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dc.contributor.authorKaram, Alexandros
dc.contributor.authorMarkkanen, Tommi
dc.contributor.authorMarzola, Luca
dc.contributor.authorNurmi, Sami
dc.contributor.authorRaidal, Martti
dc.contributor.authorRajantie, Arttu
dc.date.accessioned2020-12-01T10:59:57Z
dc.date.available2020-12-01T10:59:57Z
dc.date.issued2020
dc.identifier.citationKaram, A., Markkanen, T., Marzola, L., Nurmi, S., Raidal, M., & Rajantie, A. (2020). Novel mechanism for primordial perturbations in minimal extensions of the Standard Model. <i>Journal of High Energy Physics</i>, <i>2020</i>(11), Article 153. <a href="https://doi.org/10.1007/jhep11(2020)153" target="_blank">https://doi.org/10.1007/jhep11(2020)153</a>
dc.identifier.otherCONVID_47214096
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/72898
dc.description.abstractWe demonstrate that light spectator fields in their equilibrium can source sizeable CMB anisotropies through modulated reheating even in the absence of direct couplings to the inflaton. The effect arises when the phase space of the inflaton decay is modulated by the spectator which generates masses for the decay products. We call the mechanism indirect modulation and using the stochastic eigenvalue expansion show that it can source perturbations even four orders of magnitude larger than the observed amplitude. Importantly, the indirect mechanism is present in the Standard Model extended with right- handed neutrinos. For a minimally coupled Higgs boson this leads to a novel lower bound on the quartic coupling and constrains the neutrino Yukawas below unity.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherSpringer
dc.relation.ispartofseriesJournal of High Energy Physics
dc.rightsCC BY 4.0
dc.subject.othercosmology of theories beyond the SM
dc.subject.otherHiggs physics
dc.titleNovel mechanism for primordial perturbations in minimal extensions of the Standard Model
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202012016859
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.numberinseries11
dc.relation.volume2020
dc.type.versionpublishedVersion
dc.rights.copyright© The Authors. Article funded by SCOAP3
dc.rights.accesslevelopenAccessfi
dc.subject.ysohiukkasfysiikka
dc.subject.ysoHiggsin bosonit
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p27401
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1007/jhep11(2020)153
jyx.fundinginformationThis work was supported by the Estonian Research Council grants PRG356, PRG803, MOBTT86, MOBJD381, MOBTT5 and by the EU through the European Regional Development Fund CoE program TK133 “The Dark Side of the Universe”. This project has received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 786564. AR was funded by the U.K. Science and Technology Facilities Council grant ST/P000762/1 and Institute for Particle Physics Phenomenology Associateship.
dc.type.okmA1


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