Possible Candidates for SUSY SO(10) Model with an Intermediate Scale
Abstract
We study the possibility of an intermediate scale existing in supersymmetric SO(10) grand unified theories: The intermediate scale is demanded to be around 1012 GeV so that neutrinos can obtain masses suitable for explaining the experimental data on the deficit of solar neutrino with Mikheev-Smirnov-Wolfenstein solution and the existence of hot dark matter. We show that any Pati-Salam type intermediate symmetries are excluded by requiring reasonable conditions and only SU(2)L× SU(2)R × SU(3)C× U(1)B-L is likely to be realized as an intermediate symmetry.
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