Resonance neutrino bremsstrahlung nu->nu gamma in a strong magnetic field

被引：19

作者：

Gvozdev, AA ^{[1
]}

Mikheev, NV ^{[1
]}

Vassilevskaya, LA ^{[1
]}

机构：

[1] MOSCOW MV LOMONOSOV STATE UNIV,MOSCOW 117234,RUSSIA

来源：

PHYSICS LETTERS B | 1997年 / 410卷 / 2-4期

关键词：

D O I：

10.1016/S0370-2693(97)01014-9

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

High energy neutrino bremsstrahlung nu-->nu+gamma in a strong magnetic field (B much greater than 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 possible manifestation of the neutrino bremsstrahlung in astrophysical cataclysm of type of a supernova explosion or a mercer of neutron stars, as an origin of cosmological gamma-burst is briefly discussed. (C) 1997 Elsevier Science B.V.

引用

页码：211 / 215

页数：5

共 17 条

[1] PHOTON SPLITTING AND PHOTON DISPERSION IN A STRONG MAGNETIC FIELD [J].