Detection of solar and cosmic neutrinos by coherent scattering

Details Detection of solar and cosmic neutrinos by coherent scattering Detection of solar and cosmic neutrinos by coherent scattering

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...108....1o&link_type=abstract

Astronomy and Astrophysics, vol. 108, no. 1, Apr. 1982, p. 1-6.

Astronomy and Astrophysics

Astrophysics

9

Coherent Scattering, Cosmic Rays, Neutrinos, Particle Energy, Radiation Detectors, Solar Neutrinos, Electron Scattering, Particle Flux Density, Particle Mass

Scientific paper

The use of coherent scattering for the detection of low energy p-p solar neutrinos and cosmic neutrinos using superconducting electrons is examined. For the abundant p-p solar neutrino flux, such a detector has the advantages compared to nuclear reaction detectors of directionality and sensitivity. The only means presently available for the detection of low energy cosmic neutrinos is coherent scattering. The use of the superconducting detector for detecting the abundant predicted fluxes of massive and massless cosmic neutrinos is discussed.

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