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Constraints on the neutrino emission from the Galactic Ridge with the ANTARES telescope

hal.structure.identifierInstitut d’Investigació per a la Gestió Integrada de Zones Costaneres [IGIC]
dc.contributor.authorADRIÁN-MARTÍNEZ, S.
hal.structure.identifierGroupe de Recherche en Physique des Hautes Energies [GRPHE]
dc.contributor.authorALBERT, A.
hal.structure.identifierLaboratory of Applied Bioacoustics [LAB-UPC]
dc.contributor.authorANDRÉ, M.
dc.contributor.authorANGHINOLFI, M.
hal.structure.identifierErlangen Centre for Astroparticle Physics [ECAP]
dc.contributor.authorANTON, G.
hal.structure.identifierInstitut d’Investigació per a la Gestió Integrada de Zones Costaneres [IGIC]
dc.contributor.authorARDID, M.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorAUBERT, J. -J.
dc.contributor.authorAVGITAS, T.
dc.contributor.authorBARET, B.
dc.contributor.authorBARRIOS-MARTI, J.
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorBASA, S.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorBERTIN, V.
hal.structure.identifierEnrico Fermi - Dipartimento di Fisica
dc.contributor.authorBIAGI, S.
dc.contributor.authorBORMUTH, R.
dc.contributor.authorBOUWHUIS, M. C.
dc.contributor.authorBRUIJN, R.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorBRUNNER, J.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorBUSTO, J.
hal.structure.identifierDipartimento di Fisica [Roma La Sapienza]
dc.contributor.authorCAPONE, A.
dc.contributor.authorCARAMETE, L.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorCARR, J.
dc.contributor.authorCELLI, S.
dc.contributor.authorCHIARUSI, T.
dc.contributor.authorCIRCELLA, M.
dc.contributor.authorCOLEIRO, A.
dc.contributor.authorCONIGLIONE, R.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorCOSTANTINI, H.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorCOYLE, P.
dc.contributor.authorCREUSOT, A.
hal.structure.identifierGéoazur [GEOAZUR 7329]
dc.contributor.authorDESCHAMPS, Anne
dc.contributor.authorDE BONIS, G.
dc.contributor.authorDISTEFANO, C.
hal.structure.identifierUniversité Paris-Sud - Paris 11 [UP11]
dc.contributor.authorDONZAUD, C.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorDORNIC, D.
hal.structure.identifierGroupe de Recherche en Physique des Hautes Energies [GRPHE]
dc.contributor.authorDROUHIN, D.
hal.structure.identifierErlangen Centre for Astroparticle Physics [ECAP]
dc.contributor.authorEBERL, T.
dc.contributor.authorEL BOJADDAINI, I.
hal.structure.identifierInstitut für Theoretische Physik und Astrophysik [Würzburg]
dc.contributor.authorELSAESSER, D.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorENZENHÖFER, A.
dc.contributor.authorFEHN, K.
dc.contributor.authorFELIS, I.
dc.contributor.authorFUSCO, L. A.
dc.contributor.authorGALATÀ, S.
hal.structure.identifierLaboratoire de Physique Corpusculaire - Clermont-Ferrand [LPC]
dc.contributor.authorGAY, P.
dc.contributor.authorGEISSELSOEDER, S.
dc.contributor.authorGEYER, K.
dc.contributor.authorGIORDANO, V.
dc.contributor.authorGLEIXNER, A.
dc.contributor.authorGLOTIN, Hervé
dc.contributor.authorGRACIA-RUIZ, R.
dc.contributor.authorGRAF, K.
dc.contributor.authorHALLMANN, S.
dc.contributor.authorHAREN, H.
dc.contributor.authorHEIJBOER, A. J.
hal.structure.identifierGéoazur [GEOAZUR 7329]
dc.contributor.authorHELLO, Y.
dc.contributor.authorHERNANDEZ-REY, J. J.
dc.contributor.authorHOESSL, J.
dc.contributor.authorHOFESTAEDT, J.
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorHUGON, C.
dc.contributor.authorILLUMINATI, G.
hal.structure.identifierErlangen Centre for Astroparticle Physics [ECAP]
dc.contributor.authorJAMES, C. W.
dc.contributor.authorJONG, M.
dc.contributor.authorKADLER, M.
hal.structure.identifierErlangen Centre for Astroparticle Physics [ECAP]
dc.contributor.authorKALEKIN, O.
dc.contributor.authorKATZ, U.
dc.contributor.authorKIESSLING, D.
dc.contributor.authorKOUCHNER, A.
dc.contributor.authorKRETER, M.
hal.structure.identifierErlangen Centre for Astroparticle Physics [ECAP]
dc.contributor.authorKREYKENBOHM, I.
dc.contributor.authorKULIKOVSKIY, V.
dc.contributor.authorLACHAUD, C.
hal.structure.identifierErlangen Centre for Astroparticle Physics [ECAP]
dc.contributor.authorLAHMANN, R.
hal.structure.identifierInstitut méditerranéen d'océanologie [MIO]
dc.contributor.authorLEFÈVRE, Dominique
dc.contributor.authorLEONORA, E.
dc.contributor.authorLOUCATOS, S.
