McIntosh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Raphelt%2C+A">A. Raphelt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Souliotis%2C+G+A">G. A. Souliotis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Yennello%2C+S+J">S. J. Yennello</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="1211.2134v1-abstract-short" style="display: inline;"> The investigation of the isospin dependence of multifragmentation reactions relies on precise reconstruction of the fragmenting source. The criteria used to assign free emitted neutrons, detected with the TAMU Neutron Ball, to the quasi-projectile source are investigated in the framework of two different simulation codes. Overall and source-specific detection efficiencies for multifragmentation ev&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1211.2134v1-abstract-full').style.display = 'inline'; document.getElementById('1211.2134v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1211.2134v1-abstract-full" style="display: none;"> The investigation of the isospin dependence of multifragmentation reactions relies on precise reconstruction of the fragmenting source. The criteria used to assign free emitted neutrons, detected with the TAMU Neutron Ball, to the quasi-projectile source are investigated in the framework of two different simulation codes. Overall and source-specific detection efficiencies for multifragmentation events are found to be model independent. The equivalence of the two different methods used to assign experimentally detected charged particles and neutrons to the emitting source is shown. The method used experimentally to determine quasi-projectile emitted free neutron multiplicity is found to be reasonably accurate and sufficiently precise as to allow for the study of well-defined quasi-projectile sources. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1211.2134v1-abstract-full').style.display = 'none'; document.getElementById('1211.2134v1-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> 9 November, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2012. </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">10 pages, 8 figures. To be submitted to Nucl. Instr. and Meth. A</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1210.0691">arXiv:1210.0691</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1210.0691">pdf</a>, <a href="https://arxiv.org/ps/1210.0691">ps</a>, <a href="https://arxiv.org/format/1210.0691">other</a>]&nbsp;</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> </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.110.172701">10.1103/PhysRevLett.110.172701 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Nuclear multifragmentation time-scale and fluctuations of largest fragment size </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Gruyer%2C+D">D. Gruyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Botet%2C+R">R. Botet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ploszajczak%2C+M">M. Ploszajczak</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ademard%2C+G">G. Ademard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boisjoli%2C+M">M. Boisjoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P. Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manduci%2C+L">L. Manduci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pawlowski%2C+P">P. Pawlowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Spadaccini%2C+G">G. Spadaccini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vigilante%2C+M">M. Vigilante</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wieleczko%2C+J+P">J. P. Wieleczko</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="1210.0691v2-abstract-short" style="display: inline;"> Distributions of the largest fragment charge, Zmax, in multifragmentation reactions around the Fermi energy can be decomposed into a sum of a Gaussian and a Gumbel distribution, whereas at much higher or lower energies one or the other distribution is asymptotically dominant. We demonstrate the same generic behavior for the largest cluster size in critical aggregation models for small systems, in&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1210.0691v2-abstract-full').style.display = 'inline'; document.getElementById('1210.0691v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1210.0691v2-abstract-full" style="display: none;"> Distributions of the largest fragment charge, Zmax, in multifragmentation reactions around the Fermi energy can be decomposed into a sum of a Gaussian and a Gumbel distribution, whereas at much higher or lower energies one or the other distribution is asymptotically dominant. We demonstrate the same generic behavior for the largest cluster size in critical aggregation models for small systems, in or out of equilibrium, around the critical point. By analogy with the time-dependent irreversible aggregation model, we infer that Zmax distributions are characteristic of the multifragmentation time-scale, which is largely determined by the onset of radial expansion in this energy range. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1210.0691v2-abstract-full').style.display = 'none'; document.getElementById('1210.0691v2-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> 9 April, 2013; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 2 October, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Accepted for publication in Physical Review Letters on 8/4/2013</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1209.6535">arXiv:1209.6535</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1209.6535">pdf</a>, <a href="https://arxiv.org/format/1209.6535">other</a>]&nbsp;</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 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.86.044617">10.1103/PhysRevC.86.044617 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> New isospin e ffects in central heavy-ion collisions at Fermi energies </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Gagnon-Moisan%2C+F">F. Gagnon-Moisan</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+-">M. -F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Colonna%2C+M">M. Colonna</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roy%2C+R">R. Roy</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ademard%2C+G">G. Ademard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boisjoli%2C+M">M. Boisjoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P. Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=ee%2C+E+L">E. Legou ee</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manduci%2C+L">L. Manduci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Napolitani%2C+P">P. Napolitani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=P%C3%A2rlog%2C+M">M. P芒rlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pawlowski%2C+P">P. Pawlowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vigilante%2C+M">M. Vigilante</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="1209.6535v1-abstract-short" style="display: inline;"> Isospin e ffects on multifragmentation properties were studied thanks to nuclear collisions between di fferent isotopes of xenon beams and tin targets. It is shown that, in central collisions leading to multifragmentation, the mean number of fragments and their mean kinetic energy increase with the neutron-richness of the total system. Comparisons with a stochastic transport model allow to attribu&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.6535v1-abstract-full').style.display = 'inline'; document.getElementById('1209.6535v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1209.6535v1-abstract-full" style="display: none;"> Isospin e ffects on multifragmentation properties were studied thanks to nuclear collisions between di fferent isotopes of xenon beams and tin targets. It is shown that, in central collisions leading to multifragmentation, the mean number of fragments and their mean kinetic energy increase with the neutron-richness of the total system. Comparisons with a stochastic transport model allow to attribute the multiplicity increase to the multifragmentation stage, before secondary decay. The total charge bound in fragments is proposed as an alternate variable to quantify preequilibrium emission and to investigate symmetry energy e ffects. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.6535v1-abstract-full').style.display = 'none'; document.getElementById('1209.6535v1-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 September, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2012. </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">10 pages. 6 figures. Submitted to Physical Review C</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Physical Review C 86 (2012) 044617 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1209.5961">arXiv:1209.5961</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1209.5961">pdf</a>, <a href="https://arxiv.org/ps/1209.5961">ps</a>, <a href="https://arxiv.org/format/1209.5961">other</a>]&nbsp;</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 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/10.1088/1742-6596/420/1/012092">10.1088/1742-6596/420/1/012092 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The ASY-EOS experiment at GSI: investigating the symmetry energy at supra-saturation densities </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chartier%2C+M">M. Chartier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=F%C3%A9vre%2C+A+L">A. Le F茅vre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gannon%2C+S">S. Gannon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ga%C5%A1pari%C4%87%2C+I">I. Ga拧pari膰</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ki%C5%A1%2C+M">M. Ki拧</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kupny%2C+S">S. Kupny</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Leifels%2C+Y">Y. Leifels</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lemmon%2C+R+C">R. C. Lemmon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=%C5%81ukasik%2C+J">J. 艁ukasik</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Paw%C5%82owski%2C+P">P. Paw艂owski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Santoro%2C+S">S. Santoro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Trautmann%2C+W">W. Trautmann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Veselsky%2C+M">M. Veselsky</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Acosta%2C+L">L. Acosta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adamczyk%2C+M">M. Adamczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Ajlan%2C+A">A. Al-Ajlan</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Garawi%2C+M">M. Al-Garawi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Homaidhi%2C+S">S. Al-Homaidhi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a> , et al. (67 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="1209.5961v1-abstract-short" style="display: inline;"> The elliptic-flow ratio of neutrons with respect to protons in reactions of neutron rich heavy-ions systems at intermediate energies has been proposed as an observable sensitive to the strength of the symmetry term in the nuclear Equation Of State (EOS) at supra-saturation densities. The recent results obtained from the existing FOPI/LAND data for $^{197}$Au+$^{197}$Au collisions at 400 MeV/nucleo&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.5961v1-abstract-full').style.display = 'inline'; document.getElementById('1209.5961v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1209.5961v1-abstract-full" style="display: none;"> The elliptic-flow ratio of neutrons with respect to protons in reactions of neutron rich heavy-ions systems at intermediate energies has been proposed as an observable sensitive to the strength of the symmetry term in the nuclear Equation Of State (EOS) at supra-saturation densities. The recent results obtained from the existing FOPI/LAND data for $^{197}$Au+$^{197}$Au collisions at 400 MeV/nucleon in comparison with the UrQMD model allowed a first estimate of the symmetry term of the EOS but suffer from a considerable statistical uncertainty. In order to obtain an improved data set for Au+Au collisions and to extend the study to other systems, a new experiment was carried out at the GSI laboratory by the ASY-EOS collaboration in May 2011. