Consistent neutrino masses from cosmology and solar physics

Details Consistent neutrino masses from cosmology and solar physics Consistent neutrino masses from cosmology and solar physics

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990natur.348..617s&link_type=abstract

Nature (ISSN 0028-0836), vol. 348, Dec. 13, 1990, p. 617, 618. Research supported by the Ministero Italiano per la Ricerca Scien

Physics

23

Cosmology, Neutrinos, Particle Mass, Solar Physics, Dark Matter, Galactic Evolution, Quarks, Supernovae

Scientific paper

The solar neutrino problem and cosmological dark matter can both be accounted for by nonzero neutrino masses that are broadly compatible with the so-called 'see-saw' relation, according to which the mass of each neutrino type is proportional to the square of the mass of the associated quark. It is pointed out here that more precise estimates of neutrino masses which have recently been made still conform to the see-saw relation. This result, unless it is a chance agreement, ties together three unproven hypotheses: the see-saw mechanism, the MSW effect, and the decaying neutrino hypothesis.

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