Comparison of LMA and LOW Solar Solution Predictions in an SO(10) GUT Model

Details Comparison of LMA and LOW Solar Solution Predictions in an SO(10) GUT Model Comparison of LMA and LOW Solar Solution Predictions in an SO(10) GUT Model

2001-12-12

arxiv.org/abs/hep-ph/0112171v2

Phys.Lett. B532 (2002) 311-317

Physics

High Energy Physics

High Energy Physics - Phenomenology

Title, abstract and emphasis changed, references added

Scientific paper

10.1016/S0370-2693(02)01575-7

Within the framework of an SO(10) GUT model that can accommodate both the LMA and LOW solar neutrino mixing solutions by appropriate choice of the right-handed Majorana matrix elements, we present explicit predictions for the neutrino oscillation parameters \Delta m^2_{21}, \sin^2 2\theta_{12}, \sin^2 2\theta_{23}, \sin^2 2\theta_{13}, and \delta_{CP}. Given the observed near maximality of the atmospheric mixing, the model favors the LMA solution and predicts that \delta_{CP} is small. The suitability of Neutrino Superbeams and Neutrino Factories for precision tests of the two model versions is discussed.

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