Bi-large neutrino mixings by radiative magnification

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dc.contributor.author Mohapatra R.N.
dc.contributor.author Parida M.K.
dc.contributor.author Rajasekaran G.
dc.date.accessioned 2023-10-13T12:37:30Z
dc.date.available 2023-10-13T12:37:30Z
dc.date.issued 2004
dc.identifier 10.1007/BF02705336
dc.identifier.issn 3044289
dc.identifier.uri https://dspace.imsc.res.in/xmlui/handle/123456789/718
dc.identifier.uri https://www.ias.ac.in/article/fulltext/pram/062/03/0643-0646
dc.description.abstract Starting with the unification hypothesis of mixings of quarks and leptons and small quark-like mixings at the see-saw scale, we find that two large mixings for νe, -νμ and νμ - ντ at the weak scale are obtained as a result of renormalization group evolution and radiative magnification if the three neutrinos are quasi degenerate in masses and possess the same CP parity. We also find that Ue3 remains small and well within the CHOOZ-Palo Verde bound since the corresponding Vub for CKM mixing is very small. Several testable pedictions are pointed out.
dc.language.iso en
dc.relation.ispartof Pramana - Journal of Physics, Vol. 62, Issue. 3
dc.rights Open Access
dc.source Pramana - Journal of Physics
dc.subject Radiative magnification
dc.subject Unification of mixings
dc.title Bi-large neutrino mixings by radiative magnification
dc.description.pages 643 - 646
dc.relation.url https://www.ias.ac.in/article/fulltext/pram/062/03/0643-0646
dc.publisher Indian Academy of Sciences, Bangalore
dc.type Conference Paper


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