Explaining solar neutrinos with heavy Higgs masses in partial split supersymmetry

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dc.contributor.authorDíaz, Marco A.
dc.contributor.authorGaray Walls, Francisca
dc.contributor.authorKoch, Benjamin
dc.contributor.authorDíaz, Marco A.
dc.contributor.authorGaray Walls, Francisca
dc.contributor.authorKoch, Benjamin
dc.contributor.authorDíaz, Marco A.
dc.contributor.authorGaray Walls, Francisca
dc.contributor.authorKoch, Benjamin
dc.contributor.authorDíaz, Marco A.
dc.contributor.authorGaray Walls, Francisca
dc.contributor.authorKoch, Benjamin
dc.date.accessioned2017-04-25T19:24:30Z
dc.date.available2017-04-25T19:24:30Z
dc.date.issued2009
dc.identifier.issn1550-7998
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/20350
dc.language.isoen
dc.relation.isformatofPhysical Review D Vol. 80, no. 11 (2009), p. [113005]-113005
dc.revistaPhysical Review Des_ES
dc.rightsacceso restringido
dc.subject.ddc510
dc.subject.deweyMatemática física y químicaes_ES
dc.subject.otherNeutrinoses_ES
dc.subject.otherPartículas de Higgses_ES
dc.subject.otherSupersimetríaes_ES
dc.titleExplaining solar neutrinos with heavy Higgs masses in partial split supersymmetryes_ES
dc.typeartículo
sipa.codpersvinculados104746
sipa.codpersvinculados1006903
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