Radiative stability of neutrino-mass textures

Parida M.K.; Das C.R.; Rajasekaran G.

dc.contributor.author	Parida M.K.
dc.contributor.author	Das C.R.
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/BF02705337
dc.identifier.issn	3044289
dc.identifier.uri	https://dspace.imsc.res.in/xmlui/handle/123456789/717
dc.identifier.uri	https://www.ias.ac.in/article/fulltext/pram/062/03/0647-0650
dc.description.abstract	Neutrino-mass textures proposed at high scales are known to be unstable against radiative corrections especially for nearly degenerate mass eigenvalues. We find a mechanism in a class of gauge models including 2HDM where the RG constraints can be evaded. Consequently, a high-scale texture can match the low-energy data or be reproduced at low energies.
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	Bi-maximal texture
dc.subject	Renormalisation group
dc.title	Radiative stability of neutrino-mass textures
dc.description.pages	647 - 650
dc.relation.url	https://www.ias.ac.in/article/fulltext/pram/062/03/0647-0650
dc.publisher	Indian Academy of Sciences, Bangalore
dc.type	Conference Paper