Resonance neutrino bremsstrahlung $\nu \to \nu \gamma$ in a strong magnetic field

Abstract

High energy neutrino bremsstrahlung $\nu \to \nu +\gamma$ 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 $\gamma$-burst is discussed.

4 pages, revtex

References in corpus (2)

• Asymmetric neutrino emision and formation of rapidly moving pulsars
• The neutrino energy and momentum loss through the process $\nu \to \nu e^{-}{e}^{+}$ in a strong magnetic field

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• Elementary Particle Interactions In A Background Magnetic Field
• Radiative decay of keV-mass sterile neutrinos in a strongly magnetized plasma
• $a\to e^{+}{e}^{-}$ decay in a model with induced coupling to leptons