Solar-neutrino oscillations

Details Solar-neutrino oscillations Solar-neutrino oscillations

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..55..122k&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 55, July 1, 1985, p. 122-125. NASA-supported research.

Astronomy and Astrophysics

Astrophysics

25

Electron Scattering, Particle Interactions, Solar Neutrinos, Solar Oscillations, Astrophysics, Particle Mass, Pressure Broadening, Recoilings, Stellar Cores

Scientific paper

The authors develop the theory of oscillations of solar neutrinos as it applies to the electron recoil spectrum in ν-e scattering. The spectral information obtained by such measurements (as opposed to counting total event rates) is crucial for allowing observation of neutrino oscillations for masses down to 5×10-7eV. In this regard, the authors investigate effects of different masses and mixing angles, as well as such subtleties as thermal and pressure broadening, finite solar core size, and variable indices of refraction.

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