Decrease of gravitational mass due to neutrino emission and shock revival in supernovae

Details Decrease of gravitational mass due to neutrino emission and shock revival in supernovae Decrease of gravitational mass due to neutrino emission and shock revival in supernovae

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...403..706g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 403, no. 2, p. 706, 707.

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Emission Spectra, Gravitational Effects, Neutrinos, Stellar Mass, Supernovae, Computational Astrophysics, Red Shift, Stellar Envelopes, Stellar Evolution, X Ray Spectra

Scientific paper

Neutrino emission from the newly formed neutron star reduces the star's gravitational mass and thus reduces the depth of the gravitational potential well, out of which the mantle and envelope layers have to be pushed. We estimated that this effect can contribute about 10 percent of the energy required for a Type II supernova explosion. It can thus facilitate the shock revival in the delayed-explosion scenario.

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