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arXiv · hep-ph/9702285

Resonance neutrino bremsstrahlung $ν\to νγ$ in a strong magnetic field

A. A. Gvozdev·N. V. Mikheev·L. A. Vassilevskaya
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Abstract

High energy neutrino bremsstrahlung $ν\to ν+ γ$ in a strong magnetic field ($B \gg B_s$) is studied in the framework of the Standard Model (SM). A resonance probability and a four-vector of the neutrino energy and momentum loss are presented. A manifestation of the neutrino bremsstrahlung in astrophysical cataclysm of type of a supernova explosion or a merger of neutron stars, such as an possible origin of cosmological $γ$-burst is discussed.

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A. A. Gvozdev, N. V. Mikheev, L. A. Vassilevskaya. 1997-02-07. Resonance neutrino bremsstrahlung $ν\to νγ$ in a strong magnetic field. https://doi.org/10.1016/s0370-2693(97)01014-9

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