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Neutrino masses and mixings from supersymmetry with bilinear R-parity violation: A theory for solar and atmospheric neutrino oscillations

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Neutrino masses and mixings from supersymmetry with bilinear R-parity violation: A theory for solar and atmospheric neutrino oscillations

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dc.contributor.author	Hirsch, Martin
dc.contributor.author	Díaz, Marco Aurelio
dc.contributor.author	Porod, Werner
dc.contributor.author	Romao, J. C.
dc.contributor.author	Furtado Valle, José Wagner
dc.date.accessioned	2014-08-28T07:50:56Z
dc.date.available	2014-08-28T07:50:56Z
dc.date.issued	2000
dc.identifier.citation	Hirsch, Martin Díaz, Marco Aurelio Porod, Werner Romao, J. C. Furtado Valle, José Wagner 2000 Neutrino masses and mixings from supersymmetry with bilinear R-parity violation: A theory for solar and atmospheric neutrino oscillations Physical Review D 62 11 113008
dc.identifier.uri	http://hdl.handle.net/10550/37455
dc.description.abstract	The simplest unified extension of the minimal supersymmetric standard model with bilinear R-parity violation naturally predicts a hierarchical neutrino mass spectrum, in which one neutrino acquires mass by mixing with neutralinos, while the other two get mass radiatively. We have performed a full one-loop calculation of the neutralino-neutrino mass matrix in the bilinear R-p minimal supersymmetric standard model, taking special care to achieve a manifestly gauge invariant calculation. Moreover we have performed the renormalization of the heaviest neutrino, needed in order to get meaningful results. The atmospheric mass scale and maximal mixing angle arise from tree-level physics, while solar neutrino scale and oscillations follow from calculable one-loop corrections. If universal supergravity assumptions are made on the soft-supersymmetry breaking terms then the atmospheric scale is calculable as a function of a single R-p violating parameter by the renormalization group evolution due to the nonzero bottom quark Yukawa coupling. The solar neutrino problem must be accounted for by the small mixing angle Mikheyev-Smirnov-Wolfenstein (MSW) solution. If these assumptions are relaxed then one can implement large mixing angle solutions. The theory predicts the lightest supersymmetic particle decay to be observable at high-energy colliders, despite the smallness of neutrino masses indicated by experiment. This provides an independent way to test this solution of the atmospheric and solar neutrino anomalies.
dc.language.iso	eng
dc.relation.ispartof	Physical Review D, 2000, vol. 62, num. 11, p. 113008
dc.subject	Física
dc.title	Neutrino masses and mixings from supersymmetry with bilinear R-parity violation: A theory for solar and atmospheric neutrino oscillations
dc.type	journal article	es_ES
dc.date.updated	2014-08-28T07:50:56Z
dc.identifier.doi	10.1103/PhysRevD.62.113008
dc.identifier.idgrec	072172
dc.rights.accessRights	open access	es_ES