The Bremsstrahlung Process Nu_Tau -> Nu_e E+ E- Gamma

Details The Bremsstrahlung Process Nu_Tau -> Nu_e E+ E- Gamma The Bremsstrahlung Process Nu_Tau -> Nu_e E+ E- Gamma

1998-04-20

arxiv.org/abs/hep-ph/9804334v1

Phys.Rev. D58 (1998) 113004

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, REVTEX, includes 5 eps figs

Scientific paper

10.1103/PhysRevD.58.113004

The bremsstrahlung process Nu_Tau -> Nu_e E+ E- Gamma is the dominant photon-producing decay of heavy Tau neutrinos with m_Nu_Tau > 2 m_e so that this process is instrumental for supernova 1987A constraints on the properties of these particles, notably on their mixing amplitude with Nu_e. We calculate the rate of the bremsstrahlung process as well as the photon spectrum and the angular distribution relative to the spin direction of the parent neutrino. We carefully pay attention to the difference between Dirac and Majorana neutrinos.

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