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 |