An update on the two singlet dark matter model

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dc.contributor.author Basak, Tanushree
dc.contributor.author Coleppa, Baradhwaj
dc.contributor.author Loho, Kousik
dc.date.accessioned 2021-06-05T09:32:51Z
dc.date.available 2021-06-05T09:32:51Z
dc.date.issued 2021-05
dc.identifier.citation Basak, Tanushree; Coleppa, Baradhwaj and Loho, Kousik, "An update on the two singlet dark matter model", arXiv, Cornell University Library, DOI: arXiv:2105.09044, May 2021. en_US
dc.identifier.uri http://arxiv.org/abs/2105.09044
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/6554
dc.description.abstract We revisit the two real singlet extension of the Standard Model with a Z2 *Z'2 symmetry. One of the singlet scalars S2, by virtue of an unbroken Z'2 symmetry, plays the role of a stable dark matter candidate. The other scalar S1, with spontaneously broken Z2-symmetry, mixes with the SM Higgs boson and acts as the scalar mediator. We analyze the model by putting in the entire set of theoretical and recent experimental constraints. The latest bounds from direct detection Xenon1T experiment severely restricts the allowed region of parameter space of couplings. To ensure the dark matter satisfies the relic abundance criterion, we rely on the Breit-Wigner enhanced annihilation cross-section. Further, we study the viability of explaining the observed gamma-ray excess in the galactic center in this model with a dark matter of mass in the ~36-51 GeV window and present our conclusions.
dc.description.statementofresponsibility by Tanushree Basak, Baradhwaj Coleppa and Kousik Loho
dc.language.iso en_US en_US
dc.publisher Cornell University Library en_US
dc.subject High Energy Physics en_US
dc.subject Phenomenology en_US
dc.title An update on the two singlet dark matter model en_US
dc.type Pre-Print en_US
dc.relation.journal arXiv


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