Large neutrino mixing angles for type-I see-saw mechanism in SO(100 GUT

Bipin.R.Desai.; Rajasekaran G.; Utpal Sarkar

dc.contributor.author	Bipin.R.Desai.
dc.contributor.author	Rajasekaran G.
dc.contributor.author	Utpal Sarkar
dc.date.accessioned	2023-11-03T11:57:30Z
dc.date.available	2023-11-03T11:57:30Z
dc.date.issued	2005
dc.identifier	https://arxiv.org/abs/hep-ph/0504066
dc.identifier.uri	https://dspace.imsc.res.in/xmlui/handle/123456789/827
dc.identifier.uri	https://arxiv.org/abs/hep-ph/0504066
dc.description.abstract	We consider the neutrino mixing angles in an SO(10) GUT with the usual Higgs structure in which neutrino masses are explained by the type-I see-saw mechanism. The Dirac-neutrino Yukawa matrix then has a structure similar to that of the u-quark. We determine the light neutrino mass matrix through type-I see-saw mechanism using the experimentally consistent u-quark Yukawa matrix. We find that large neutrino mixing-angles emerge naturally in this model.
dc.language.iso	en
dc.relation.ispartof	arXiv
dc.rights	Open Access
dc.source	arXiv
dc.subject	High Energy Physics – Phenomenology
dc.title	Large neutrino mixing angles for type-I see-saw mechanism in SO(100 GUT
dc.description.pages	1 - 3
dc.relation.url	https://arxiv.org/abs/hep-ph/0504066
dc.publisher	arXiv
dc.type	article