Pair production of helicity-flipped neutrinos in supernovae

Details Pair production of helicity-flipped neutrinos in supernovae Pair production of helicity-flipped neutrinos in supernovae

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ahoe.work.....p&link_type=abstract

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Physics

Emissivity, Energy Dissipation, Neutrinos, Pair Production, Supernovae, Stellar Cores, Stellar Mass, Temperature Dependence, Thermal Emission

Scientific paper

The emissivity was calculated for the pair production of helicity-flipped neutrinos, in a way that can be used in supernova calculations. Also presented are simple estimates which show that such process can act as an efficient energy-loss mechanism in the shocked supernova core, and this fact is used to extract neutrino mass limits from SN 1987A neutrino observations.

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