General Relativistic Simulations of Stellar Core Collapse and Postbounce Evolution with Boltzmann Neutrino Transport

Details General Relativistic Simulations of Stellar Core Collapse and Postbounce Evolution with Boltzmann Neutrino Transport General Relativistic Simulations of Stellar Core Collapse and Postbounce Evolution with Boltzmann Neutrino Transport

Feb 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001stin...0206126l&link_type=abstract

Technical Report, DE2001-776209; P01-110142

Physics

Nuclear Physics

Boltzmann Transport Equation, Stellar Mass, Neutrinos, Astrophysics, Gravitational Collapse, Stellar Evolution, Relativistic Theory, Hydrodynamics, Nuclear Physics, Simulation

Scientific paper

We present self-consistent general relativistic simulations of stellar core collapse, bounce, and postbounce evolution for 13, 15, and 20 solar mass progenitors in spherical symmetry. Our simulations implement three-flavor Boltzmann neutrino transport and standard nuclear physics. The results are compared to our corresponding simulations with Newtonian hydrodynamics and O(v/c) Boltzmann transport.

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