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First results on dark matter annihilation in the Sun using the ANTARES neutrino telescope

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First results on dark matter annihilation in the Sun using the ANTARES neutrino telescope

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dc.contributor.author Adrián Martínez, Silvia es_ES
dc.contributor.author Ardid Ramírez, Miguel es_ES
dc.contributor.author Larosa, Giuseppina es_ES
dc.contributor.author Martínez Mora, Juan Antonio es_ES
dc.contributor.author Al Samaraib, I. es_ES
dc.contributor.author Albert, A. es_ES
dc.contributor.author André, M. es_ES
dc.contributor.author Anghinolfie, M. es_ES
dc.contributor.author Anton, G. es_ES
dc.contributor.author Anton, L. es_ES
dc.contributor.author Anvar, S. es_ES
dc.contributor.author Astraatmadja, T. es_ES
dc.contributor.author Aubert, J.J. es_ES
dc.contributor.author Baret, B. es_ES
dc.contributor.author Basa, S. es_ES
dc.date.accessioned 2016-05-04T15:42:22Z
dc.date.available 2016-05-04T15:42:22Z
dc.date.issued 2013-11
dc.identifier.uri http://hdl.handle.net/10251/63639
dc.description.abstract A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was found to be compatible with background expectations. The 90% CL upper limits in terms of spin-dependent and spin-independent WIMP-proton cross-sections are derived and compared to predictions of two supersymmetric models, CMSSM and MSSM-7. The ANTARES limits are comparable with those obtained by other neutrino observatories and are more stringent than those obtained by direct search experiments for the spin-dependent WIMP-proton cross-section in the case of hard self-annihilation channels (W+W-, T+ T-). es_ES
dc.description.sponsorship The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l' enegie atomique et aux energies alternatives (CEA), Agence National de la Recherche (ANR), Commission Europeenne (FEDER fund and Marie Curie Program), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia e Innovacion (MICINN), Prometeo of Generalitat Valenciana and MultiDark, Spain; Agence de l'Oriental and CNRST, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. en_EN
dc.language Inglés es_ES
dc.publisher IOP Publishing: Hybrid Open Access es_ES
dc.relation Centre National de la Recherche Scientifique (CNRS), France es_ES
dc.relation Commissariat a l'enegie atomique et aux energies alternatives (CEA), France es_ES
dc.relation Agence National de la Recherche (ANR), France es_ES
dc.relation Commission Europeenne (FEDER fund and Marie Curie Program), France es_ES
dc.relation Region Alsace (contrat CPER), France es_ES
dc.relation Region Provence-Alpes-Cote d'Azur, France es_ES
dc.relation Departement du Var and Ville de La Seyne-sur-Mer, France es_ES
dc.relation Bundesministerium fur Bildung und Forschung (BMBF), Germany es_ES
dc.relation Istituto Nazionale di Fisica Nucleare (INFN), Italy es_ES
dc.relation Stichting voor Fundamenteel Onderzoek der Materie (FOM), the Netherlands es_ES
dc.relation Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands es_ES
dc.relation National Authority for Scientific Research (ANCS), Romania es_ES
dc.relation Ministerio de Ciencia e Innovacion (MICINN), Spain es_ES
dc.relation Prometeo of Generalitat Valenciana and MultiDark, Spain es_ES
dc.relation Agence de l'Oriental, Morocco es_ES
dc.relation CNRST, Morocco es_ES
dc.relation.ispartof Journal of Cosmology and Astroparticle Physics es_ES
dc.rights Reserva de todos los derechos es_ES
dc.subject Neutrino experiments es_ES
dc.subject Dark matter detectors es_ES
dc.subject Supersymmetry and cosmology es_ES
dc.subject Particle physics - cosmology connection es_ES
dc.subject.classification FISICA APLICADA es_ES
dc.title First results on dark matter annihilation in the Sun using the ANTARES neutrino telescope es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1088/1475-7516/2013/11/032
dc.rights.accessRights Abierto es_ES
dc.contributor.affiliation Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres es_ES
dc.contributor.affiliation Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada es_ES
dc.description.bibliographicCitation Adrián Martínez, S.; Ardid Ramírez, M.; Larosa, G.; Martínez Mora, JA.; Al Samaraib, I.; Albert, A.; André, M.... (2013). First results on dark matter annihilation in the Sun using the ANTARES neutrino telescope. Journal of Cosmology and Astroparticle Physics. 11(32):1-22. doi:10.1088/1475-7516/2013/11/032 es_ES
dc.description.accrualMethod Senia es_ES
dc.relation.publisherversion http://dx.doi.org/10.1088/1475-7516/2013/11/032 es_ES
dc.description.upvformatpinicio 1 es_ES
dc.description.upvformatpfin 22 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 11 es_ES
dc.description.issue 32 es_ES
dc.relation.senia 251965 es_ES
dc.identifier.eissn 1475-7516


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