JPS Conf. Proc. 14, 020611 (2017) [3 pages]
Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)
Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations
1Department für Physik, Universität Basel, CH-4056 Basel, Switzerland
2Department of Physics, North Carolina State University, Raleigh, NC 29695-8202, U.S.A.
3Institut für Kernphysik, Technische Universität Darmstadt, D-64289 Darmstadt, Germany
Received August 20, 2016

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.

©2017 The Physical Society of Japan

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