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arXiv · 1804.03182

PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties

Kevin Ebinger·Sanjana Curtis·Carla Fröhlich·Matthias Hempel·Albino Perego·Matthias Liebendörfer·Friedrich-Karl Thielemann
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Abstract

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$_\odot$.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.

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Kevin Ebinger, Sanjana Curtis, Carla Fröhlich, Matthias Hempel, Albino Perego, Matthias Liebendörfer, Friedrich-Karl Thielemann. 2018-04-09. PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties. https://doi.org/10.3847/1538-4357/aae7c9

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