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Ilya Mandel
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More wesbite tweaks
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‎index.html‎

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@@ -178,151 +178,71 @@ <h1 style="font-size:3em">Our
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</header>
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<!-- <div class="column" style="font-weight:bold"> -->
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<div>
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<!-- <h2 align="center">Current Developers</h2> -->
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<h2>Current Developers</h2>
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<ul style=
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"list-style-type:disc">
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<li><a href=
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"http://www.broekgaarden.nl/floor/wordpress/">
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Floor Broekgaarden</a>
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</li>
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<li><a href=
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"https://ryosuke-hirai.github.io/">
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Ryosuke Hirai</a>
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</li>
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<li><a href=
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"https://www.uva.nl/en/profile/j/u/s.justham/s.justham.html">
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Stephen Justham</a>
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</li>
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<li> Veome Kapil </li>
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<li><a href=
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"https://themikelau.github.io/">
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Mike Lau</a>
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</li>
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<li><a href=
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"http://ilyamandel.github.io/">
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Ilya Mandel</a>
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</li>
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<li><a href=
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"http://www.selmademink.com/">
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Selma de Mink</a>
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</li>
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<li> JD Merritt </li>
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<li><a href=
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"http://rileys.id.au/JeffsResearch.html">
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Jeff Riley</a>
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</li>
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<li>Tim Riley</li>
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<li>Nicolas Rodriguez-Segovia</li>
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<li>Isobel Romero-Shaw</li>
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<li><a href=
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"https://liekevanson.github.io/">
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Lieke van Son</a>
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</li>
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<li>Simon Stevenson</li>
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<li>Alejandro
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Vigna-Gomez</li>
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<li>Serena Vinciguerra</li>
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<li><a href=
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"https://reinhold-willcox.github.io/home.html">
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Reinhold Willcox</a>
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</li>
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<li><a href=
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"https://tomwagg.com">Tom
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Wagg</a>
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</li>
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</ul>
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</div>
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<!-- <div class="column" style="font-weight:bold"> -->
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<div>
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<!-- <h2 align="center">Past Developers</h2> -->
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<h2>Past Developers</h2>
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<ul style=
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"list-style-type:disc">
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<li>Poojan Agrawal</li>
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<li>Jim Barrett</li>
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<li>Kit Boyett</li>
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<li>Ben Bradnick</li>
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<li>Debatri
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Chattopadhyay</li>
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<li>Sebastian Gaebel</li>
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<li>Fabian Gittins</li>
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<li>George Howitt</li>
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<li>Lokesh Khandelwal</li>
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<li>Floris Kummer</li>
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<li><a href=
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"https://cneijssel.github.io/cneijssel/">
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Coenraad Neijssel</a>
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</li>
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</ul>
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</div>
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<!-- <div class="column" style="font-weight:bold"> -->
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<div>
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<!-- <h2 align="center">Collaborators</h2> -->
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<h2>Collaborators</h2>
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<ul style=
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"list-style-type:disc">
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<li>Simone Bavera</li>
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<li>Chris Belczynski</li>
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<li>Christopher Berry</li>
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<li>JJ Eldridge</li>
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<li>Tassos Fragos</li>
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<li>Jarrod Hurley</li>
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<li>Morgan MacLeod</li>
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<li>Philipp
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Podsiadlowski</li>
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<li>Ashley Ruiter</li>
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<li>Dorottya Szécsi</li>
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</ul>
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</div>
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<div>
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<!-- <h2 align="center">Current Developers</h2> -->
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<h2>Current Developers</h2>
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<ul style="list-style-type:disc">
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<li>Adam Brcek</li>
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<li><a href="http://www.broekgaarden.nl/floor/wordpress/">Floor Broekgaarden</a></li>
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<li>Paul Disberg</li>
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<li><a href="https://ryosuke-hirai.github.io/">Ryosuke Hirai</a></li>
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<li>Veome Kapil</li>
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<li><a href="https://themikelau.github.io/">Mike Lau</a></li>
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<li><a href="http://ilyamandel.github.io/">Ilya Mandel</a></li>
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<li>JD Merritt</li>
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<li><a href="http://rileys.id.au/JeffsResearch.html"> Jeff Riley</a></li>
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<li>Yuzhe (Robert) Song</li>
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<li>Simon Stevenson</li>
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<li><a href="https://liekevanson.github.io/">Lieke van Son</a></li>
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<li>Avi Vajpeyi</li>
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<li>Alejandro Vigna Gomez</li>
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<li><a href="https://reinhold-willcox.github.io/home.html">Reinhold Willcox</a></li>
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</ul>
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</div>
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<!-- <div class="column" style="font-weight:bold"> -->
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<div>
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<!-- <h2 align="center">Past Developers</h2> -->
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<h2>Past Developers</h2>
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<ul style="list-style-type:disc">
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<li>Poojan Agrawal</li>
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<li>Jim Barrett</li>
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<li>Adam Boesky</li>
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<li>Kit Boyett</li>
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<li>Ben Bradnick</li>
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<li>Debatri Chattopadhyay</li>
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<li>Sebastian Gaebel</li>
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<li>Fabian Gittins</li>
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<li>George Howitt</li>
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<li>Lokesh Khandelwal</li>
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<li>Floris Kummer</li>
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<li><a href= "https://cneijssel.github.io/cneijssel/">Coenraad Neijssel</a>
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<li>Tim Riley</li>
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<li>Nicholas Rodriguez-Segovia</li>
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<li>Isobel Romero-Shaw</li>
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<li>Serena Vinciguerra</li>
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<li><a href="https://tomwagg.com">Tom Wagg</a>
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</ul>
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</div>
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<!-- <div class="column" style="font-weight:bold"> -->
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<div>
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<!-- <h2 align="center">Current and past collaborators</h2> -->
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<h2>Collaborators</h2>
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<ul style="list-style-type:disc">
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<li>Simone Bavera</li>
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<li>Chris Belczynski</li>
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<li>Christopher Berry</li>
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<li><a href= "http://www.selmademink.com/">Selma de Mink</a></li>
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<li>JJ Eldridge</li>
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<li>Tassos Fragos</li>
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<li><a href= "https://www.uva.nl/en/profile/j/u/s.justham/s.justham.html">Stephen Justham</a></li>
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<li>Jarrod Hurley</li>
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<li>Morgan MacLeod</li>
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<li>Philipp Podsiadlowski</li>
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<li>Ashley Ruiter</li>
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<li>Dorottya Szécsi</li>
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</ul>
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</div>
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</section>
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</div>
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</div>

