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dc.contributor.authorMegías Fernández, Eugenio 
dc.contributor.authorNardini, Germano
dc.contributor.authorQuirós, Mariano
dc.date.accessioned2024-05-17T06:25:05Z
dc.date.available2024-05-17T06:25:05Z
dc.date.issued2023-11-13
dc.identifier.citationEugenio Megías, Germano Nardini, and Mariano Quirós. Pulsar timing array stochastic background from light Kaluza-Klein resonances. Phys. Rev. D 108, 095017 (2023) [10.1103/PhysRevD.108.095017]es_ES
dc.identifier.urihttps://hdl.handle.net/10481/91889
dc.description.abstractWe investigate the potential of the warped extradimension framework as an explanation for the recently observed stochastic gravitational background at nHz frequencies in pulsar timing arrays (PTA). Our analysis reveals that the PTA data can be effectively accommodated by a first-order phase transition triggered by a radion at the MeV-GeV scale feebly coupled to the Standard Model. Remarkably, this outcome remains robust irrespective of the specific details of the warped extradimension embedding, providing a foundation for future investigations aiming to develop concrete extradimension descriptions of Nature. We also demonstrate that many existing embeddings are not viable, as their radion and graviton phenomenology clash with a MeV–GeV scale radion. As a possible way out, we sketch a promising solution involving multiple branes, wherein the light radion, graviton, and ensuing light resonances remain consistent with collider bounds and gravity tests.es_ES
dc.description.sponsorshipProject No. PID2020–114767GB-I00 funded by MCIN/AEI/ 10.13039/501100011033es_ES
dc.description.sponsorshipFEDER/Junta de Andalucía-Consejería de Economía y Conocimiento 2014-2020 Operational Programme under Grant No. A-FQM-178-UGR18es_ES
dc.description.sponsorshipJunta de Andalucía under Grant No. FQM-225es_ES
dc.description.sponsorshipThe Ramón y Cajal Program of the Spanish MICIN and by the European Social Fund under Grant No. RYC-2016-20678es_ES
dc.description.sponsorshipThe “Prórrogas de Contratos Ramón y Cajal” Program of the University of Granadaes_ES
dc.description.sponsorshipThe grant Project. No. 302640 funded by the Research Council of Norwayes_ES
dc.description.sponsorshipDepartament d’Empresa i Coneixement, Generalitat de Catalunya, Grant No. 2021SGR00649es_ES
dc.description.sponsorshipMinisterio de Economía y Competitividad, Grant No. PID2020–115845GB-I00es_ES
dc.description.sponsorshipCERCA program of the Generalitat de Catalunyaes_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.rightsAtribución 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.titlePulsar timing array stochastic background from light Kaluza-Klein resonanceses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.doi10.1103/PhysRevD.108.095017
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersiones_ES


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