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BEGIN:VEVENT
SUMMARY:Binary Neutron Star Merger Simulations with Microphysical Equation
  of State using Spritz
DTSTART:20260409T143000Z
DTEND:20260409T160000Z
DTSTAMP:20260725T103253Z
UID:26843081-a775-4af5-8839-c8df579d9477
SEQUENCE:2
CREATED:20260409T090424Z
DESCRIPTION:I present results from new simulations performed with Spritz\,
  a general-relativistic magnetohydrodynamics (GRMHD) code built on the Ein
 stein Toolkit infrastructure and developed for highprecision studies of bi
 nary 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 unequ
 al-mass systems\, inspired by the GW170817 event. Our analysis focuses on 
 the gravitational-wave (GW) emission\, as well as on the potential formati
 on of relativistic jets and neutron-rich outflows.
LAST-MODIFIED:20260409T090448Z
LOCATION:DF Seminar Room (2-8.3)\, 2nd floor of Physics Building
URL:http://df.vps.tecnico.ulisboa.pt/pt/eventos/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 f
 rom new simulations performed with Spritz\, a general-relativistic magneto
 hydrodynamics (GRMHD) code built on the Einstein Toolkit infrastructure an
 d developed for highprecision studies of binary neutron star (BNS) mergers
  with realistic microphysical equations of state (EOS).<br/><br/> These si
 mulations build upon recent developments in the code\, which enable the ev
 olution of magnetized systems with tabulated EOS. We model magnetized bina
 ries employing tabulated EOS for equal-mass and unequal-mass systems\, ins
 pired by the GW170817 event. Our analysis focuses on the gravitational-wav
 e (GW) emission\, as well as on the potential formation of relativistic je
 ts and neutron-rich outflows.</p>
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