6533b831fe1ef96bd1299a1c
RESEARCH PRODUCT
Characterization of the atmospheric muon flux in IceCube
C. Pérez De Los HerosM. DayJulian KempN. A. StanishaJ. FeintzeigJoshua PepperT. AndersonK.-h. BeckerM. SchimpJavier GonzalezP. GretskovYiqian XuMatt DunkmanGiorgio MaggiT. Fischer-waselsM. Lesiak-bzdakP. RedlA. SchukraftC. De ClercqE. CheungE. MiddellElisa BernardiniDirk RyckboschSander VanheuleMarkus AckermannS. W. BarwickL. SchulteD. HeeremanLarissa PaulF. ScheriauKarim GhorbaniM. J. LarsonAlbrecht KarleA. SchönwaldD. AltmannG. GolupR. GaiorP. B. PriceN. KurahashiTodor StanevDawn WilliamsC. WendtG. MerinoN. WandkowskyL. SabbatiniG. De WasseigeJenni AdamsCarlos ArguellesK. WiebeT. O. B. SchmidtS. HickfordK. SchattoG. KohnenSurujhdeo SeunarineJ. MillerJ. LeunerR. G. StokstadKirill FilimonovR. HoffmannR. NahnhauerS. TilavC. WalckR. EaganS. SchoenenDelia TosiM. G. AartsenJuanan AguilarT. R. WoodKurt WoschnaggThorsten GlusenkampL. ClassenL. MohrmannS. YoshidaSegev BenzviThomas K. GaisserG. B. YodhM. StamatikosJ. PützE. A. StrahlerM. RelichB. ChristyM. W. E. SmithPaul EvensonK. RawlinsW. HuelsnitzA. IshiharaSpencer KleinSpencer KleinJ. Becker TjusAnatoli FedynitchM. KrollA. GoldschmidtHermann KolanoskiL. BrayeurK. HelbingJames MadsenN. Van EijndhovenC. HaackDmitry ChirkinB. KaminskyI. TaboadaJ. VeenkampD. Z. BessonK. D. De VriesAlexander KappesS. FlisKara HoffmanA. H. Cruz SilvaA. O'murchadhaM. N. TobinB. HansmannA. KoobTimo KargGerald PrzybylskiE. BeiserA. OmairatM. ZollM. JurkovicH.-p. BretzKillian HolzapfelA. ChristovD. J. KoskinenCarsten RottTeresa MontaruliD. R. NygrenM. QuinnanFrank McnallyHershal PandyaK. MeagherA. StasikNathan WhitehornM. BissokWolfgang RhodeA. MeliKendall MahnM. KauerM. KauerR. KonietzE. MiddlemasG. KrollM. GlaglaP. BerghausXianwu XuMarek KowalskiJ. BlumenthalK. HultqvistB. RiedelJoshua HignightJ. KläsM. E. HuberT. MenneC. BohmMaria TselengidouS. SchönebergL. RädelL. GerhardtL. GerhardtDarren GrantOlga BotnerJ. KunnenCh. WeaverM. VehringK. HoshinaS. BöserJ. AuffenbergC. HaC. HaCarl PfendnerV. BaumChad FinleyA. ObertackeGlenn SpiczakSarah NowickiDamian PielothK. MaseAli KheirandishD. F. CowenJ. P. A. M. De AndréA. M. BrownS. EulerU. NaumannMohamed RameezE. UngerM. WallraffT. FuchsL. KöpkeT. StezelbergerM. VogeS. M. SabaA. BernhardD. HellwigChristian SpieringJustin VandenbrouckeMike RichmanKael HansonA. OlivasM. StahlbergA. Haj IsmailN. BuzinskyA. TerliukS. WesterhoffF. HuangM. UsnerJustin LanfranchiM. BörnerJ. KirylukMartin RongenJ. CaseyMatthias VraegheL. WilleP. O. HulthHans NiederhausenRené ReimannBjörn EichmannH. WissingR. HellauerPaolo DesiatiDaniel BindigT. C. ArlenR. StrömX. BaiSally RobertsonAlexander SandrockB. J. WhelanK. ClarkJ. FeldeJ. L. KelleyMarkus AhlersSamvel Ter-antonyanK. KringsRamesh KoiralaDennis SoldinH. TaavolaE. BlaufussD. J. BoersmaJ. C. DavisS. De RidderM. LabareMaryon AhrensM. MediciS. CoendersThomas MeuresN. L. StrotjohannA. R. FazelyE. PinatDonglian XuSubir SarkarSubir SarkarR. MaunuT. KuwabaraJ. C. GrohC. KopperE. JacobiJoakim SandroosAzadeh KeivaniA. HomeierM. CasierChristopher WiebuschJ. DaughheteeJ. P. YanezJ. LünemannR. C. BayG. W. SullivanD. BerleyG. C. HillJames E. BraunRezo ShanidzeJuan Carlos Diaz-velezM. ArchingerL. GladstoneJ. J. BeattyD. SeckelS. FaheyS. MiareckiS. MiareckiJ. C. GallagherTyce