Completely dark matter from rapid-turn multifield inflation

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dc.citation.articleNumber181
dc.citation.journalTitleJournal of High Energy Physics
dc.citation.volumeNumber2023
dc.contributor.authorKolb, Edward W.
dc.contributor.authorLong, Andrew J.
dc.contributor.authorMcDonough, Evan
dc.contributor.authorPayeur, Guillaume
dc.date.accessioned2023-03-10T19:04:09Z
dc.date.available2023-03-10T19:04:09Z
dc.date.issued2023
dc.description.abstractWe study cosmological gravitational particle production as applied to “rapid-turn” models of inflation involving two scalar fields. We are interested in the production of massive spin-0 particles that only interact gravitationally and provide a candidate for the dark matter. Specifically, we study two models of rapid-turn multifield inflation, motivated in part by the de Sitter swampland conjecture, that are distinguished by the curvature of field space and the presence or absence of field space ‘angular momentum’ conservation. We find that one of these models leads to insufficient particle production and cannot explain the observed dark matter relic abundance. The second model is able to explain the origin of spin-0 dark matter via gravitational production, and we identify the relevant region of parameter space that is consistent with measurements of the dark-matter relic abundance, the dark-matter-photon isocurvature perturbations, and the spectrum of curvature perturbations that is probed by cosmological observations. Our work demonstrates the compatibility of the de Sitter swampland conjecture with completely dark matter.
dc.identifier.citationKolb, Edward W., Long, Andrew J., McDonough, Evan, et al.. "Completely dark matter from rapid-turn multifield inflation." <i>Journal of High Energy Physics,</i> 2023, (2023) Springer Nature: https://doi.org/10.1007/JHEP02(2023)181.
dc.identifier.digitalJHEP02-2023-181
dc.identifier.doihttps://doi.org/10.1007/JHEP02(2023)181
dc.identifier.urihttps://hdl.handle.net/1911/114493
dc.language.isoeng
dc.publisherSpringer Nature
dc.rightsThis article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleCompletely dark matter from rapid-turn multifield inflation
dc.typeJournal article
dc.type.dcmiText
dc.type.publicationpublisher version
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