Radiative Transition of Massless Neutrino in Strong Magnetic Field
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Radiative transition of massless neutrino $ν_l \to ν_l + γ$ ($l = e, μ, τ$) 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.
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
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