6533b870fe1ef96bd12d07a3
RESEARCH PRODUCT
Measurement of the atmospheric ?µ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope
The Antares CollaborationS. Adrián-martínezA. AlbertI. Al SamaraiM. AndréM. AnghinolfiG. AntonS. AnvarM. ArdidT. AstraatmadjaJ-j. AubertB. BaretJ. Barrios-martíS. BasaV. BertinS. BiagiC. BigongiariC. BogazziB. BouhouM. C. BouwhuisR. BruijnJ. BrunnerJ. BustoA. CaponeL. CarameteC. CarloganuJ. CarrS. CecchiniZ. CharifPh. CharvisT. ChiarusiM. CircellaF. ClassenL. CoreH. CostantiniP. CoyleA. CreusotC. CurtilI. DekeyserA. DeschampsG. De BonisM. P. DecowskiC. DistefanoC. DonzaudD. DornicQ. DorostiD. DrouhinA. DumasT. EberlU. EmanueleA. EnzenhöferJ-p. ErnenweinS. EscoffierK. FehnP. FermaniV. FlaminioF. FolgerU. FritschL. A. FuscoS. GalatàP. GayS. GeisselsöderK. GeyerG. GiacomelliV. GiordanoA. GleixnerJ. P. Gómez-gonzálezK. GrafG. GuillardH. Van HarenA. J. HeijboerY. HelloJ. J. Hernández-reyB. HeroldJ. HösslC. W. JamesM. De JongM. KadlerO. KalekinA. KappesU. KatzP. KooijmanA. KouchnerI. KreykenbohmV. KulikovskiyR. LahmannE. LambardG. LambardG. LarosaD. LattuadaD. LefèvreE. LeonoraD. Lo PrestiH. LoehnerS. LoucatosF. LouisS. ManganoM. MarcelinA. MargiottaJ. A. Martínez-moraS. MartiniT. MichaelT. MontaruliM. MorgantiH. MotzC. MuellerM. NeffE. NezriD. PalioselitisG. E. PavalasC. PerrinaP. PiattelliV. PopaT. PradierC. RaccaR. RichterC. RivièreA. RobertK. RoenschA. RostovtsevD. F. E. SamtlebenM. SanguinetiP. SapienzaJ. SchmidJ. SchnabelS. SchulteF. SchüsslerT. SeitzR. ShanidzeC. SiegerF. SimeoneA. SpiesM. SpurioJ. J. M. SteijgerTh. StolarczykA. Sánchez-losaM. TaiutiC. TamburiniY. TayalatiA. TrovatoB. VallageC. ValléeV. Van ElewyckP. VerninE. VisserS. WagnerJ. WilmsE. De WolfK. YatkinH. YepesJ. D. ZornozaJ. Zúñigasubject
Astrofísica:Desenvolupament humà i sostenible::Medi ambient [Àrees temàtiques de la UPC]Physics and Astronomy (miscellaneous)Raigs còsmicsFluxOceanografia7. Clean energy01 natural scienceslaw.inventionlawUnderwater acousticsEnergy range 0.1 to 200 TeVNeutrino TelescopePhysicsRange (particle radiation)Spectral index[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]atmospheric neutrinoNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsLorentz Invariance ViolationFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]OscillationsSoroll -- Aspectes ambientalsAstrophysics::High Energy Astrophysical PhenomenaCosmic rayddc:500.2MACRONuclear physicsTelescopeMUONSSEARCH0103 physical sciencesNeutrinsNeutrinos010306 general physicsEngineering (miscellaneous)Cosmic raysDETECTOR:Física::Acústica [Àrees temàtiques de la UPC]ANTARESAtmospheric neutrino antineutrino010308 nuclear & particles physicsAntares telescopeHigh Energy Physics::Phenomenology[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]13. Climate actionFISICA APLICADAlorentz invariance violation; neutrino oscillation; muonsHigh Energy Physics::ExperimentEnergy (signal processing)Bar (unit)description
Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic rays with air nuclei. In this paper, a measurement of the atmospheric energy spectrum in the energy range 0.1-200 TeV is presented, using data collected by the ANTARES underwater neutrino telescope from 2008 to 2011. Overall, the measured flux is similar to 25 % higher than predicted by the conventional neutrino flux, and compatible with the measurements reported in ice. The flux is compatible with a single power-law dependence with spectral index gamma (meas)=3.58 +/- 0.12. With the present statistics the contribution of prompt neutrinos cannot be established.
year | journal | country | edition | language |
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2013-08-01 | European Physical Journal C |