Radiative stability of neutrino-mass textures

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dc.creatorParida, M. K.
dc.creatorDas, C. R.
dc.creatorRajasekaran, G.
dc.date2002-03-10
dc.date.accessioned2026-07-07T11:09:14Z
dc.date.available2026-07-07T11:09:14Z
dc.descriptionNeutrino-mass textures proposed at high-scales are known to be unstable against radiative corrections especially for nearly degenerate eigen values. Within the renormalization group constraints we find a mechanism in a class of gauge theories which guarantees reproduction of any high-scale texture at low energies with radiative stability. We also show how the mechanism explains solar and atmospheric neutrino anomalies through the bimaximal texture at high scale.
dc.description4 pages REVTEX, 1 Postscript fig
dc.identifierhttps://arxiv.org/abs/hep-ph/0203097
dc.identifierhttp://arxiv.org/abs/hep-ph/0203097
dc.identifierPramana62:647-650,2004
dc.identifierdoi:10.1007/BF02705337
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190396
dc.subjectHigh Energy Physics - Phenomenology
dc.titleRadiative stability of neutrino-mass textures
dc.typetext

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