Unstable neutrinos from gravitational stellar collapse and Cygnus X-3

Details Unstable neutrinos from gravitational stellar collapse and Cygnus X-3 Unstable neutrinos from gravitational stellar collapse and Cygnus X-3

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..55.2645f&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 55, Dec. 9, 1985, p. 2645-2648.

Astronomy and Astrophysics

Astrophysics

16

Astrophysics, Gravitational Collapse, Neutrinos, Particle Mass, X Ray Binaries, Broken Symmetry, Constraints, Flux Quantization, Stellar Evolution, Supernovae

Scientific paper

Constraints are surveyed for massive neutrinos which decay without emitting radiation. It is pointed out that the delayed neutrino flux signal at the time of a type-II supernova and high-energy neutrinos from Cygnus X-3 will give information on the scale parameter that causes neutrino decays far beyond the reach of laboratory experiments. The possibility is also shown that for a particular parameter value the decaying neutrinos from a supernova may increase the background events in underground detectors.

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