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dc.contributor.authorAlbert, A.
dc.contributor.authorDíaz García, Antonio Francisco 
dc.contributor.authorLópez Coto, Daniel 
dc.contributor.authorNavas Concha, Sergio 
dc.contributor.authorAntares Collaboration
dc.date.accessioned2022-09-02T11:13:42Z
dc.date.available2022-09-02T11:13:42Z
dc.date.issued2022-03-11
dc.identifier.citationPublished version: The ANTARES collaboration... [et al.]. JCAP06(2022)028. [https://doi.org/10.1088/1475-7516/2022/06/028]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/76486
dc.description.abstractSearches for dark matter (DM) have not provided any solid evidence for the existence of weakly interacting massive particles in the GeV-TeV mass range. Coincidentally, the scale of new physics is being pushed by collider searches well beyond the TeV domain. This situation strongly motivates the exploration of DM masses much larger than a TeV. Secluded scenarios contain a natural way around the unitarity bound on the DM mass, via the early matter domination induced by the mediator of its interactions with the Standard Model. High-energy neutrinos constitute one of the very few direct accesses to energy scales above a few TeV. An indirect search for secluded DM signals has been performed with the ANTARES neutrino telescope using data from 2007 to 2015. Upper limits on the DM annihilation cross section for DM masses up to 6PeV are presented and discussed.es_ES
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS), Commissariat à l’énergie atomique et aux énergies alternatives (CEA), Commission Européenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF)es_ES
dc.description.sponsorshipLabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX- 0001), Région Île-de-France (DIM-ACAV), Région Alsace (contrat CPER), Région Provence- Alpes-Côte d’Azur, Département du Var and Ville de La Seyne-sur-Mer, Francees_ES
dc.description.sponsorshipBundesministerium für Bildung und Forschung (BMBF), Germanyes_ES
dc.description.sponsorshipIstituto Nazionale di Fisica Nucleare (INFN), Italyes_ES
dc.description.sponsorshipNederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), The Netherlandses_ES
dc.description.sponsorshipExecutive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romaniaes_ES
dc.description.sponsorshipMinisterio de Ciencia, Innovación, Investigación y Universidades (MCIU): Programa Estatal de Generación de Conocimiento (refs. PGC2018- 096663-B-C41, -A-C42, -B-C43, -B-C44) (MCIU/FEDER), Generalitat Valenciana: Prometeo (PROMETEO/2020/019), Grisolía (refs. GRISOLIA/2018/119, /2021/192) and GenT (refs. CIDEGENT/2018/034, /2019/043, /2020/049, /2021/023) programs, Junta de Andalucía (ref. A-FQM-053-UGR18), La Caixa Foundation (ref. LCF/BQ/IN17/ 11620019), EU: MSC program (ref. 101025085), Spaines_ES
dc.description.sponsorshipMinistry of Higher Education, Scientific Research and Innovation, Moroccoes_ES
dc.description.sponsorshipArab Fund for Economic and Social Development, Kuwaites_ES
dc.description.sponsorshipIfremer, AIM and Foselev Marinees_ES
dc.description.sponsorshipInitiative Physique des Infinis (IPI), Sorbonne Université.es_ES
dc.language.isoenges_ES
dc.publisherInstitute of Physicses_ES
dc.rightsAtribución 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.subjectDark matter experimentses_ES
dc.subjectNeutrino experimentses_ES
dc.subjectUltra high energy photons and neutrinoses_ES
dc.titleSearch for secluded dark matter towards the Galactic Centre with the ANTARES neutrino telescopees_ES
dc.typejournal articlees_ES
dc.rights.accessRightsopen accesses_ES
dc.type.hasVersionSMURes_ES


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Atribución 4.0 Internacional
Except where otherwise noted, this item's license is described as Atribución 4.0 Internacional