New interactions in neutrino oscillations with three light flavors

Details New interactions in neutrino oscillations with three light flavors New interactions in neutrino oscillations with three light flavors

1997-06-10

arxiv.org/abs/hep-ph/9706309v3

Phys.Rev.Lett. 80 (1998) 4637-4640

Physics

High Energy Physics

High Energy Physics - Phenomenology

Final version, to appear in Phys. Rev. Letters dated May 25, 1998

Scientific paper

10.1103/PhysRevLett.80.4637

If one assumes solar and LSND neutrino oscillations to explain the corresponding data, then the atmospheric neutrino deficit cannot be accommodated within the Standard Model with three light flavors, unless one ignores the data's zenith-angle dependence. We propose a novel solution to this problem by postulating large anomalous diagonal $\nu_\tau$-quark interactions which affect $\nu_\mu - \nu_\tau$ oscillations traversing the Earth and induce the observed zenith-angle dependence.

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