Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations
High Energy Astrophysical Phenomena
2017-03-29 v1 Solar and Stellar Astrophysics
Abstract
We report on a method, PUSH, for triggering core-collapse supernova (CCSN) explosions of massive stars in spherical symmetry. This method provides a framework to study many important aspects of core collapse supernovae: the effects of the shock passage through the star, explosive supernova nucleosynthesis and the progenitor-remnant connection. Here we give an overview of the method, compare the results to multi-dimensional simulations and investigate the effects of the progenitor and the equation of state on black hole formation.
Keywords
Cite
@article{arxiv.1610.05629,
title = {Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations},
author = {Kevin Ebinger and Sanjana Sinha and Carla Fröhlich and Albino Perego and Matthias Hempel and Marius Eichler and Jordi Casanova and Matthias Liebendörfer and Friedrich-Karl Thielemann},
journal= {arXiv preprint arXiv:1610.05629},
year = {2017}
}
Comments
Proceedings for Nuclei in the Cosmos XIV, Niigata, Japan (2016)