E6 leptoquarks and the solar-neutrino problem

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

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvd..44.3971r&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 44, Issue 12, 15 December 1991, pp.3971-3973

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The possibility that nonconventional 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 νe-ντ oscillations if these neutrinos have the masses required in the ordinary Mikheyev-Smirnov-Wolfenstein 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 resonant behavior in the Sun if the neutrinos are massless.

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