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.5961v1-abstract-full').style.display = 'none'; document.getElementById('1209.5961v1-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> 26 September, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2012. </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">Talk given by P. Russotto at the 11th International Conference on Nucleus-Nucleus Collisions (NN2012), San Antonio, Texas, USA, May 27-June 1, 2012. To appear in the NN2012 Proceedings in Journal of Physics: Conference Series (JPCS)</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1208.4887">arXiv:1208.4887</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1208.4887">pdf</a>, <a href="https://arxiv.org/ps/1208.4887">ps</a>, <a href="https://arxiv.org/format/1208.4887">other</a>]&nbsp;</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 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.physletb.2012.12.073">10.1016/j.physletb.2012.12.073 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Asymmetry Dependence of the Nuclear Caloric Curve </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=McIntosh%2C+A+B">Alan B. McIntosh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonasera%2C+A">Aldo Bonasera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cammarata%2C+P">Paul Cammarata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hagel%2C+K">Kris Hagel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heilborn%2C+L">Lauren Heilborn</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kohley%2C+Z">Zachary Kohley</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mabiala%2C+J">Justin Mabiala</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=May%2C+L+W">Larry W. May</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">Paola Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Raphelt%2C+A">Andrew Raphelt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Souliotis%2C+G+A">George A. Souliotis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wuenschel%2C+S">Sara Wuenschel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Zarrella%2C+A">Andrew Zarrella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Yennello%2C+S+J">Sherry J. Yennello</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="1208.4887v1-abstract-short" style="display: inline;"> A basic feature of the nuclear equation of state is not yet understood: the dependence of the nuclear caloric curve on the neutron-proton asymmetry. Predictions of theoretical models differ on the magnitude and even the sign of this dependence. In this work, the nuclear caloric curve is examined for fully reconstructed quasi-projectiles around mass A=50. The caloric curve extracted with the moment&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1208.4887v1-abstract-full').style.display = 'inline'; document.getElementById('1208.4887v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1208.4887v1-abstract-full" style="display: none;"> A basic feature of the nuclear equation of state is not yet understood: the dependence of the nuclear caloric curve on the neutron-proton asymmetry. Predictions of theoretical models differ on the magnitude and even the sign of this dependence. In this work, the nuclear caloric curve is examined for fully reconstructed quasi-projectiles around mass A=50. The caloric curve extracted with the momentum quadrupole fluctuation thermometer shows that the temperature varies linearly with quasi-projectile asymmetry (N-Z)/A. An increase in asymmetry of 0.15 units corresponds to a decrease in temperature on the order of 1 MeV. These results also highlight the importance of a full quasi-projectile reconstruction in the study of thermodynamic properties of hot nuclei. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1208.4887v1-abstract-full').style.display = 'none'; document.getElementById('1208.4887v1-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> 23 August, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Physics Letters B 719, 337 (2013) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1202.3370">arXiv:1202.3370</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1202.3370">pdf</a>, <a href="https://arxiv.org/ps/1202.3370">ps</a>, <a href="https://arxiv.org/format/1202.3370">other</a>]&nbsp;</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 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.85.034617">10.1103/PhysRevC.85.034617 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Constraining the Symmetry Term in the Nuclear Equation of State at Sub-Saturation Densities and Finite Temperatures </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonasera%2C+A">A. Bonasera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=McIntosh%2C+A">A. McIntosh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tripathi%2C+R">R. Tripathi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galanopoulos%2C+S">S. Galanopoulos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hagel%2C+K">K. Hagel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heilborn%2C+L">L. Heilborn</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kohley%2C+Z">Z. Kohley</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=May%2C+L+W">L. W. May</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mehlman%2C+M">M. Mehlman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Soisson%2C+S+N">S. N. Soisson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Souliotis%2C+G+A">G. A. Souliotis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Shetty%2C+D+V">D. V. Shetty</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Smith%2C+W+B">W. B. Smith</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Stein%2C+B+C">B. C. Stein</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wuenschel%2C+S">S. Wuenschel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Yennello%2C+S+J">S. J. Yennello</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="1202.3370v1-abstract-short" style="display: inline;"> Methods of extraction of the symmetry energy (or enthalpy) coefficient to temperature ratio from isobaric and isotopic yields of fragments produced in Fermi-energy heavy-ion collisions are discussed. We show that the methods are consistent when the hot fragmenting source is well characterized and its excitation energy and isotopic composition are properly taken into account. The results are indepe&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1202.3370v1-abstract-full').style.display = 'inline'; document.getElementById('1202.3370v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1202.3370v1-abstract-full" style="display: none;"> Methods of extraction of the symmetry energy (or enthalpy) coefficient to temperature ratio from isobaric and isotopic yields of fragments produced in Fermi-energy heavy-ion collisions are discussed. We show that the methods are consistent when the hot fragmenting source is well characterized and its excitation energy and isotopic composition are properly taken into account. The results are independent of the mass number of the detected fragments, which suggests that their fate is decided very early in the reaction. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1202.3370v1-abstract-full').style.display = 'none'; document.getElementById('1202.3370v1-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> 15 February, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2012. </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, 9 figures, submitted to Phys. Rev. C and accepted for publication</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1202.0192">arXiv:1202.0192</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1202.0192">pdf</a>, <a href="https://arxiv.org/ps/1202.0192">ps</a>, <a href="https://arxiv.org/format/1202.0192">other</a>]&nbsp;</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 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.86.011602">10.1103/PhysRevC.86.011602 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Persistence of odd-even staggering in charged fragment yields from the 112Sn+58Ni collision at 35 MeV/nucleon </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Casini%2C+G">G. Casini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Piantelli%2C+S">S. Piantelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maurenzig%2C+P+R">P. R. Maurenzig</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Olmi%2C+A">A. Olmi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bardelli%2C+L">L. Bardelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barlini%2C+S">S. Barlini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benelli%2C+M">M. Benelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bini%2C+M">M. Bini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Calviani%2C+M">M. Calviani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mangiarotti%2C+A">A. Mangiarotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pasquali%2C+G">G. Pasquali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Poggi%2C+G">G. Poggi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Stefanini%2C+A+A">A. A. Stefanini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bruno%2C+M">M. Bruno</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Morelli%2C+L">L. Morelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kravchuk%2C+V+L">V. L. Kravchuk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzano%27%2C+G">G. Lanzano&#39;</a> , et al. (11 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="1202.0192v2-abstract-short" style="display: inline;"> Odd-even staggering effects on charge distributions are investigated for fragments produced in semiperipheral and central collisions of 112Sn+58Ni at 35 MeV/nucleon. For fragments with Z&lt;16 one observes a clear overproduction of even charges, which decreases for heavier fragments. In peripheral collisions staggering effects persist up to Z about 40. For light fragments, staggering appears to be su&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1202.0192v2-abstract-full').style.display = 'inline'; document.getElementById('1202.0192v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1202.0192v2-abstract-full" style="display: none;"> Odd-even staggering effects on charge distributions are investigated for fragments produced in semiperipheral and central collisions of 112Sn+58Ni at 35 MeV/nucleon. For fragments with Z&lt;16 one observes a clear overproduction of even charges, which decreases for heavier fragments. In peripheral collisions staggering effects persist up to Z about 40. For light fragments, staggering appears to be substantially independent of the centrality of the collisions, suggesting that it is mainly related to the last few steps in the decay of hot nuclei. