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Cosmological signatures of superheavy dark matter
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).
Number of Authors: 42020 (English)In: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, no 7, article id 231Article in journal (Refereed) Published
Abstract [en]

We discuss two possible scenarios, namely the curvaton mechanism and the dark matter density modulation, where non-Gaussianity signals of superheavy dark matter produced by gravity can be enhanced and observed. In both scenarios, superheavy dark matter couples to an additional light field as a mediator. In the case of derivative coupling, the resulting non-Gaussianities induced by the light field can be large, which can provide inflationary evidences for these superheavy dark matter scenarios.

Place, publisher, year, edition, pages
2020. no 7, article id 231
Keywords [en]
Cosmology of Theories beyond the SM, Beyond Standard Model
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:su:diva-185450DOI: 10.1007/JHEP07(2020)231ISI: 000559805700002OAI: oai:DiVA.org:su-185450DiVA, id: diva2:1503682
Available from: 2020-11-25 Created: 2020-11-25 Last updated: 2022-02-25Bibliographically approved

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Zhou, Siyi

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