Please use this identifier to cite or link to this item: https://ir.swu.ac.th/jspui/handle/123456789/12217
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dc.contributor.authorTreesukrat W.
dc.contributor.authorUttayarat P.
dc.date.accessioned2021-04-05T03:02:16Z-
dc.date.available2021-04-05T03:02:16Z-
dc.date.issued2019
dc.identifier.issn17426588
dc.identifier.other2-s2.0-85077820146
dc.identifier.urihttps://ir.swu.ac.th/jspui/handle/123456789/12217-
dc.identifier.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85077820146&doi=10.1088%2f1742-6596%2f1380%2f1%2f012093&partnerID=40&md5=5e3b32aa82d9e90217307bd7bc841937
dc.description.abstractDark matter is a clear evidence of new physics beyond the Standard Model. In this work, we consider the inert doublet model where dark matter is a member of a new Higgs doublet. In this scenario, dark matter properties can be calculated. We then test model predictions against experimental results such as the LHC Higgs data, the electroweak precision measurements and dedicated dark matter searches. In addition, we subject the model to theoretical constraints: Perturbativity, vacuum stability and unitarity. Finally, we identify the viable parameter space of the model. © Published under licence by IOP Publishing Ltd.
dc.subjectBeryllium compounds
dc.subjectGalaxies
dc.subjectDark matter searches
dc.subjectHiggs doublet models
dc.subjectNew physics
dc.subjectParameter spaces
dc.subjectPrecision measurement
dc.subjectTest Modeling
dc.subjectThe standard model
dc.subjectVacuum stability
dc.subjectDark Matter
dc.titleDark matter from the inert Higgs doublet model
dc.typeConference Paper
dc.rights.holderScopus
dc.identifier.bibliograpycitationJournal of Physics: Conference Series. Vol 1380, No.1 (2019)
dc.identifier.doi10.1088/1742-6596/1380/1/012093
Appears in Collections:Scopus 1983-2021

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