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Models of Supernova Explosions: Where Do We Stand?

Published online by Cambridge University Press:  19 September 2016

Wolfgang Hillebrandt
Wolfgang Hillebrandt*
Affiliation:
Max-Planck-Institut für Astrophysik, 85748 Garching, Germany;wfh@mpa-garching.mpg.de

Summary

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The present status of our understanding of core-collapse and of thermonuclear supernovae is reviewed. It will be argued that the failure of numerical simulations of the collapse of massive stars to produce explosions is probably caused by our incomplete knowledge of the (micro-) physics involved. In contrast, for thermonuclear (type Ia) supernovae the basic physics seems to be well under control and, therefore, it is not surprising that model predictions and observations are in good agreement.

Type
Part IV Supernovae: Models
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 241 - 251
Copyright
Copyright © Springer-Verlag 2005

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