Supernova Modeling: Progress and Challenges
Author:
Publisher
Elsevier BV
Subject
Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics
Reference22 articles.
1. Revival of a stalled supernova shock by neutrino heating;Bethe;Astrophys. J.,1985
2. Stability of standing accretion shocks, with an eye toward core-collapse supernovae;Blondin;Astrophys. J.,2003
3. Pulsar spins from an instability in the accretion shock of supernovae;Blondin;Nature,2007
4. Generation of magnetic fields by the stationary accretion shock instability;Endeve;Astrophys. J.,2010
5. Protoneutron star evolution and the neutrino-driven wind in general relativistic neutrino radiation hydrodynamics simulations;Fischer;Astron. Astrophys.,2010
Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Neutron Structure Properties of Titanium in a Supernova;Physics of Atomic Nuclei;2021-11
2. Neutron–proton interaction, bubble structure and neutron skin properties of Co in a Supernova;Indian Journal of Physics;2021-03-01
3. Neutrino quantum kinetics;Physical Review D;2014-05-07
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