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dc.contributorVirginia Techen
dc.contributor.authorLoinaz, W.en
dc.contributor.authorOkamura, N.en
dc.contributor.authorRayyan, S.en
dc.contributor.authorTakeuchi, T.en
dc.contributor.authorWijewardhana, L. C. R.en
dc.date.accessioned2013-12-18T19:46:40Zen
dc.date.available2013-12-18T19:46:40Zen
dc.date.issued2003-10-01en
dc.identifier.citationLoinaz, W ; Okamura, N ; Rayyan, S ; et al., OCT 1 2003. “Quark-lepton unification and lepton flavor nonconservation from a TeV-scale seesaw neutrino mass texture,” PHYSICAL REVIEW D 68(7): 073001. DOI: 10.1103/PhysRevD.68.073001en
dc.identifier.issn0556-2821en
dc.identifier.urihttp://hdl.handle.net/10919/24753en
dc.description.abstractIn a recent paper we pointed out that the mixing of the light neutrinos with heavy gauge singlet states could reconcile the Z-pole data from e(+)e(-) colliders and the nu(mu) ((nu) over bar (mu)) scattering data from the NuTeV experiment at Fermilab. We further noted that the mixing angle required to fit the data is much larger than what would be expected from the conventional seesaw mechanism. In this paper, we show how such mixings can be arranged by a judicious choice of the neutrino mass texture. We also argue that by invoking the unification of the Dirac mass matrix for the up-type quarks and the neutrinos, the mass of the heavy states can naturally be expected to lie in the few TeV range. The model is strongly constrained by the lepton flavor changing process mu-->egamma which requires lepton universality to be violated in the charged channel.en
dc.language.isoen_USen
dc.publisherAmerican Physical Societyen
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subjectmixing anglesen
dc.subjectstandard modelen
dc.subjectheavy-leptonsen
dc.subjectmatrixen
dc.subjectsymmetryen
dc.subjectoscillationsen
dc.subjecthierarchyen
dc.subjectmu->e-gammaen
dc.subjectcouplingsen
dc.subjectmuonen
dc.subjectAstronomy & Astrophysicsen
dc.subjectPhysicsen
dc.titleQuark-lepton unification and lepton flavor nonconservation from a TeV-scale seesaw neutrino mass textureen
dc.typeArticle - Refereeden
dc.contributor.departmentInstitute for Particle, Nuclear and Astronomical Sciences (IPNAS)en
dc.contributor.departmentPhysicsen
dc.identifier.urlhttp://link.aps.org/doi/10.1103/PhysRevD.68.073001en
dc.date.accessed2013-12-16en
dc.title.serialPhysical Review Den
dc.identifier.doihttps://doi.org/10.1103/PhysRevD.68.073001en


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