Electron-electron neutrino bremsstrahlung. - I

descriptionPublicationkeyboard_double_arrow_right Article 01 Sep 1969 English Publisher:Springer Science and Business Media LLCJournal:Il Nuovo Cimento A, volume 63, pages 354-366 (issn: 0369-3546, eissn: 1826-9869,

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Authors: P. Cazzola; A. Saggion;

doi: 10.1007/bf02963175 , 10.1007/bf02963176

Electron-electron neutrino bremsstrahlung. - I

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Abstract

We compute the transition probability per unit time and volume relative to processes of the general type a1 + a2 → a3 + a4 + v + v, where a1, a3 are charged baryons or leptons and a2, a4 are leptons, in view of estimating the neutrino energy loss rate in stars due to these processes. A general expression is given for the neutrino energy loss rate in the case of a nondegenerate gas of fermions.

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