Three-flavor vacuum oscillations of atmospheric and solar neutrinos

Details Three-flavor vacuum oscillations of atmospheric and solar neutrinos Three-flavor vacuum oscillations of atmospheric and solar neutrinos

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvd..49..328a&link_type=abstract

Physical Review D (Particles and Fields), Volume 49, Issue 1, 1 January 1994, pp.328-332

Physics

12

Neutrino Mass And Mixing, Ordinary Neutrinos (Nuw Bosons, Elementary Particle Processes

Scientific paper

Vacuum oscillations of νμ into ντ and either matter-enhanced or ``just-so'' vacuum oscillations of νe into νμ are generally invoked to explain the observed discrepancies in atmospheric and solar neutrino fluxes, respectively. In this paper, regions of the three-neutrino-flavor parameter space, compatible with the existing atmospheric and solar neutrino data (including the new results from GALLEX) within the vacuum oscillation scheme, are identified.

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