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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/14450
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dc.contributor.authorVaidya, Rishikesh-
dc.date.accessioned2024-02-24T03:51:53Z-
dc.date.available2024-02-24T03:51:53Z-
dc.date.issued2002-09-
dc.identifier.urihttps://www.sciencedirect.com/science/article/pii/S0550321302005606-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14450-
dc.description.abstractWe perform a general analytic study of feasibility of obtaining a combined explanation for the deficits in the solar and the atmospheric neutrino fluxes with two large mixing angles in supersymmetric model with bilinear R parity violations. The required hierarchy among the solar and atmospheric neutrino mass scales follows in this framework in the presence of an approximate Higgs–slepton universality at the weak scale. The solar mixing angle is shown to be related to non-universality in slepton mass terms specifically to differences in soft parameters of the first two leptonic generations. It is shown that this flavour universality violation should be as strong as the Higgs–slepton universality violation if solar neutrino mixing angle is to be large. The standard supergravity models with universal boundary conditions at a high scale lead to the required Higgs–slepton universality violations but the predicted violation of flavour universality among the first two generations is much smaller than required. This model therefore cannot provide an explanation of large solar neutrino mixing angle unless some universality violations in soft supersymmetry breaking parameters are introduced at a high scale itself.en_US
dc.language.isoenen_US
dc.publisherElsevieren_US
dc.subjectPhysicsen_US
dc.subjectBilinear R violationen_US
dc.subjectBi-maximalen_US
dc.titleBi-maximal mixing and bilinear R violationen_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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