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Invisible dilaton

dc.contributor.authorBrax, Philippe
dc.contributor.authorBurrage, Clare
dc.contributor.authorRuiz Cembranos, José Alberto
dc.contributor.authorValageas, Patrick
dc.date.accessioned2024-12-03T18:54:50Z
dc.date.available2024-12-03T18:54:50Z
dc.date.issued2023-05-09
dc.descriptionCOST Actions: Cosmic WISPers CA21106 and Cosmo Verse CA2136 Grant ST/T000732/1
dc.description.abstractWe analyze the dynamics of a light scalar field responsible for the mu term of the Higgs potential and coupled to matter via the Higgs-portal mechanism. We find that this dilaton model is stable under radiative corrections induced by the standard model particle masses. When the background value of the scalar field is stabilized at the minimum of the scalar potential, the scalar field fluctuations only couple quadratically to the massive fields of the standard model preventing the scalar direct decay into standard model particles. Cosmologically and prior to the electroweak symmetry breaking, the scalar field rolls down along its effective potential before eventually oscillating and settling down at the electroweak minimum. These oscillations can be at the origin of dark matter due to the initial misalignment of the scalar field compared to the electroweak minimum, and we find that, when the mass of the scalar field is less than the electron volt scale and acts as a condensate behaving like dark matter on large scales, the scalar particles cannot thermalize with the standard model thermal bath. As matter couples in a composition-dependent manner to the oscillating scalar, this could lead to a violation of the equivalence principle aboard satellites such as the MICROSCOPE experiment and the next generation of tests of the equivalence principle. Local gravitational tests are evaded thanks to the weakness of the quadratic coupling in the dark matter halo, and we find that, around other sources, these dilaton models could be subject to a screening akin to the symmetron mechanism.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.facultyInstituto de Física de Partículas y del Cosmos (IPARCOS)
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Ciencia e Innovación (España)
dc.description.sponsorshipAgencia Estatal deInvestigación (España)
dc.description.sponsorshipEuropean Commission
dc.description.sponsorshipScience and Technology Facilities Council (UK)
dc.description.sponsorshipAgence Nationale de la Recherche (France)
dc.description.sponsorshipUniversitè Paris-Saclay
dc.description.statuspub
dc.identifier.citationBrax, P., Burrage, C., Cembranos, J. A. R. & Valageas, P. (2023). Invisible dilaton. Physical Review D 107, 095015.
dc.identifier.doi10.1103/physrevd.107.095015
dc.identifier.essn2470-0029
dc.identifier.issn2470-0010
dc.identifier.officialurlhttps://doi.org/10.1103/PhysRevD.107.095015
dc.identifier.relatedurlhttps://doi.org/10.1103/PhysRevD.107.095015
dc.identifier.urihttps://hdl.handle.net/20.500.14352/112013
dc.issue.number9
dc.journal.titlePhysical Review D
dc.language.isoeng
dc.page.final095015-17
dc.page.initial095015-1
dc.publisherAmerican Physical Society
dc.relation.projectIDinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-107394GB-I00/ES/COSMOLOGIA, ASTROFISICA Y GRAVITACION DEL UNIVERSO OSCURO/
dc.relation.projectIDANR-11-IDEX-0003-01
dc.relation.projectIDANR-10-LABX-0038
dc.rightsAttribution 4.0 Internationalen
dc.rights.accessRightsopen access
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subject.cdu530.12
dc.subject.keywordCold dark-matter
dc.subject.keywordGeneral relativity
dc.subject.keywordField
dc.subject.keywordOscillations
dc.subject.ucmFísica (Física)
dc.subject.ucmAstrofísica
dc.subject.unesco2212 Física Teórica
dc.subject.unesco2101 Cosmología y Cosmogonía
dc.titleInvisible dilaton
dc.typejournal article
dc.type.hasVersionVoR
dc.volume.number107
dspace.entity.typePublication
relation.isAuthorOfPublicationc5a4cc87-ceba-494d-95ab-d54b9b1a35e3
relation.isAuthorOfPublication.latestForDiscoveryc5a4cc87-ceba-494d-95ab-d54b9b1a35e3

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