Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/7749
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dc.contributor.authorKarmakar, Siddharthaen_US
dc.date.accessioned2022-03-17T01:00:00Z-
dc.date.accessioned2022-03-21T11:13:53Z-
dc.date.available2022-03-17T01:00:00Z-
dc.date.available2022-03-21T11:13:53Z-
dc.date.issued2018-
dc.identifier.citationKarmakar, S. (2018). Composite inert doublet dark matter. Paper presented at the Springer Proceedings in Physics, , 203 599-602. doi:10.1007/978-3-319-73171-1_141en_US
dc.identifier.isbn9.78332E+12-
dc.identifier.issn0930-8989-
dc.identifier.otherEID(2-s2.0-85048049072)-
dc.identifier.urihttps://doi.org/10.1007/978-3-319-73171-1_141-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/7749-
dc.description.abstractWe explore inert doublet dark matter model in a scenario where the scalars including the standard model Higgs originate from an underlying strongly-interacting sector. In particular, we concentrate on a model based on a (formula presented) coset. We show that the parameter space allowed from DM relic density in the usual non-composite inert doublet model can get modified by the interplay of the compositeness scale, the relevant quartic coupling and mass differences of the new scalars. © 2018, Springer International Publishing AG, part of Springer Nature.en_US
dc.language.isoenen_US
dc.publisherSpringer Science and Business Media, LLCen_US
dc.sourceSpringer Proceedings in Physicsen_US
dc.subjectGalaxiesen_US
dc.subjectCompositenessen_US
dc.subjectDark matteren_US
dc.subjectMass differenceen_US
dc.subjectModel-based OPCen_US
dc.subjectNon-compositeen_US
dc.subjectParameter spacesen_US
dc.subjectThe standard modelen_US
dc.subjectHigh energy physicsen_US
dc.titleComposite Inert Doublet Dark Matteren_US
dc.typeConference Paperen_US
Appears in Collections:Department of Physics

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