The core-collapse supernova explosion mechanism

Bernhard Müller

doi:10.1017/S1743921317002575

The core-collapse supernova explosion mechanism

Bernhard Müller

School of Physics and Astronomy

Research output: Contribution to journal › Article › Research › peer-review

6 Citations (Scopus)

Abstract

The explosion mechanism of core-collapse supernovae is a long-standing problem in stellar astrophysics. We briefly outline the main contenders for a solution and review recent efforts to model core-collapse supernova explosions by means of multi-dimensional simulations. Focusing on the neutrino-driven mechanism, we summarize currents efforts to predict supernova explosion and remnant properties.

Original language	English
Pages (from-to)	17-24
Number of pages	8
Journal	Proceedings of the International Astronomical Union
Volume	12
Issue number	S329
DOIs	https://doi.org/10.1017/S1743921317002575
Publication status	Published - 1 Nov 2016

Keywords

Convection
Hydrodynamics
Instabilities
Methods: Numerical
Neutrinos
Stars: Evolution
Stars: Interiors
Supernovae: General
Turbulence

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10.1017/S1743921317002575

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Cite this

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AB - The explosion mechanism of core-collapse supernovae is a long-standing problem in stellar astrophysics. We briefly outline the main contenders for a solution and review recent efforts to model core-collapse supernova explosions by means of multi-dimensional simulations. Focusing on the neutrino-driven mechanism, we summarize currents efforts to predict supernova explosion and remnant properties.

KW - Convection

KW - Hydrodynamics

KW - Instabilities

KW - Methods: Numerical

KW - Neutrinos

KW - Stars: Evolution

KW - Stars: Interiors

KW - Supernovae: General

KW - Turbulence

UR - https://www.scopus.com/pages/publications/85046974866

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DO - 10.1017/S1743921317002575

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VL - 12

SP - 17

EP - 24

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

IS - S329

ER -

The core-collapse supernova explosion mechanism

Abstract

Keywords

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