Neutrino-nucleus interactions in core-collapse supernovae

Details Neutrino-nucleus interactions in core-collapse supernovae Neutrino-nucleus interactions in core-collapse supernovae

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...376..678b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 376, Aug. 1, 1991, p. 678-700. Research supported by DOE.

Statistics

Computation

68

Neutrinos, Nuclear Interactions, Stellar Cores, Supernovae, Computational Astrophysics, Gravitational Collapse, Nuclear Astrophysics, Shock Waves

Scientific paper

Differential cross sections for charged-current and inelastic neutral-current neutrino-nucleus interactions have been computed. These are incorporated into a radiation hydrodynamics code, and a number of models have been evolved with the aim of determining the role of these rates in the evolution of the collapsing core and in the supernova mechanism. In particular, attention is given to the effect of these rates on the infall epoch, the prompt shock propagation phase, and the delayed-shock phase in the evolution of the core.

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