Radiative neutrino transition $\nu \to \nu \gamma$ in strongly magnetized plasma
High Energy Physics - Phenomenology
2009-10-31 v3
Abstract
The influence of strongly magnetized electron-positron plasma on the radiative neutrino transition is investigated. The probability and mean losses of the neutrino energy and momentum are calculated taking account of the photon dispersion and large radiative corrections near the resonance. It is shown that the combined effect of plasma and strong magnetic field decreases the probability and mean values of the neutrino energy and momentum loss in comparison with these values obtained in pure magnetic field.
Keywords
Cite
@article{arxiv.hep-ph/9907345,
title = {Radiative neutrino transition $\nu \to \nu \gamma$ in strongly magnetized plasma},
author = {M. V. Chistyakov and N. V. Mikheev},
journal= {arXiv preprint arXiv:hep-ph/9907345},
year = {2009}
}
Comments
12 pages, 3 figure, LaTeX2e, uses epsf.sty, typos fixed, accepted to Physics Letters B