Time dependence of the Brookhaven solar-neutrino counting rate and the neutrino-oscillation hypothesis

Details Time dependence of the Brookhaven solar-neutrino counting rate and the neutrino-oscillation hypothesis Time dependence of the Brookhaven solar-neutrino counting rate and the neutrino-oscillation hypothesis

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aipc...52..129e&link_type=abstract

AIP Conference Proceedings, Volume 52, pp. 129-138 (1979).

Computer Science

1

Radiation Detectors

Scientific paper

Pomeranchuk has suggested that one might directly observe neutrino oscillations in a solar-neutrino experiment if the oscillation wavelength were comparable to the annual earth-sun distance variation from perihelion to aphelion, 5×106 km. We find that data from the Brookhaven solar-neutrino experiment can be interpreted to marginally favor the neutrino-oscillation hypothesis at the 2-standard-deviation level. If the effect is not a statistical fluctuation, the estimated value for Δm2= mν12-mν1 2∠4×10-10 eV2 is such that terrestrial tests would seem to be unfeasible.

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