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Phys. Rev. D 59, 097702 (1999) [4 pages]

Minimal seesaw model for atmospheric and solar neutrino oscillations

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Ernest Ma
Department of Physics, University of California, Riverside, California 92521

D. P. Roy
Department of Physics, University of Durham, Durham, DH1 3LE, United Kingdom
Tata Institute of Fundamental Research, Homi Bhabha Road, Bombay 400005, India

Received 1 December 1998; published 6 April 1999

We present a minimal seesaw model based on an extension of the standard model (SM) which includes an additional U(1), with gauge charge B-3/2(Lμ+Lτ). The requirement of anomaly cancellation implies the existence of two right-handed singlet neutrinos, carrying this gauge charge, which have normal Dirac couplings to νμ and ντ but suppressed ones to νe. Assuming the U(1) symmetry breaking scale to be 1012-1016 GeV, this model can naturally account for the large (small) mixing solutions to the atmospheric (solar) neutrino oscillations.

© 1999 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.59.097702
DOI:
10.1103/PhysRevD.59.097702
PACS:
12.60.Cn, 12.15.Ff, 14.60.Pq