Gravitational Waves from Core-Collapse Supernova using CHIMERA: Models and Numerical Methods

Details Gravitational Waves from Core-Collapse Supernova using CHIMERA: Models and Numerical Methods Gravitational Waves from Core-Collapse Supernova using CHIMERA: Models and Numerical Methods

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aps..apra14001m&link_type=abstract

American Physical Society, APS April Meeting 2010, February 13-16, 2010, abstract #A14.001

Physics

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CHIMERA is a multi-dimensional code composed of three tightly coupled physics modules: VH1 used to evolve stellar gas hydrodynamics, MGFLD-TRANS which handles the neutrino transport, and XNET that describes the thermonuclear reactions. These are complemented with a sophisticated equation of state for nuclear matter (Lattimer-Swesty) and a self-gravity solver capable of an approximation to general-relativistic gravity. We will present the latest simulations of core-collapse supernova for different-mass progenitors. These models are evolved for up to one second in all cases, making them some of longest term simulations of their kind. )

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