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BEGIN:VEVENT
SUMMARY:Binary Neutron Star Merger Simulations with Microphysical Equation
  of State using Spritz
DTSTART:20260409T143000Z
DTEND:20260409T160000Z
DTSTAMP:20260730T124520Z
UID:26843081-a775-4af5-8839-c8df579d9477
SEQUENCE:1
CREATED:20260409T090414Z
DESCRIPTION: I present results from new simulations performed with Spritz\
 , a general-relativistic magnetohydrodynamics (GRMHD) code built on the Ei
 nstein Toolkit infrastructure and developed for highprecision studies of b
 inary neutron star (BNS) mergers with realistic microphysical equations of
  state (EOS). These simulations build upon recent developments in the code
 \, which enable the evolution of magnetized systems with tabulated EOS. We
  model magnetized binaries employing tabulated EOS for equal-mass and uneq
 ual-mass systems\, inspired by the GW170817 event. Our analysis focuses on
  the gravitational-wave (GW) emission\, as well as on the potential format
 ion of relativistic jets and neutron-rich outflows.  
LAST-MODIFIED:20260409T090414Z
LOCATION:DF Seminar Room (2-8.3)\, 2nd floor of Physics Building
URL:http://df.vps.tecnico.ulisboa.pt/en/events/binary-neutron-star-merger-
 simulations-with-microphysical-equation-of-state-using-spritz/
X-ALT-DESC;FMTTYPE=text/html:<p data-block-key="ut4n8"> I present results 
 from new simulations performed with Spritz\, a general-relativistic magnet
 ohydrodynamics (GRMHD) code built on the Einstein Toolkit infrastructure a
 nd developed for highprecision studies of binary neutron star (BNS) merger
 s with realistic microphysical equations of state (EOS). <br/><br/>These s
 imulations build upon recent developments in the code\, which enable the e
 volution of magnetized systems with tabulated EOS. We model magnetized bin
 aries employing tabulated EOS for equal-mass and unequal-mass systems\, in
 spired by the GW170817 event. Our analysis focuses on the gravitational-wa
 ve (GW) emission\, as well as on the potential formation of relativistic j
 ets and neutron-rich outflows.  </p>
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