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1202.0192v2-abstract-full').style.display = 'none'; document.getElementById('1202.0192v2-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> 9 July, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 1 February, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2012. </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, 6 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C 86, 011602 (2012) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1111.2965">arXiv:1111.2965</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1111.2965">pdf</a>, <a href="https://arxiv.org/ps/1111.2965">ps</a>, <a href="https://arxiv.org/format/1111.2965">other</a>]&nbsp;</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"> Experimental evidence of quantum quenching of fluctuations in heavy ion collisions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Stein%2C+B+C">B. C. Stein</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Zheng%2C+H">H. Zheng</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonasera%2C+A">A. Bonasera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Soisson%2C+S+N">S. N. Soisson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=McIntosh%2C+A">A. McIntosh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tripathi%2C+R">R. Tripathi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Souliotis%2C+G+A">G. A. Souliotis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keksis%2C+A+L">A. L. Keksis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wuenschel%2C+S">S. Wuenschel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kohley%2C+Z">Z. Kohley</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=May%2C+L+W">L. W. May</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Yennello%2C+S+J">S. J. Yennello</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="1111.2965v1-abstract-short" style="display: inline;"> The first experimental results of a new quantum method for calculating nuclear temperature and density of fragmenting heavy ions is presented. This method is based on fluctuations in the event quadrupole momentum and fragment multiplicity distributions of light Fermions. The cal- culated temperatures are lower than those obtained with a similar classical method. Quenching of the normalized multipl&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1111.2965v1-abstract-full').style.display = 'inline'; document.getElementById('1111.2965v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1111.2965v1-abstract-full" style="display: none;"> The first experimental results of a new quantum method for calculating nuclear temperature and density of fragmenting heavy ions is presented. This method is based on fluctuations in the event quadrupole momentum and fragment multiplicity distributions of light Fermions. The cal- culated temperatures are lower than those obtained with a similar classical method. Quenching of the normalized multiplicity distributions of light fermions due to Pauli blocking is also observed. These results indicate a need for a quantum treatment when dealing with statistical properties of fragmenting heavy-ions. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1111.2965v1-abstract-full').style.display = 'none'; document.getElementById('1111.2965v1-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 November, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2011. </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, 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/1002.1645">arXiv:1002.1645</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1002.1645">pdf</a>, <a href="https://arxiv.org/ps/1002.1645">ps</a>, <a href="https://arxiv.org/format/1002.1645">other</a>]&nbsp;</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 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.105.142701">10.1103/PhysRevLett.105.142701 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> New scalings in nuclear fragmentation </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Raduta%2C+A+R">Ad. R. Raduta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gagnon-Moisan%2C+F">F. Gagnon-Moisan</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P. Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lukasik%2C+J">J. Lukasik</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=P%C3%A2rlog%2C+M">M. P芒rlog</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roy%2C+R">R. Roy</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Spadaccini%2C+G">G. Spadaccini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vigilante%2C+M">M. Vigilante</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wieleczko%2C+J+P">J. P. Wieleczko</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Zwieglinski%2C+B">B. Zwieglinski</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="1002.1645v2-abstract-short" style="display: inline;"> Fragment partitions of fragmenting hot nuclei produced in central and semiperipheral collisions have been compared in the excitation energy region 4-10 MeV per nucleon where radial collective expansion takes place. It is shown that, for a given total excitation energy per nucleon, the amount of radial collective energy fixes the mean fragment multiplicity. It is also shown that, at a given total e&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1002.1645v2-abstract-full').style.display = 'inline'; document.getElementById('1002.1645v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1002.1645v2-abstract-full" style="display: none;"> Fragment partitions of fragmenting hot nuclei produced in central and semiperipheral