6533b826fe1ef96bd1283ddd

RESEARCH PRODUCT

SEARCH FOR A CORRELATION BETWEEN ANTARES NEUTRINOS AND PIERRE AUGER OBSERVATORY UHECRs ARRIVAL DIRECTIONS

S. Adrian MartinezI. Al SamaraiA. AlbertM. AndreM. AnghinolfiG. AntonS. AnvarM. ArdidT. AstraatmadjaJ. J. AubertB. BaretS. BasaL. J. BeemsterV. BertinS. BiagiC. BigongiariC. BogazziM. Bou CaboB. BouhouM. C. BouwhuisJ. BrunnerJ. BustoF. CamarenaAntonio CaponeC. CarloganuG. CarminatiJ. CarrS. CecchiniZ. CharifPh CharvisT. ChiarusiM. CircellaR. ConiglioneL. CoreH. CostantiniP. CoyleA. CreusotC. CurtilGiulia De BonisM. P. DecowskiI. DekeyserA. DeschampsC. DistefanoC. DonzaudD. DornicQ. DorostiD. DrouhinT. EberlU. EmanueleA. EnzenhoferJ. P. ErnenweinS. EscoffierK. FehnPaolo FermaniM. FerriS. FerryV. FlaminioF. FolgerU. FritschJ. L. FudaS. GalataP. GayK. GeyerG. GiacomelliV. GiordanoJ. P. Gomez GonzalezK. GrafG. GuillardG. HalladjianG. HallewellM. HamalH. Van HarenJ. HartmanA. J. HeijboerY. HelloJ. J. Hernandez ReyB. HeroldJ. HosslC. C. HsuM. De JongM. KadlerO. KalekinA. KappesU. KatzO. KavatsyukP. KooijmanC. KopperA. KouchnerI. KreykenbohmV. KulikovskiyR. LahmannG. LambardG. LarosaD. LattuadaD. LefevreG. LimD. Lo PrestiD. Lo PrestiH. LoehnerS. LoucatosF. LouisS. ManganoM. MarcelinA. MargiottaJ. A. Martinez MoraA. MeliT. MontaruliM. MorgantiN. MorgantiL. MoscosoH. MotzM. NeffE. NezriD. PalioselitisG. E. PavalasK. PayetP. PayreJ. PetrovicP. PiattelliN. Picot ClementeV. PopaT. PradierE. PresaniC. RaccaC. ReedG. RiccobeneC. RichardtR. RichterC. RiviereA. RobertK. RoenschA. RostovtsevJ. Ruiz RivasM. RujoiuG. V. RussoF. SalesaD. F. E. SamtlebenA. Sanchez LosaP. SapienzaJ. SchmidJ. SchnabelF. SchockJ. P. SchullerF. SchusslerT. SeitzR. ShanidzeFrancesco SimeoneA. SpiesM. SpurioJ. J. M. SteijgerTh StolarczykM. TaiutiC. TamburiniA. TrovatoS. ToscanoB. VallageC. ValleeV. Van ElewyckG. VannoniM. VecchiP. VerninE. VisserS. WagnerG. WijnkerJ. WilmsE. De WolfH. YepesD. ZaborovJ. D. ZornozaJ. Zuniga

subject

AstrofísicaSELECTIONPOINT SOURCESTELESCOPE[PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]Astrophysics::High Energy Astrophysical Phenomenaastroparticle physics – cosmic rays – neutrinos[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]FOS: Physical sciencesCosmic rayAstrophysicsPROPAGATIONACCELERATION7. Clean energy01 natural scienceslaw.inventionTelescopecosmic rayslaw0103 physical sciencesICECUBE DETECTORBURSTSNeutrinos010303 astronomy & astrophysicsCosmic raysPierre Auger ObservatoryAstroparticle physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NUCLEI010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyneutrinosastroparticle physicAstronomy and AstrophysicsGALACTIC MAGNETIC-FIELDMassless particleENERGY COSMIC-RAYSSpace and Planetary Scienceastroparticle physicsFISICA APLICADAHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)Lepton

description

A multimessenger analysis optimized for a correlation of arrival directions of ultra-high energy cosmic rays (UHECRs) and neutrinos is presented and applied to 2190 neutrino candidate events detected in 2007-2008 by the ANTARES telescope and 69 UHECRs observed by the Pierre Auger Observatory between 2004 January 1 and 2009 December 31. No significant correlation is observed. Assuming an equal neutrino flux (E-2 energy spectrum) from all UHECR directions, a 90% CL upper limit on the neutrino flux of 5.0 x 10(-8) GeV cm(-2) s(-1) per source is derived.

yearjournalcountryeditionlanguage
2013-08-08
10.1088/0004-637x/774/1/19http://hdl.handle.net/11585/372746