Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/4548
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dc.contributor.authorSACHDEVA, DIVYAen_US
dc.contributor.authorSadhukhan, Soumyaen_US
dc.date.accessioned2020-04-17T06:09:20Z
dc.date.available2020-04-17T06:09:20Z
dc.date.issued2020-03en_US
dc.identifier.citationPhysical Review D, 101(5).en_US
dc.identifier.issn2470-0029en_US
dc.identifier.issn2470-0010en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/4548-
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.101.055045en_US
dc.description.abstractEven if the LHC observations are consistent with the Standard model (SM), current LHC results are not precise enough to rule out the presence of new physics. Taking a contrarian view of the SM Higgs fandom, we look out for a more suitable candidate for the 125 GeV boson observed at the LHC. At the same time, a recent result from CMS hints toward an excess near 95 GeV in the diphoton ( γ γ ) channel. Given these aspects, we revisit the Higgs-radion mixing model to explore the viability of the radion mixed Higgs to be the 125 GeV boson along with the presence of a light radion (to be precise, Higgs mixed radion) that can show up in future experiments in the γ γ channel. We find that the mixed radion-Higgs scenario gives a better fit than the SM, with the radion mixed Higgs as a more suitable 125 GeV scalar candidate. It also gives rise to a diphoton excess from the light radion, consistent with the LHC observations.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectPhysicsen_US
dc.subjectTOC-APR-2020en_US
dc.subject2020en_US
dc.subject2020-APR-WEEK3en_US
dc.titleDiscussing 125 GeV and 95 GeV excess in light radion modelen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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