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arXiv Open Access 2016

Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations

Kevin Ebinger Sanjana Sinha Carla Fröhlich Albino Perego Matthias Hempel +4 lainnya
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Abstrak

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.

Topik & Kata Kunci

astro-ph.HE astro-ph.SR

Penulis (9)

K

Kevin Ebinger

S

Sanjana Sinha

C

Carla Fröhlich

A

Albino Perego

M

Matthias Hempel

M

Marius Eichler

J

Jordi Casanova

M

Matthias Liebendörfer

F

Friedrich-Karl Thielemann

Format Sitasi

APA MLA BibTeX
Ebinger, K., Sinha, S., Fröhlich, C., Perego, A., Hempel, M., Eichler, M. et al. (2016). Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations. https://arxiv.org/abs/1610.05629

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Informasi Jurnal
Tahun Terbit
2016
Bahasa
en
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arXiv
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Open Access ✓