Litcius/Paper detail

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>M</mml:mi><mml:mn>1</mml:mn></mml:math> neutrino transport within the numerical-relativistic code BAM with application to low mass binary neutron star mergers

Federico Schianchi, Henrique Gieg, Vsevolod Nedora, Anna Neuweiler, Maximiliano Ujevic, Mattia Bulla, Tim Dietrich

2024Physical review. D/Physical review. D.20 citationsDOIOpen Access PDF

Abstract

A crucial ingredient in accurate simulations of neutron star-neutron star and neutron star-black hole mergers is the inclusion of neutrino transport and its effects on the physics and astrophysics of these phenomena. The authors implement a neutrino radiative transport scheme in their general relativistic hydrodynamics code, BAM, do more accurately simulate these mergers and map the effects of neutrino transport on the ejecta from neutron star-neutron star mergers.

Topics & Concepts

NeutrinoPhysicsParticle physicsPulsars and Gravitational Waves ResearchGamma-ray bursts and supernovaeHigh-Energy Particle Collisions Research
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>M</mml:mi><mml:mn>1</mml:mn></mml:math> neutrino transport within the numerical-relativistic code BAM with application to low mass binary neutron star mergers | Litcius