Predictions from high scale mixing unification hypothesis

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dc.contributor.author Abbas G.
dc.contributor.author Gupta S.
dc.contributor.author Rajasekaran G.
dc.contributor.author Srivastava R.
dc.date.accessioned 2023-10-13T12:37:29Z
dc.date.available 2023-10-13T12:37:29Z
dc.date.issued 2014
dc.identifier 10.1103/PhysRevD.89.093009
dc.identifier.issn 15507998
dc.identifier.uri https://dspace.imsc.res.in/xmlui/handle/123456789/693
dc.identifier.uri https://doi.org/10.1103/PhysRevD.89.093009
dc.description.abstract We investigate the renormalization group evolution of masses and mixing angles of Majorana neutrinos under the "high scale mixing unification" hypothesis. Assuming the unification of quark-lepton mixing angles at a high scale, we show that all the experimentally observed neutrino oscillation parameters can be obtained, within the 3-σ range, through the running of corresponding renormalization group equations provided neutrinos have the same charge parity and are quasidegenerate. One of the novel results of our analysis is that θ23 turns out to be nonmaximal and lies in the second octant. Furthermore, we derive new constraints on the allowed parameter space for the unification scale, supersymmetry breaking scale and tanβ, for which the high scale mixing unification hypothesis works. © 2014 American Physical Society.
dc.language.iso en
dc.relation.ispartof Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 89, Issue. 9
dc.rights Copyrighted by the Publisher
dc.source Physical Review D - Particles, Fields, Gravitation and Cosmology
dc.title Predictions from high scale mixing unification hypothesis
dc.relation.url https://doi.org/10.1103/PhysRevD.89.093009
dc.publisher American Physical Society
dc.type Article


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