Origin of quark-lepton flavor in SO(10) with type II seesaw mechanism
被引:34
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作者:
Dutta, Bhaskar
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机构:
Texas A&M Univ, Dept Phys, College Stn, TX 77843 USATexas A&M Univ, Dept Phys, College Stn, TX 77843 USA
Dutta, Bhaskar
[1
]
Mimura, Yukihiro
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Univ Maryland, Dept Phys, College Pk, MD 20742 USA
Univ Maryland, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USATexas A&M Univ, Dept Phys, College Stn, TX 77843 USA
Mimura, Yukihiro
[2
,3
]
Mohapatra, R. N.
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Univ Maryland, Dept Phys, College Pk, MD 20742 USA
Univ Maryland, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USATexas A&M Univ, Dept Phys, College Stn, TX 77843 USA
Mohapatra, R. N.
[2
,3
]
机构:
[1] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA
[2] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
[3] Univ Maryland, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USA
Diverse mass and mixing patterns between the quarks and leptons makes it challenging to construct a simple grand unified theory of flavor. We show that SO(10) supersymmetry grand unified theories with type II seesaw mechanism giving neutrino masses provide a natural framework for addressing this issue. A simple ansatz that the dominant Yukawa matrix (the 10-Higgs coupling to matter) has rank one appears to simultaneously explain both the large lepton mixings as well as the observed quark flavor hierarchy in these models. A testable prediction of this ansatz is the neutrino mixing, U-e3, which should be observable in planned long baseline experiments.
机构:
Case Western Reserve Univ, Dept Phys, Cleveland, OH 44106 USA
Case Western Reserve Univ, Ctr Educ & Res Cosmol & Astrophys CERCA, Cleveland, OH 44106 USACase Western Reserve Univ, Dept Phys, Cleveland, OH 44106 USA
Perez, Pavel Fileviez
Murgui, Clara
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机构:
CALTECH, Walter Burke Inst Theoret Phys, Pasadena, CA 91125 USACase Western Reserve Univ, Dept Phys, Cleveland, OH 44106 USA