Radiative Transition of Massless Neutrino in Strong Magnetic Field

1997/09/02 by A. A. Gvozdev, Gvozdev, A. A., N. V. Mikheev +3
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #hep-ph

paper · pdf · doi:10.48550/arxiv.hep-ph/9709218

4 pages, latex. Talk given at the XXXII Rencontres de Moriond on Elecrtoweak interactions and unified theories, Les Arcs, Savoie, France, March 15-22, 1997

arxiv created 1997/09/02 · arxiv updated 2009/11/30

Abstract

Radiative transition of massless neutrino ν_l → ν_l + γ (l = e, μ, τ) in a strong magnetic field is investigated in the framework of the Standard Model. The process probability and the mean values of the neutrino energy and momentum loss are presented. Possible astrophysical manifestation of the process considered is analysed.

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