Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations
arXiv:1610.05629 · doi:10.7566/JPSCP.14.020611
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.
Proceedings for Nuclei in the Cosmos XIV, Niigata, Japan (2016)
References in corpus (8)
- Core-collapse supernova equations of state based on neutron star observations
- Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
- Statistical Model for a Complete Supernova Equation of State
- Protoneutron star evolution and the neutrino driven wind in general relativistic neutrino radiation hydrodynamics simulations
- The isotropic diffusion source approximation for supernova neutrino transport
- Symmetry energy impact in simulations of core-collapse supernovae
- Pushing 1D CCSNe to explosions: model and SN 1987A
- Two-Dimensional Core-Collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport