Geochemical integrations of the neutrino flux from stellar collapses

Details Geochemical integrations of the neutrino flux from stellar collapses Geochemical integrations of the neutrino flux from stellar collapses

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988natur.333..325h&link_type=abstract

Nature (ISSN 0028-0836), vol. 333, May 26, 1988, p. 325-329.

Physics

14

Galactic Radiation, Geochemistry, Neutrinos, Stellar Evolution, Antimatter, Gravitational Collapse, Solar Neutrinos

Scientific paper

The galactic neutrino flux from stellar collapses may be measurable in geochemical experiments. Absorption cross-sections can be maximized and backgrounds from solar neutrinos and terrestrial antineutrinos minimized by exploiting neutrino capture reactions in which nuclei are excited above the threshold for particle breakup. Only a few practical candidate reactions exist; one of them, 98Mo(νe,e-)97Tc+n, is being studied in a current solar neutrino experiment, and an interesting limit on the galactic stellar collapse rate may soon be obtained. See also 061.267.

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