In a previously presented proof-of-principle study we established a parametrized spherically symmetric explosion method (PUSH) that can reproduce many features of core-collapse supernovae. The present paper goes beyond a specific application that is able to reproduce observational properties of SN1987A and performs a systematic study of the explosion properties for an extensive set of non-rotating, solar metallicity stellar progenitor models in the mass range from 10.8 to 120 M⊙.This includes the transition from neutron stars to black holes as the final result of the collapse of massive stars, and the relation of the latter to supernovae and faint/failed supernovae. The present paper provides the basis for extended nucleosynthesis predictions in a forthcoming paper to be employed in galactic evolution models.
@article{arxiv.1804.03182,
title = {PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties},
author = {Kevin Ebinger and Sanjana Curtis and Carla Fröhlich and Matthias Hempel and Albino Perego and Matthias Liebendörfer and Friedrich-Karl Thielemann},
journal= {arXiv preprint arXiv:1804.03182},
year = {2020}
}