Observing the dark scalar doublet and its impact on the standard-model Higgs boson at colliders

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dc.contributor.author Cao Q.-H.
dc.contributor.author Ma E.
dc.contributor.author Rajasekaran G.
dc.date.accessioned 2023-10-13T12:37:29Z
dc.date.available 2023-10-13T12:37:29Z
dc.date.issued 2007
dc.identifier 10.1103/PhysRevD.76.095011
dc.identifier.issn 15507998
dc.identifier.uri https://dspace.imsc.res.in/xmlui/handle/123456789/708
dc.identifier.uri https://doi.org/10.1103/PhysRevD.76.095011
dc.description.abstract If the standard model of particle interactions is extended to include a second scalar doublet [H+,(H0+iA0)/2], which is odd under an unbroken Z2 discrete symmetry, it may be called the dark scalar doublet, because its lightest neutral member, say H0, is one possible component for the dark matter of the Universe. We discuss the general phenomenology of the four particles of this doublet, without assuming that H0 is the dominant source of dark matter. We also consider the impact of this dark scalar doublet on the phenomenology of the standard-model Higgs boson h. © 2007 The American Physical Society.
dc.language.iso en
dc.relation.ispartof Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 76, Issue. 9
dc.rights Copyrighted by the Publisher
dc.source Physical Review D - Particles, Fields, Gravitation and Cosmology
dc.title Observing the dark scalar doublet and its impact on the standard-model Higgs boson at colliders
dc.description.pages 1 - 11
dc.relation.url https://doi.org/10.1103/PhysRevD.76.095011
dc.type Article


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