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorMARCELIN, M.
hal.structure.identifierEnrico Fermi - Dipartimento di Fisica
dc.contributor.authorMARGIOTTA, A.
dc.contributor.authorMARINELLI, A.
dc.contributor.authorMARTINEZ-MORA, J. A.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorMATHIEU, A.
dc.contributor.authorMICHAEL, T.
dc.contributor.authorMIGLIOZZI, P.
hal.structure.identifierLaboratoire des technologies Innovantes [Tanger] [LTI]
dc.contributor.authorMOUSSA, A.
dc.contributor.authorMUELLER, C.
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorNEZRI, E.
dc.contributor.authorPAVALAS, G. E.
dc.contributor.authorPELLEGRINO, C.
dc.contributor.authorPERRINA, C.
dc.contributor.authorPIATTELLI, P.
dc.contributor.authorPOPA, V.
hal.structure.identifierDépartement Recherches Subatomiques [DRS-IPHC]
dc.contributor.authorPRADIER, T.
hal.structure.identifierGroupe de Recherche en Physique des Hautes Energies [GRPHE]
dc.contributor.authorRACCA, C.
dc.contributor.authorRICCOBENE, G.
dc.contributor.authorROENSCH, K.
dc.contributor.authorSALDANA, M.
dc.contributor.authorSAMTLEBEN, D. F. E.
dc.contributor.authorSANCHEZ-LOSA, A.
dc.contributor.authorSANGUINETI, M.
dc.contributor.authorSAPIENZA, P.
dc.contributor.authorSCHNABEL, J.
hal.structure.identifierDépartement de Physique des Particules (ex SPP) [DPhP]
dc.contributor.authorSCHÜSSLER, F.
dc.contributor.authorSEITZ, T.
dc.contributor.authorSIEGER, C.
hal.structure.identifierEnrico Fermi - Dipartimento di Fisica
dc.contributor.authorSPURIO, M.
hal.structure.identifierDépartement de Physique des Particules (ex SPP) [DPhP]
dc.contributor.authorSTOLARCZYK, Th.
dc.contributor.authorTAIUTI, M.
dc.contributor.authorTROVATO, A.
dc.contributor.authorTSELENGIDOU, M.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorTURPIN, D.
dc.contributor.authorTONNIS, C.
dc.contributor.authorVALLAGE, B.
hal.structure.identifierCentre de Physique des Particules de Marseille [CPPM]
dc.contributor.authorVALLÉE, Corentin
hal.structure.identifierInstitut universitaire de France [IUF]
dc.contributor.authorVAN ELEWYCK, V.
dc.contributor.authorVISSER, E.
dc.contributor.authorVIVOLO, D.
dc.contributor.authorWAGNER, S.
hal.structure.identifierErlangen Centre for Astroparticle Physics [ECAP]
dc.contributor.authorWILMS, J.
dc.contributor.authorZORNOZA, J. D.
dc.contributor.authorZUNGA, J.
dc.date.issued2016-09
dc.identifier.issn0370-2693
dc.description.abstractEnA highly significant excess of high-energy astrophysical neutrinos has been reported by the IceCube Collaboration. Some features of the energy and declination distributions of IceCube events hint at a North/South asymmetry of the neutrino flux. This could be due to the presence of the bulk of our Galaxy in the Southern hemisphere. The ANTARES neutrino telescope, located in the Mediterranean Sea, has been taking data since 2007. It offers the best sensitivity to muon neutrinos produced by galactic cosmic ray interactions in this region of the sky. In this letter a search for an extended neutrino flux from the Galactic Ridge region is presented. Different models of neutrino production by cosmic ray propagation are tested. No excess of events is observed and upper limits for different neutrino flux spectral indices Gamma are set. For Gamma = 2.4 the 90% confidence level flux upper limit at 100 TeV for one neutrino flavour corresponds to phi(1f)(0) (100TeV) = 2.0 . 10(-17) GeV-1 cm(-2) s(-1) sr(-1). Under this assumption, at most two events of the IceCube cosmic candidates can originate from the Galactic Ridge. A simple power-law extrapolation of the Fermi-LAT flux to account for IceCube High Energy Starting Events is excluded at 90% confidence level. (C) 2016 The Authors. Published by Elsevier B.V.
dc.language.isoen
dc.publisherElsevier
dc.title.enConstraints on the neutrino emission from the Galactic Ridge with the ANTARES telescope
dc.typeArticle de revue
dc.identifier.doi10.1016/j.physletb.2016.06.051
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv1602.03036
bordeaux.journalPhysics Letters B
bordeaux.page143--148
bordeaux.volume760
bordeaux.peerReviewedoui
hal.identifierhal-01441182
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01441182v1
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