Radiative neutrino decays in very strong magnetic fields

Details Radiative neutrino decays in very strong magnetic fields Radiative neutrino decays in very strong magnetic fields

1996-10-22

arxiv.org/abs/hep-ph/9610439v1

Phys.Lett. B390 (1997) 263-267

Physics

High Energy Physics

High Energy Physics - Phenomenology

Latex2e with elsart-style, 10 pages with 2 ps-figures. To appear in Physics Letters B

Scientific paper

10.1016/S0370-2693(96)01406-2

The radiative decay $\nu_H \to \nu_L + \gamma$ of massive neutrinos is analyzed in the framework of the standard model with lepton mixing for very strong magnetic fields $B\gg B_{cr} = m_e^2/e \sim 4.14 \times 10^{13}$G. The analysis is based on the approximate decay amplitude obtained by Gvozdev et al. Numerical results as well as analytical approximations for the decay rate are obtained for energies of the initial neutrino below and {\em above} the electron-positron pair creation threshold $2m_e$.

Affiliated with

Also associated with

No associations

Rating

Radiative neutrino decays in very strong magnetic fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radiative neutrino decays in very strong magnetic fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiative neutrino decays in very strong magnetic fields will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-700853