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Discussing 125 GeV and 95 GeV excess in light radion model

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dc.contributor.author SACHDEVA, DIVYA en_US
dc.contributor.author Sadhukhan, Soumya en_US
dc.date.accessioned 2020-04-17T06:09:20Z
dc.date.available 2020-04-17T06:09:20Z
dc.date.issued 2020-03 en_US
dc.identifier.citation Physical Review D, 101(5). en_US
dc.identifier.issn 2470-0029 en_US
dc.identifier.issn 2470-0010 en_US
dc.identifier.uri http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/4548
dc.identifier.uri https://doi.org/10.1103/PhysRevD.101.055045 en_US
dc.description.abstract Even 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.iso en en_US
dc.publisher American Physical Society en_US
dc.subject Physics en_US
dc.subject TOC-APR-2020 en_US
dc.subject 2020 en_US
dc.subject 2020-APR-WEEK3 en_US
dc.title Discussing 125 GeV and 95 GeV excess in light radion model en_US
dc.type Article en_US
dc.contributor.department Dept. of Physics en_US
dc.identifier.sourcetitle Physical Review D en_US
dc.publication.originofpublisher Foreign en_US


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