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dc.contributor.authorKainulainen, Kimmo
dc.contributor.authorKoskivaara, Olli
dc.contributor.authorNurmi, Sami
dc.date.accessioned2023-04-19T10:02:56Z
dc.date.available2023-04-19T10:02:56Z
dc.date.issued2023
dc.identifier.citationKainulainen, K., Koskivaara, O., & Nurmi, S. (2023). Tachyonic production of dark relics : a non-perturbative quantum study. <i>Journal of High Energy Physics</i>, <i>2023</i>(4), Article 43. <a href="https://doi.org/10.1007/jhep04(2023)043" target="_blank">https://doi.org/10.1007/jhep04(2023)043</a>
dc.identifier.otherCONVID_182783314
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/86430
dc.description.abstractWe study production of dark relics during reheating after the end of inflation in a system consisting of a non-minimally coupled spectator scalar field and the inflaton. We derive a set of renormalized quantum transport equations for the one-point function and the two-point function of the spectator field and solve them numerically. We find that our system can embody both tachyonic and parametric instabilities. The former is an expected result due to the non-minimal coupling, but the latter displays new features driven by a novel interplay of the two-point function with the Ricci scalar. We find that when the parametric instability driven by the two-point function takes place, it dominates the total particle production. The quantitative results are also found to be highly sensitive to the model parameters.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherSpringer
dc.relation.ispartofseriesJournal of High Energy Physics
dc.rightsCC BY 4.0
dc.subject.otherearly universe particle physics
dc.subject.othernon-equilibrium field theory
dc.subject.othermodels for dark matter
dc.subject.othernonperturbative effects
dc.titleTachyonic production of dark relics : a non-perturbative quantum study
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-202304192549
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn1126-6708
dc.relation.numberinseries4
dc.relation.volume2023
dc.type.versionpublishedVersion
dc.rights.copyright© 2023 the Authors
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.subject.ysohiukkasfysiikka
dc.subject.ysopimeä aine
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p14101
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1007/jhep04(2023)043
jyx.fundinginformationArticle funded by SCOAP3.
dc.type.okmA1


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