Neutrino mass explanations of solar and atmospheric neutrino deficits and hot dark matter

Details Neutrino mass explanations of solar and atmospheric neutrino deficits and hot dark matter Neutrino mass explanations of solar and atmospheric neutrino deficits and hot dark matter

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvd..48.3259c&link_type=abstract

Physical Review D (Particles and Fields), Volume 48, Issue 7, 1 October 1993, pp.3259-3263

Physics

277

Quark And Lepton Masses And Mixing, Dark Matter

Scientific paper

If the solar and atmospheric neutrino deficits and the apparent need for a hot dark matter component all result from neutrino mass, one of three neutrino mass patterns is required. Of these, two appear quite unlikely, leading to a unique solution which points to further experimental tests. We briefly outline possible theoretical models which could generate these three neutrino mass matrices without adjustment of parameters.

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