Study of the sun's neutrino brightness curve with the help of a chlorine-argon neutrino detector

Details Study of the sun's neutrino brightness curve with the help of a chlorine-argon neutrino detector Study of the sun's neutrino brightness curve with the help of a chlorine-argon neutrino detector

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982zhpmr..35..491g&link_type=abstract

(ZHETF Pis'ma v Redaktsiiu, vol. 35, June 5, 1982, p. 491-494.) JETP Letters, vol. 35, June 5, 1982, p. 608-611. Translation.

Physics

Brightness Distribution, Particle Flux Density, Radiation Detectors, Solar Neutrinos, Argon Isotopes, Chlorine, Cosmic Rays, Solar Activity Effects

Scientific paper

It is shown that the rate of formation of Ar-37 in the Brookhaven solar-neutrino detector oscillates with periods 20 + or - 1, 25.5 + or - 1.5 months, and approximately 11 years and with a modulation depth greater than approximately 0.3 with a confidence level not lower than 99.5%. These oscillations are interpreted as resulting from the modulation of the neutrino flux by gravitational oscillations at the center of the sun. Further experiments for studying the sun's neutrino brightness curve with the help of the chlorine-argon neutrino detector are discussed.

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