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<p>Of interest for the EO group...<br>
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<div id="divRplyFwdMsg" dir="ltr"><font face="Calibri, sans-serif" color="#000000" style="font-size:11pt"><b>From:</b> Joonas Nättilä <joonas.nattila@su.se><br>
<b>Sent:</b> Monday, June 4, 2018 1:58 PM<br>
<b>To:</b> people@nordita.org; alla@astro.su.se<br>
<b>Cc:</b> Andrew W. Steiner<br>
<b>Subject:</b> Nordita Astrophysics Seminar Thu. June 7 @ 13:30</font>
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<div><span class="">Dear All,</span><span class=""><br class="">
</span><span class=""><br class="">
</span><span class="">The</span><span class=""></span><span class=""> next </span><span class="">Nordita</span><span class=""> </span><span class="">Astrophysics</span><span class=""> </span><span class="">Semi</span><span class="">nar</span><span class=""> will
be on </span><span class=""><b class="">Thursday June 7 at 13:30</b></span><span class=""> (room 112:028</span><span class="">, </span><b class=""><span class="">Nordita</span><span class=""> South</span><span class=""> </span><span class="">Building</span></b><span class="">).
Note the day since our usual Wednesday is a national holiday.</span>
<div class=""><span class=""><br class="">
</span></div>
<span class=""><br class="">
<br class="">
Speaker:<br class="">
Andrew Steiner (Univ. Tennessee / Oak Ridge National Lab)<br class="">
<br class="">
Title: <br class="">
The Nature of Dense Matter from Multi-Messenger Observations of Neutron Stars<br class="">
<br class="">
Abstract: <br class="">
Constructing the most complete picture of the neutron star interior is (currently) only possible through the combined analysis of several data sets. We use Bayesian inference to combine neutron star observations, nuclear experiments, and nuclear theory. In
this talk, I will begin by describing some of the methodology before presenting our predictions for neutron star tidal deformabilities and their relationship to GW170817. I will then go beyond the bulk thermodynamics of dense matter and show how our work is
beginning to constrain the proton-to-neutron ratio and the nature of superfluidity in dense matter. Finally, I will describe how our results can be used as the input for more accurate simulations of neutron star mergers.<br class="">
<br class="">
Welcome!<br class="">
<br class="">
Add to calendar: </span> <a href="http://agenda.albanova.se/conferenceDisplay.py/ical?confId=6562" class="">http://agenda.albanova.se/conferenceDisplay.py/ical?confId=6562</a><span class=""><br class="">
<br class="">
<br class="">
<div class="">Cheers,<br class="">
Joonas<br class="">
<br class="">
---<br class="">
Nordita Fellow<br class="">
KTH Royal Institute of Technology and Stockholm University<br class="">
Roslagstullsbacken 17, SE-10691 Stockholm, Sweden<br class="">
<br class="">
<a href="http://natj.github.io" class="">http://natj.github.io</a><br class="">
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<br class="">
</span></div>
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