Neutrino transport and the prompt mechanism for type II supernovae

Details Neutrino transport and the prompt mechanism for type II supernovae Neutrino transport and the prompt mechanism for type II supernovae

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...340..384m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 340, May 1, 1989, p. 384-395.

Astronomy and Astrophysics

Astrophysics

46

Neutrinos, Stellar Interiors, Supernovae, Electron Capture, Electron Scattering, Equations Of State, Heavy Nuclei, Relativity, Shock Wave Propagation, Supernova 1987A

Scientific paper

Consideration is given to the possibility that a soft nuclear equation of state and general relativistic hydrodynamics can produce a shock with sufficient strength to propagate directly through a low-mass iron core during a stellar collapse. It is found that neutrino-electron scattering produces shock failure due to neutrino downscatter during collapse. Neutrino-electron scattering has little effect during shock propagation. It is shown that neutrino-matter energy exchange is important at densities below trapping density.

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