Does the Davis neutrino experiment show a variable Ar-37 production rate?

Details Does the Davis neutrino experiment show a variable Ar-37 production rate? Does the Davis neutrino experiment show a variable Ar-37 production rate?

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..154g&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Feb. 1984, p. 154-160) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Jan.-Feb

Astronomy and Astrophysics

Astronomy

2

Argon Isotopes, Frequency Distribution, Particle Flux Density, Particle Production, Solar Neutrinos, Monte Carlo Method, Poisson Density Functions, Solar Flux, Statistical Analysis

Scientific paper

The data from Davis's (1968, 1976) experiment to measure the solar neutrino flux are analyzed by the successive-difference, Kolmogorov-Smirnov, and chi-squared methods. A comparison is also made against Monte Carlo simulations by Cleveland. Davis's data do not contravene the hypothesis that the Ar-37 production rate remains constant, except the two points would exceed the likely statistical fluctuations, provided the background events have a Poisson distribution and statistical analysis itself does not distort the distribution function. The fulfillment of these two conditions must be tested.

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