collisions have been compared in the excitation energy region 4-10 MeV per nucleon where radial collective expansion takes place. It is shown that, for a given total excitation energy per nucleon, the amount of radial collective energy fixes the mean fragment multiplicity. It is also shown that, at a given total excitation energy per nucleon, the different properties of fragment partitions are completely determined by the reduced fragment multiplicity (fragment multiplicity normalized to the source size). Freeze-out volumes seem to play a role in the scalings observed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1002.1645v2-abstract-full').style.display = 'none'; document.getElementById('1002.1645v2-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 September, 2010; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 8 February, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2010. </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, submitted to PRL</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.Lett.105:142701,2010 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/nucl-ex/0609045">arXiv:nucl-ex/0609045</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/nucl-ex/0609045">pdf</a>, <a href="https://arxiv.org/ps/nucl-ex/0609045">ps</a>, <a href="https://arxiv.org/format/nucl-ex/0609045">other</a>]&nbsp;</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 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/epjst/e2007-00255-y">10.1140/epjst/e2007-00255-y <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Isotope analysis in central heavy ion collisions at intermediate energies </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Collaboration%2C+N">NUCL-EX Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=%3A"> :</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Abbondanno%2C+U">U. Abbondanno</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bardelli%2C+L">L. Bardelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barlini%2C+S">S. Barlini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bini%2C+M">M. Bini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bruno%2C+M">M. Bruno</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cannata%2C+F">F. Cannata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casini%2C+G">G. Casini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiari%2C+M">M. Chiari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Agostino%2C+M">M. D&#39;Agostino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=DeSanctis%2C+J">J. DeSanctis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giussani%2C+A">A. Giussani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gramegna%2C+F">F. Gramegna</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kravchuk%2C+V+L">V. L. Kravchuk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanchais%2C+A+L">A. L. Lanchais</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Moroni%2C+A">A. Moroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nannini%2C+A">A. Nannini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Olmi%2C+A">A. Olmi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ordine%2C+A">A. Ordine</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pasquali%2C+G">G. Pasquali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Piantelli%2C+S">S. Piantelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Poggi%2C+G">G. Poggi</a> , et al. (1 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="nucl-ex/0609045v1-abstract-short" style="display: inline;"> Symmetry energy is a key quantity in the study of the equation of state of asymmetric nuclear matter. Heavy ion collisions at low and intermediate energies, performed at Laboratori Nazionali di Legnaro and Laboratori Nazionali del Sud, can be used to extract information on the symmetry energy coefficient Csym, which is currently poorly known but relevant both for astrophysics and for structure o&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0609045v1-abstract-full').style.display = 'inline'; document.getElementById('nucl-ex/0609045v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="nucl-ex/0609045v1-abstract-full" style="display: none;"> Symmetry energy is a key quantity in the study of the equation of state of asymmetric nuclear matter. Heavy ion collisions at low and intermediate energies, performed at Laboratori Nazionali di Legnaro and Laboratori Nazionali del Sud, can be used to extract information on the symmetry energy coefficient Csym, which is currently poorly known but relevant both for astrophysics and for structure of exotic nuclei. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0609045v1-abstract-full').style.display = 'none'; document.getElementById('nucl-ex/0609045v1-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> 29 September, 2006; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2006. </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">2 pages, 1 figure. Proceedings of 7th International Conference on Radioactive Nuclear Beams (RNB7), to be published in The European Physical Journal A</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur.Phys.J.ST150:21-22,2007 </p> </li> </ol> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <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>&nbsp;&nbsp;</span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary"> <!-- MetaColumn 1 --> <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> <!-- end MetaColumn 1 --> <!-- MetaColumn 2 --> <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> <!-- end MetaColumn 2 --> </div> </footer> <script src="https://static.arxiv.org/static/base/1.0.0a5/js/member_acknowledgement.js"></script> </body> </html>

Pages: 1 2 3 4 5 6 7 8 9 10