2002/09/23 by A. V. Kuznetsov, А. В. Кузнецов, Kuznetsov, A. V. +3
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #Quantum, superfluid, helium dynamics #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0209253
10 pages, LATEX, 2 EPS figures, talk presented at the 12th International Seminar ``Quarks-2002'', Valday and Novgorod, Russia, June 1-7, 2002, to appear in the Proceedings (in v.2 the dates of the Seminar are corrected)
openalex publication_date 2002/09/23 · arxiv created 2002/10/02 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The recent studies is reported of the neutrino photoproduction on nuclei, gamma + Ze -> Ze + gamma + nu + anti-nu, in a strong magnetic field. It is shown that the catalyzing influence of the field on the process decreases essentially because of the modification of the photon dispersion properties in a strong magnetic field. Therefore, at any field magnitude, neutrino photoproduction cannot compete with the URCA processes. This conclusion contradicts a recent statement in the literature.