Neutrino annihilation in Type II supernovae

Details Neutrino annihilation in Type II supernovae Neutrino annihilation in Type II supernovae

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...314l...7g&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 314, March 1, 1987, p. L7-L10. Research supported b

Astronomy and Astrophysics

Astrophysics

156

Annihilation Reactions, Neutrinos, Radiative Transfer, Supernovae, Electrons, Neutron Stars, Positrons, Stellar Envelopes, Stellar Mass Ejection

Scientific paper

Neutrino-antineutrino annihilation into electrons and positrons can deposit more than 10 to the 51st ergs above the neutrino-sphere of a type II supernova. All species of neutrino contribute roughly equally to the deposited energy. This process, which appears not to have been included in numerical calculations of supernova explosions, may help to drive off the stellar mantle.

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