Invisible axion and neutrino masses

dc.contributorUniversidade de São Paulo (USP)
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T14:08:21Z
dc.date.accessioned2022-10-05T15:03:42Z
dc.date.available2014-05-20T14:08:21Z
dc.date.available2022-10-05T15:03:42Z
dc.date.created2014-05-20T14:08:21Z
dc.date.issued2006-01-01
dc.identifierPhysical Review D. College Pk: American Physical Soc, v. 73, n. 1, 4 p., 2006.
dc.identifier1550-7998
dc.identifierhttp://hdl.handle.net/11449/23972
dc.identifier10.1103/PhysRevD.73.017701
dc.identifierWOS:000235009900092
dc.identifierWOS000235009900092.pdf
dc.identifier6783433390235727
dc.identifier0000-0001-5279-8438
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3897191
dc.description.abstractWe show that in any invisible axion model due to the effects of effective nonrenormalizable interactions related to an energy scale near the Peccei-Quinn, grand unification or even the Planck scale, active neutrinos necessarily acquire masses in the sub-eV range. Moreover, if sterile neutrinos are also included and if appropriate cyclic Z(N) symmetries are imposed, it is possible that some of these neutrinos are heavy while others are light.
dc.languageeng
dc.publisherAmerican Physical Soc
dc.relationPhysical Review D
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.titleInvisible axion and neutrino masses
dc.typeArtigo


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