corner
corner

Phys. Rev. D 58, 113004 (1998) [6 pages]

Bremsstrahlung process ντνee+e-γ

Download: PDF (162 kB) Buy this article Export: BibTeX or EndNote (RIS)

H. Schmid and G. Raffelt
Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Föhringer Ring 6, 80805 München, Germany

A. Leike
Ludwig-Maximilians-Universität, Sektion Physik, Theresienstrasse 37, 80333 München, Germany

Received 21 April 1998; published 29 October 1998

The bremsstrahlung process ντνee+e-γ is the dominant photon-producing decay of heavy τ neutrinos with mντ>2me so that this process is instrumental for supernova 1987A constraints on the properties of these particles, notably on their mixing amplitude with νe. 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.

© 1998 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.58.113004
DOI:
10.1103/PhysRevD.58.113004
PACS:
14.60.Pq, 13.35.Hb, 14.60.Lm, 97.60.Bw