<html><head><meta http-equiv="Content-Type" content="text/html charset=utf-8"></head><body style="word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space;" class="">Dear all,<div class=""><br class=""></div><div class="">our next speaker at the EO meeting (oct 11, 13:00, @KTH meeting room on the 5th floor),</div><div class="">will be <b class="">André da SIlva Schneider</b>. Below the info on his talk:</div><div class=""><br class=""></div><div class="">%%%%%%%%%%%%%</div><div class="">Title: "Equation of State Effects on Core-collapse Supernovae"</div><div style="margin-top: 0px; margin-bottom: 0px;" class=""><br class=""></div><div style="margin-top: 0px; margin-bottom: 0px;" class="">Abstract: </div><div style="margin-top: 0px; margin-bottom: 0px;" class=""><br class=""></div><div style="margin-top: 0px; margin-bottom: 0px;" class="">In this talk I present a method to compute the equation of state (EOS) of dense matter for astrophysical simulations. </div><div style="margin-top: 0px; margin-bottom: 0px;" class="">I discuss how current uncertainties in the parameters that determine the EOS affect the outcome of a core-collapse supernova simulation. </div><div style="margin-top: 0px; margin-bottom: 0px;" class=""><br class=""></div><div style="margin-top: 0px; margin-bottom: 0px;" class="">%%%%%%%%%%%%%</div><div style="margin-top: 0px; margin-bottom: 0px;" class=""><br class=""></div><div style="margin-top: 0px; margin-bottom: 0px;" class="">cheers</div><div style="margin-top: 0px; margin-bottom: 0px;" class=""><br class=""></div><div style="margin-top: 0px; margin-bottom: 0px;" class="">/Francesco</div></body></html>