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arXiv · 1610.05629

Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations

Kevin Ebinger·Sanjana Sinha·Carla Fröhlich·Albino Perego·Matthias Hempel·Marius Eichler·Jordi Casanova·Matthias Liebendörfer·Friedrich-Karl Thielemann
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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.

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Kevin Ebinger, Sanjana Sinha, Carla Fröhlich, Albino Perego, Matthias Hempel, Marius Eichler, Jordi Casanova, Matthias Liebendörfer, Friedrich-Karl Thielemann. 2016-10-12. Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations. https://doi.org/10.7566/jpscp.14.020611

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