Modeling core collapse supernovae in 2 and 3 dimensions with spectral neutrino transport-Reference-Cited by-同舟云学术

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Modeling core collapse supernovae in 2 and 3 dimensions with spectral neutrino transport

Published:2006-09-01 Issue: Volume:46 Page:393-402
ISSN:1742-6588
Container-title:Journal of Physics: Conference Series
language:
Short-container-title:J. Phys.: Conf. Ser.

Author:

Bruenn S W,Dirk C J,Mezzacappa A,Hayes J C,Blondin J M,Hix W R,Messer O E B

Publisher

IOP Publishing

Subject

General Physics and Astronomy

Link

http://stacks.iop.org/1742-6596/46/i=1/a=054/pdf

Reference27 articles.

1. The Piecewise Parabolic Method (PPM) for gas-dynamical simulations

2. Stellar core collapse - Numerical model and infall epoch

3. Computational methods for nucleosynthesis and nuclear energy generation

4. Supernova 1987A Revisited

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1. Physical mechanism of core-collapse supernovae that neutrinos drive;Proceedings of the Japan Academy, Series B;2024-03-11

2. Core-collapse Supernova Simulations with Reduced Nucleosynthesis Networks;The Astrophysical Journal;2023-07-01

3. Nucleosynthesis in Jet-Driven and Jet-Associated Supernovae;Handbook of Nuclear Physics;2023

4. Nucleosynthesis in Jet-Driven and Jet-Associated Supernovae;Handbook of Nuclear Physics;2022-11-13

5. A force explosion condition for spherically symmetric core-collapse supernovae;Monthly Notices of the Royal Astronomical Society;2022-06-30

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