Neutrino energy loss in stellar interiors

Details Neutrino energy loss in stellar interiors Neutrino energy loss in stellar interiors

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...296..197m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 296, Sept. 1, 1985, p. 197-203.

Astronomy and Astrophysics

Astrophysics

123

Energy Dissipation, Neutrinos, Pair Production, Stellar Evolution, Stellar Interiors, Stellar Structure, Bremsstrahlung, Integral Equations

Scientific paper

The energy loss rates due to pair, photo-, and plasma neutrino processes are calculated in the framework of the Weinberg-Salam theory for wide ranges of densities and temperatures. Accurate analytic fitting formulae are presented to facilitate the application of the result. It is found that the present calculation gives a neutrino energy loss rate which is substantially lower than that of Beaudet, Petrosian, and Salpeter. The reduction factor α is in the range 0.35 ⪉ α ⪉ 0.88 depending on the neutrino masses, density, and temperature.

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