‎science.html‎

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is publicly available at <a href=
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"https://github.com/TeamCOMPAS/COMPAS">
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https://github.com/TeamCOMPAS/COMPAS</a>,
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Further information can be found in
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Further information can be found in the
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<a href=
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"http://arXiv.org/abs/2109.10352">the
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COMPAS methods paper</a> or in more
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"http://arXiv.org/abs/2109.10352">
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first </a> and
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<a href=
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"http://arXiv.org/abs/2506.02316">
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second </a>
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COMPAS methods papers or in more
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technical <a href=
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"https://compas.science/docs">documentation</a>.
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The <a href=
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"https://zenodo.org/record/6346444#.YjGanxBByfU">
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latest COMPAS data release</a> is
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latest COMPAS data releases</a> are
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available through our <a href=
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"https://zenodo.org/communities/compas/">
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zenodo community.</a></p>
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zenodo community</a> and/or <a href="https://gwlandscape.org.au/publications/">GWLandscape</a>.</p>
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</article>
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<!-- Papers Header -->
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<header id="papers" class="major">
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<!-- Description -->
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<p>
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We perform population synthesis of massive binaries to study the mergers ofneutron stars (NSs) and black holes (BHs) with the cores of their giantsecondaries during common envelope evolution (CEE). We use different values ofthe efficiency parameter $\alpha_{\rm CE}$ in the framework of the energyformalism for traditional CEE ($\alpha_{\rm CE} \leq 1$) and includingadditional energy sources to unbind the envelope ($\alpha_{\rm CE} &gt; 1$). Weconstrain the possible values of $\alpha_{\rm CE}$ by comparing the results ofour simulations with local rate densities of binary compact object mergers asinferred from gravitational waves observations. We find two primaryevolutionary pathways of binary systems that result in NS-core mergers, whileonly one of them can also lead to the merger of a BH with the core of the giantstar. We explore the zero age main sequence (ZAMS) statistical properties ofsystems that result in NS/BH-core mergers and find that the two evolutionarychannels correspond to a bimodal distribution of orbital separations. Weestimate the percentage of the mergers&#39; event rates relative to core collapsesupernovae (CCSNe). We include the effect of mass accreted by the NS/BH duringCEE in a separate set of simulations and find it does not affect the mergers&#39;event rates.
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We perform population synthesis of massive binaries to study the mergers of neutron stars (NSs) and black holes (BHs) with the cores of their giant secondaries during common envelope evolution (CEE). We use different values of the efficiency parameter $\alpha_{\rm CE}$ in the framework of the energy formalism for traditional CEE ($\alpha_{\rm CE} \leq 1$) and including additional energy sources to unbind the envelope ($\alpha_{\rm CE} &gt; 1$). We constrain the possible values of $\alpha_{\rm CE}$ by comparing the results of our simulations with local rate densities of binary compact object mergers as inferred from gravitational waves observations. We find two primary evolutionary pathways of binary systems that result in NS-core mergers, while only one of them can also lead to the merger of a BH with the core of the giant star. We explore the zero age main sequence (ZAMS) statistical properties ofsystems that result in NS/BH-core mergers and find that the two evolutionary channels correspond to a bimodal distribution of orbital separations. We estimate the percentage of the mergers&#39; event rates relative to core collapses upernovae (CCSNe). We include the effect of mass accreted by the NS/BH duringCEE in a separate set of simulations and find it does not affect the mergers event rates.
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</p>
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</div>
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</article>

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