Radiative Transition of Massless Neutrino in Strong Magnetic Field

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dc.creatorGvozdev, A. A.
dc.creatorMikheev, N. V.
dc.creatorVassilevskaya, L. A.
dc.date1997-09-02
dc.date.accessioned2026-07-07T04:02:21Z
dc.date.available2026-07-07T04:02:21Z
dc.descriptionRadiative 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.
dc.description4 pages, latex. Talk given at the XXXII Rencontres de Moriond on Elecrtoweak interactions and unified theories, Les Arcs, Savoie, France, March 15-22, 1997
dc.identifierhttps://arxiv.org/abs/hep-ph/9709218
dc.identifierhttp://arxiv.org/abs/hep-ph/9709218
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/47193
dc.subjectHigh Energy Physics - Phenomenology
dc.titleRadiative Transition of Massless Neutrino in Strong Magnetic Field
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