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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.identifier.citationPublished version: The ANTARES collaboration... [et al.] JCAP06(2022)018. DOI: [10.1088/1475-7516/2022/06/018]es_ES
dc.description.abstractSolar Atmospheric Neutrinos (SA nu s) are produced by the interaction of cosmic rays with the solar medium. The detection of SA nu s would provide useful information on the composition of primary cosmic rays as well as the solar density. These neutrinos represent an irreducible source of background for indirect searches for dark matter towards the Sun and the measurement of their flux would allow for a better assessment of the uncertainties related to these searches. In this paper we report on the analysis performed, based on an unbinned likelihood maximisation, to search for SA nu s with the ANTARES neutrino telescope. After analysing the data collected over 11 years, no evidence for a solar atmospheric neutrino signal has been found. An upper limit at 90% confidence level on the flux of solar atmospheric neutrinos has been obtained, equal to 7x10(-11) [TeV-1 cm(-2) s(-1)] b at E-nu = 1 TeV for the reference cosmic ray model assumed.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), LabEx 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, Programa Operativo FEDER 2014-2020/Junta de Andalucía-Consejería de Economía y Conocimiento/ Proyecto 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, Morocco, and the Arab Fund for Economic and Social Development, Kuwait.es_ES
dc.publisherInstitute of Physicses_ES
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.subjectNeutrino telescopees_ES
dc.subjectSolar atmospheric neutrinoses_ES
dc.subjectDark matteres_ES
dc.titleSearch for solar atmospheric neutrinos with the ANTARES neutrino telescopees_ES

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Attribution-NonCommercial-NoDerivatives 4.0 Internacional
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivatives 4.0 Internacional