Neutrino energy loss in stellar interiors. V - Recombination neutrino process

Details Neutrino energy loss in stellar interiors. V - Recombination neutrino process Neutrino energy loss in stellar interiors. V - Recombination neutrino process

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...415..267k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 415, no. 1, p. 267-277.

Statistics

Computation

11

Electron Recombination, Energy Dissipation, Neutrinos, Particle Energy, Stellar Interiors, Computational Astrophysics, Nuclear Fusion, Particle Theory

Scientific paper

The neutrino energy loss rates due to recombination neutrino process are calculated for nonrelative electrons in the framework of the Weinberg-Salam theory. The Coulomb distortion effects for the electrons in the continuum states are accurately taken into account. These effects reduce the neutrino energy loss rates drastically, by more than 1.5 orders of magnitude. Comparison with other neutrino processes is made. It is found that the recombination neutrino process is a dominant neutrino process for relatively large Z-values at relatively low densities and low temperatures. The results of the calculation are expressed by an analytical fitting formula.

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