Freeze-in dark matter through forbidden channel in U(1) B-L

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dc.contributor.author Konar, Partha
dc.contributor.author Roshan, Rishav
dc.contributor.author Show, Sudipta
dc.coverage.spatial United Kingdom
dc.date.accessioned 2022-03-29T10:53:08Z
dc.date.available 2022-03-29T10:53:08Z
dc.date.issued 2022-03
dc.identifier.citation Konar, Partha; Roshan, Rishav and Show, Sudipta, "Freeze-in dark matter through forbidden channel in U(1) B-L", Journal of Cosmology and Astroparticle Physics, DOI: 10.1088/1475-7516/2022/03/021, vol. 2022, no. 3, Mar. 2022. en_US
dc.identifier.issn 1475-7516
dc.identifier.uri https://doi.org/10.1088/1475-7516/2022/03/021
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/7619
dc.description.abstract We examine a scenario for freeze-in production of dark matter, which occurs due to the large thermal correction to the mass of a decaying mediator particle present in the thermal bath of the early Universe. We show that the decays, which are kinematically forbidden otherwise, can open up at very high temperatures and dominate the dark matter production. We explore such forbidden production of dark matter in the minimal U(1)B-L model, comparing dark matter phenomenology in the context of forbidden frozen-in with the standard picture.
dc.description.statementofresponsibility by Partha Konar, Rishav Roshan and Sudipta Show
dc.format.extent vol. 2022, no. 3
dc.language.iso en_US en_US
dc.publisher IOP Publishing en_US
dc.subject Dark matter en_US
dc.subject Forbidden channel en_US
dc.subject Decaying mediator en_US
dc.subject Phenomenology en_US
dc.subject Matter en_US
dc.title Freeze-in dark matter through forbidden channel in U(1) B-L en_US
dc.type Article en_US
dc.relation.journal Journal of Cosmology and Astroparticle Physics


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