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Calculable inverse-seesaw neutrino masses in supersymmetry

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dc.contributor.author	Bazzocchi, F.
dc.contributor.author	Cerdeño, David G.
dc.contributor.author	Muñoz López, Carlos
dc.contributor.author	Furtado Valle, José Wagner
dc.date.accessioned	2015-09-28T10:26:07Z
dc.date.available	2015-09-28T10:26:07Z
dc.date.issued	2010
dc.identifier.citation	Bazzocchi, F. Cerdeño, David G. Muñoz López, Carlos Furtado Valle, José Wagner 2010 Calculable inverse-seesaw neutrino masses in supersymmetry Physical Review D 81 5 051701
dc.identifier.uri	http://hdl.handle.net/10550/47377
dc.description.abstract	We provide a scenario where naturally small and calculable neutrino masses arise from a supersymmetry breaking renormalization-group-induced vacuum expectation value. We adopt a minimal supergravity scenario without ad hoc supersymmetric mass parameters. The lightest supersymmetric particle can be an isosinglet scalar neutrino state, potentially viable as WIMP dark matter through its Higgs new boson coupling. The scenario leads to a plethora of new phenomenological implications at accelerators including the Large Hadron Collider.
dc.language.iso	eng
dc.relation.ispartof	Physical Review D, 2010, vol. 81, num. 5, p. 051701
dc.subject	Física
dc.title	Calculable inverse-seesaw neutrino masses in supersymmetry
dc.type	journal article	es_ES
dc.date.updated	2015-09-28T10:26:07Z
dc.identifier.doi	10.1103/PhysRevD.81.051701
dc.identifier.idgrec	065108
dc.rights.accessRights	open access	es_ES