Neutrino production in stellar matter by photons in a renormalizable scalar-boson-exchange model of weak interactions

Mathematics – Logic

Scientific paper

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Astronomical Models, Neutrinos, Particle Interactions, Particle Production, Stellar Mass Ejection, Annihilation Reactions, Bosons, Energy Dissipation, Stellar Radiation

Scientific paper

A calculation of the rate of energy loss in stellar matter through neutrino production by two-photon annihilation is presented. It uses the scalar-boson-exchange model of Kummer and Segre (1965) for weak interactions. The results show that this mechanism for energy loss unlikely to be significant astrophysically. Comparison with a phenomenological calculation suggests that the mass of the scalar boson may be about 19 GeV.

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