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Core-Collapse Supernovae at the Threshold

Published online by Cambridge University Press:  19 September 2016

H.-Th. Janka ,
R. Buras ,
K. Kifonidis ,
A. Marek  and
M. Rampp
H.-Th. Janka
Affiliation:
Max-Planck-Institut für Astrophysik, Postfach 1317, 85741 Garching, Germany; thj@mpa-garching.mpg.de
R. Buras
Affiliation:
Max-Planck-Institut für Astrophysik, Postfach 1317, 85741 Garching, Germany; thj@mpa-garching.mpg.de
K. Kifonidis
Affiliation:
Max-Planck-Institut für Astrophysik, Postfach 1317, 85741 Garching, Germany; thj@mpa-garching.mpg.de
A. Marek
Affiliation:
Max-Planck-Institut für Astrophysik, Postfach 1317, 85741 Garching, Germany; thj@mpa-garching.mpg.de
M. Rampp
Affiliation:
Max-Planck-Institut für Astrophysik, Postfach 1317, 85741 Garching, Germany; thj@mpa-garching.mpg.de

Summary

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Recent progress in modeling core-collapse supernovae is summarized and set in perspective. Two-dimensional simulations with state-of-the-art treatment of neutrino transport still fail to produce powerful explosions, but evidence is presented that they are very close to a success.

Information

Type
Part IV Supernovae: Models
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 253 - 262
Copyright
Copyright © Springer-Verlag 2005

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