Cosmic Neutrino Oscillations

Details Cosmic Neutrino Oscillations Cosmic Neutrino Oscillations

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.373b&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

The evidences for neutrino oscillations are found in atmospheric and solar neutrinos. The strongest evidence for atmospheric neutrino oscillations is given by zenith-angular dependence of muon neutrino flux. In case of solar neutrinos the evidence is weaker. All five solar-neutrino experiments show the deficit of the flux by a factor 2-3 as compared with the Standard Solar Model prediction. The latter is strongly confirmed by helioseismic measurements. Thus, solar neutrino measurements have a status of disappearance oscillation experiment. The atmospheric and solar neutrinos will be reviewed in the light of recent SuperKamiokande data. The consequences for other astrophysical phenomena will be discussed.

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