The Long Term: Six-dimensional Core-collapse Supernova Models
Abstract
The computational difficulty of six-dimensional neutrino radiation hydrodynamics has spawned a variety of approximations, provoking a long history of uncertainty in the core-collapse supernova explosion mechanism. Under the auspices of the Terascale Supernova Initiative, we are honoring the physical complexity of supernovae by meeting the computational challenge head-on, undertaking the development of a new adaptive mesh refinement code for self-gravitating, six-dimensional neutrino radiation magnetohydrodynamics. This code--called {\em GenASiS}, for {\em Gen}eral {\em A}strophysical {\em Si}mulation {\em S}ystem--is designed for modularity and extensibility of the physics. Presently in use or under development are capabilities for Newtonian self-gravity, Newtonian and special relativistic magnetohydrodynamics (with `realistic' equation of state), and special relativistic energy- and angle-dependent neutrino transport--including full treatment of the energy and angle dependence of scattering and pair interactions.
Cite
@article{arxiv.astro-ph/0510704,
title = {The Long Term: Six-dimensional Core-collapse Supernova Models},
author = {Christian Y. Cardall and Alexei O. Razoumov and Eirik Endeve and Anthony Mezzacappa},
journal= {arXiv preprint arXiv:astro-ph/0510704},
year = {2017}
}
Comments
23 pages. Proceedings of Open Issues in Understanding Core Collapse Supernovae, National Institute for Nuclear Theory, University of Washington, 22-24 June 2004, World Scientific, in press