Reaction cross section for solar flare neutrinos with Cl-37 and O-16 targets

Details Reaction cross section for solar flare neutrinos with Cl-37 and O-16 targets Reaction cross section for solar flare neutrinos with Cl-37 and O-16 targets

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...337l..59f&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 337, Feb. 1, 1989, p. L59-L63.

Astronomy and Astrophysics

Astrophysics

7

Absorption Cross Sections, Chlorine, Oxygen, Solar Flares, Solar Neutrinos, Cerenkov Counters, Particle Acceleration, Particle Flux Density, Solar Activity

Scientific paper

Neutrino reaction cross sections are calculated for Cl-37 (electron neutrino, electron) Ar-37 and electron neutrino + O-16 yields electron + anything for the neutrino energy range 50-200 MeV. If the excess neutrino captures observed in the Davis experiment, which seem to correspond to the period during which large solar flares were recorded, are ascribed to the solar-flare neutrinos, 5000 (300) recoil electron events are expected in a 1000-ton water Cerenkov detector, if neutrino energy is 100 (50) MeV. Such detectors have a sensitivity to monitor the solar-flare neutrino event to the level of the maximum theoretical estimate for the flare neutrino flux.

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