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dc.contributor.authorEnqvist, Kari
dc.contributor.authorKarciauskas, Mindaugas
dc.contributor.authorLebedev, Oleg
dc.contributor.authorRusak, Stanislav
dc.contributor.authorZatta, Marco
dc.date.accessioned2016-12-13T10:03:49Z
dc.date.available2016-12-13T10:03:49Z
dc.date.issued2016
dc.identifier.citationEnqvist, K., Karciauskas, M., Lebedev, O., Rusak, S., & Zatta, M. (2016). Postinationary vacuum instability and Higgs-inflaton couplings. <i>Journal of Cosmology and Astroparticle Physics</i>, <i>11</i>, Article 025. <a href="https://doi.org/10.1088/1475-7516/2016/11/025" target="_blank">https://doi.org/10.1088/1475-7516/2016/11/025</a>
dc.identifier.otherCONVID_26355727
dc.identifier.otherTUTKAID_71937
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/52294
dc.description.abstractThe Higgs-inflaton coupling plays an important role in the Higgs field dynamics in the early Universe. Even a tiny coupling generated at loop level can have a dramatic effect on the fate of the electroweak vacuum. Such Higgs-inflaton interaction is present both at the trilinear and quartic levels in realistic reheating models. In this work, we examine the Higgs dynamics during the preheating epoch, focusing on the effects of the parametric and tachyonic resonances. We use lattice simulations and other numerical tools in our studies. We find that the resonances can induce large fluctuations of the Higgs field which destabilize the electroweak vacuum. Our considerations thus provide an upper bound on quartic and trilinear interactions between the Higgs and the inflaton. We conclude that there exists a favorable range of the couplings within which the Higgs field is stabilized during both inflation and preheating epochs.en
dc.language.isoeng
dc.publisherInstitute of Physics Publishing Ltd.; Scuola Internazionale Superiore di Studi Avanzati (SISSA)
dc.relation.ispartofseriesJournal of Cosmology and Astroparticle Physics
dc.subject.otherHiggs-inflation couplings
dc.titlePostinationary vacuum instability and Higgs-inflaton couplings
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201612024930
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2016-12-02T13:15:10Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn1475-7516
dc.relation.numberinseries0
dc.relation.volume11
dc.type.versionpublishedVersion
dc.rights.copyright© the Authors, 2016. This is an open access article distributed under the terms of a Creative Commons License. Funded by SCOAP3.
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber278722
dc.rights.urlhttps://creativecommons.org/licenses/by/3.0/
dc.relation.doi10.1088/1475-7516/2016/11/025
dc.relation.funderSuomen Akatemiafi
dc.relation.funderResearch Council of Finlanden
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundinginformationM.K. is supported by the Academy of Finland project 278722 and during the initial stages of this work was supported by JSPS as an International Research Fellow of the Japan Society for the Promotion of Science. O.L. and M.Z. acknowledge support from the Academy of Finland project “The Higgs and the Universe”.
dc.type.okmA1


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© the Authors, 2016. This is an open access article distributed under the terms of a Creative Commons License. Funded by SCOAP3.
Ellei muuten mainita, aineiston lisenssi on © the Authors, 2016. This is an open access article distributed under the terms of a Creative Commons License. Funded by SCOAP3.