We investigate the SO(10) grand unified model with generation flipping. The model contains one extra matter multiplet psi(10) and it mixes with the usual matter multiplets psi(i)(16) when SO(10) is broken down to SU(5). We find the parameter region of the model in which the observed quark masses and mixings are well reproduced. The resulting parameter region is consistent with the observation that only psi(i)(16) have a source of hierarchies and indicates that the mixing between second and third generations tends to be large in the lepton sector, which is consistent with the observed maximal mixing of the atmospheric neutrino oscillation. We also show that the model can accommodate MSW and vacuum oscillation solutions to the solar neutrino deficit depending on the form of the Majorana mass matrix for the right-handed neutrinos.
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Texas A&M Univ, Dept Phys, College Stn, TX 77843 USATexas A&M Univ, Dept Phys, College Stn, TX 77843 USA
Dutta, Bhaskar
Mimura, Yukihiro
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Univ Maryland, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USA
Univ Maryland, Dept Phys, College Pk, MD 20742 USATexas A&M Univ, Dept Phys, College Stn, TX 77843 USA
Mimura, Yukihiro
Mohapatra, R. N.
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Univ Maryland, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USA
Univ Maryland, Dept Phys, College Pk, MD 20742 USATexas A&M Univ, Dept Phys, College Stn, TX 77843 USA
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Osaka Inst Technol, Jr Coll, Dept Gen Educ, Asahi Ku, Osaka 5358585, JapanOsaka Inst Technol, Jr Coll, Dept Gen Educ, Asahi Ku, Osaka 5358585, Japan
Nishiura, H
Matsuda, K
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机构:Osaka Inst Technol, Jr Coll, Dept Gen Educ, Asahi Ku, Osaka 5358585, Japan
Matsuda, K
Fukuyama, T
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机构:Osaka Inst Technol, Jr Coll, Dept Gen Educ, Asahi Ku, Osaka 5358585, Japan