Solar neutrino problem in seesaw model.

Details Solar neutrino problem in seesaw model. Solar neutrino problem in seesaw model.

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cotph..30..113f&link_type=abstract

Commun. Theor. Phys., Vol. 30, No. 1, p. 113 - 116

Physics

Solar Neutrinos, Neutrinos: Dark Matter

Scientific paper

A specific texture for the Dirac and Majorana mass matrices in the seesaw model leading to a pair of almost degenerate neutrinos is discussed. This texture can be obtained by imposing a global U(1) symmetry. This model could solve the solar neutrino problem through the MSW mechanism and offer the hot component of the dark matter of the Universe which requires Σm(νi) = 7 eV.

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