Pair production of helicity-flipped neutrinos in supernovae

Bibcode
1989ahoe.work.....P
Perez, Armando; Gandhi, Raj
Referencia bibliográfica

Unknown

Fecha de publicación:
7
1989
Número de autores
2
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Sin árbitro
Supernovas
Corazones estelares

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