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Search for a diffuse flux of high-energy neutrino mu with the ANTARES neutrino telescope

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Search for a diffuse flux of high-energy neutrino mu with the ANTARES neutrino telescope

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dc.contributor.author Aguilar, J. A. es_ES
dc.contributor.author Al Samarai, I. es_ES
dc.contributor.author Albert, A. es_ES
dc.contributor.author André, M. es_ES
dc.contributor.author Anghinolfi, M. es_ES
dc.contributor.author Anton, G.
dc.contributor.author Anvar, S.
dc.contributor.author Ardid Ramírez, Miguel
dc.contributor.author Assis Jesus, A.C.
dc.contributor.author Astraatmadja, T.
dc.contributor.author Aubert, J-J.
dc.contributor.author Bou Cabo, Manuel
dc.contributor.author Camarena Femenia, Francisco
dc.contributor.author Larosa, Giuseppina
dc.contributor.author Martínez Mora, Juan Antonio
dc.date.accessioned 2017-12-21T12:37:56Z
dc.date.available 2017-12-21T12:37:56Z
dc.date.issued 2011 es_ES
dc.identifier.issn 0370-2693 es_ES
dc.identifier.uri http://hdl.handle.net/10251/93274
dc.description.abstract [EN] A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neutrino telescope is presented. A (0.83×2¿) sr sky was monitored for a total of 334 days of equivalent live time. The searched signal corresponds to an excess of events, produced by astrophysical sources, over the expected atmospheric neutrino background. The observed number of events is found compatible with the background expectation. Assuming an E -2 flux spectrum, a 90% c.l. upper limit on the diffuse ¿ ¿ flux of E 2¿90%=5.3×10 -8 GeVcm -2s -1sr -11 in the energy range 20 TeV-2.5 PeV is obtained. Other signal models with different energy spectra are also tested and some rejected. © 2010 Elsevier B.V. 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'energie atomique et aux energies alternatives (CEA), Agence National de la Recherche (ANR), Commission Europenne (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 (GVA) and MultiDark, Spain. 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 ELSEVIER SCIENCE BV es_ES
dc.relation.ispartof Physics Letters B es_ES
dc.rights Reconocimiento - No comercial - Sin obra derivada (by-nc-nd) es_ES
dc.subject ANTARES es_ES
dc.subject Diffuse muon neutrino flux es_ES
dc.subject Neutrino telescope es_ES
dc.subject.classification FISICA APLICADA es_ES
dc.title Search for a diffuse flux of high-energy neutrino mu with the ANTARES neutrino telescope es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1016/j.physletb.2010.11.070 es_ES
dc.rights.accessRights Abierto es_ES
dc.contributor.affiliation Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada 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.description.bibliographicCitation Aguilar, JA.; Al Samarai, I.; Albert, A.; André, M.; Anghinolfi, M.; Anton, G.; Anvar, S.... (2011). Search for a diffuse flux of high-energy neutrino mu with the ANTARES neutrino telescope. Physics Letters B. 696(1):16-22. https://doi.org/10.1016/j.physletb.2010.11.070 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion http://doi.org/10.1016/j.physletb.2010.11.070 es_ES
dc.description.upvformatpinicio 16 es_ES
dc.description.upvformatpfin 22 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 696 es_ES
dc.description.issue 1 es_ES
dc.relation.pasarela S\211311 es_ES
dc.contributor.funder Centre National de la Recherche Scientifique, Francia
dc.contributor.funder Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia
dc.contributor.funder Agence Nationale de la Recherche, Francia
dc.contributor.funder European Commission
dc.contributor.funder European Regional Development Fund
dc.contributor.funder Conseil Régional d'Alsace
dc.contributor.funder Conseil Régional Provence-Alpes-Côte d'Azur
dc.contributor.funder Département du Var and Ville de La Seyne-sur-Mer
dc.contributor.funder Bundesministerium für Bildung und Forschung, Alemania
dc.contributor.funder Instituto Nazionale di Fisica Nucleare
dc.contributor.funder Foundation for Fundamental Research on Matter, Holanda
dc.contributor.funder Netherlands Organization for Scientific Research
dc.contributor.funder Council on grants of the President of the Russian Federation
dc.contributor.funder National Authority for Scientific Research, Rumanía
dc.contributor.funder Ministerio de Ciencia e Innovación
dc.contributor.funder Generalitat Valenciana


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