The isotropic electron antineutrino flux - A clue to the rate of stellar gravitational collapse in the universe

Details The isotropic electron antineutrino flux - A clue to the rate of stellar gravitational collapse in the universe The isotropic electron antineutrino flux - A clue to the rate of stellar gravitational collapse in the universe

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61...51d&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Jan.-Feb. 1984, p. 51, 52) Soviet Astronomy (ISSN 0038-5301), vol. 28, Jan.-Feb. 1984, p. 30

Astronomy and Astrophysics

Astronomy

2

Antineutrinos, Gravitational Collapse, Stellar Evolution, Cosmic Ray Showers, Cosmology, Electron Flux Density, Isotropy

Scientific paper

It is pointed out to the possibility of obtaining information on the
intensity of the processes of stellar evolution during the last (10 -
12)×109 years by the registration of an isotropic flux
of electron antineutrinos born in the gravitational collapses of massive
stars.

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