Neutrino energy loss in stellar interiors. III - Pair, photo-, plasma, and bremsstrahlung processes

Details Neutrino energy loss in stellar interiors. III - Pair, photo-, plasma, and bremsstrahlung processes Neutrino energy loss in stellar interiors. III - Pair, photo-, plasma, and bremsstrahlung processes

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339..354i&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 1, 1989, p. 354-364.

Statistics

Computation

158

Computational Astrophysics, Energy Dissipation, Neutrinos, Stellar Interiors, Bremsstrahlung, Dense Plasmas, Pair Production, Stellar Evolution

Scientific paper

Detailed results of the calculation of the neutrino energy-loss rates due to pair, photo-, plasma, and bremsstrahlung processes corresponding to the density-temperature regime 1-10 to the 14th g/cu cm, 10 to the 7th - 10 to the 11th K are presented. The calculation is based on the Weinberg-Salam theory. The present calculation is the most accurate calculation to date covering the widest density-temperature regime. The discrepancies with the previous works are carefully examined. Extensive tables are prepared to show the detailed results of the photo-neutrino energy-loss rate.

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