E6 leptoquarks and the solar neutrino problem

Details E6 leptoquarks and the solar neutrino problem E6 leptoquarks and the solar neutrino problem

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991stin...9211956r&link_type=abstract

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Physics

Flavor (Particle Physics), Leptons, Oscillations, Quarks, Solar Neutrinos, Sun, Nucleons, Vacuum

Scientific paper

The possibility that non-conventional neutrino oscillations take place in the superstring inspired E6 models is considered. In this context, the influence of leptoquark mediated interactions of the neutrinos with nucleons in the resonant flavor conversion is discussed. It is shown that this effect can be significant for ve - vtau oscillations if these neutrinos have masses required in the ordinary Mikheyev-Smirnov-Wolfenstein (MSW) effect, and may lead to a solution of the solar neutrino problem even in the absence of vacuum mixings. On the other hand, this model cannot lead to a resonant behavior in the sun if the neutrinos are massless.

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