DeyoungP. A. ToaleM. LeuermannJ. PosseltF. BosA. StößlTim RuheAllan HallgrenSandro KopperReina H. MaruyamaM. SchmitzK. JeroSofia VallecorsaD. HebeckerMatthias WolfThomas EhrhardtAndrea TurcatiJ. Van SantenH. G. SanderGary BinderGary BinderAxel GroßGeorge JaparidzeSeongjin InElisa ResconiM. S. SutherlandG. TešićS. RichterD. GierD. BoseJ. P. DummT. PalczewskiC. WicharyB. EberhardtH. S. MatisK. AbrahamFrancis HalzenP. ZarzhitskyO. FadiranR. MorseH. DembinskiDariusz Gorasubject
Prompt leptonsleptonAtmospheric muons; Cosmic rays; Prompt leptons; Astronomy and AstrophysicsPhysics::Instrumentation and DetectorsHadronAtmospheric muonsprimary [cosmic radiation]PROTON01 natural sciencesIceCubesurface [detector]atmosphere [muon]NEUTRINO TELESCOPEproduction [muon]PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)ELEMENTAL GROUPSDetectormodel [interaction]Astrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAY MUONSENERGY-SPECTRUMvector mesonstatisticsINTRINSIC CHARMddc:540Physique des particules élémentaireshigh [energy]Astrophysics - High Energy Astrophysical Phenomenaatmosphere [showers]Atmosperic muonsexceptionalairflux [muon]Astrophysics::High Energy Astrophysical Phenomenaspectrum [multiplicity]energy spectrumFOS: Physical sciencesCosmic rayatmosphere [cosmic radiation]Nuclear physicscosmic rays0103 physical sciencesARRIVAL DIRECTIONSVector meson010306 general physicsCosmic raysZenithANISOTROPYMuon010308 nuclear & particles physicsAstronomy and AstrophysicsSpectral componenttracksMODELPhysics and Astronomy13. Climate actionTEVspectralHigh Energy Physics::ExperimenthadronLeptondescription
Muons produced in atmospheric cosmic ray showers account for the by far dominant part of the event yield in large-volume underground particle detectors. The IceCube detector, with an instrumented volume of about a cubic kilometer, has the potential to conduct unique investigations on atmospheric muons by exploiting the large collection area and the possibility to track particles over a long distance. Through detailed reconstruction of energy deposition along the tracks, the characteristics of muon bundles can be quantified, and individual particles of exceptionally high energy identified. The data can then be used to constrain the cosmic ray primary flux and the contribution to atmospheric lepton fluxes from prompt decays of short-lived hadrons. In this paper, techniques for the extraction of physical measurements from atmospheric muon events are described and first results are presented. The multiplicity spectrum of TeV muons in cosmic ray air showers for primaries in the energy range from the knee to the ankle is derived and found to be consistent with recent results from surface detectors. The single muon energy spectrum is determined up to PeV energies and shows a clear indication for the emergence of a distinct spectral component from prompt decays of short-lived hadrons. The magnitude of the prompt flux, which should include a substantial contribution from light vector meson di-muon decays, is consistent with current theoretical predictions. The variety of measurements and high event statistics can also be exploited for the evaluation of systematic effects. In the course of this study, internal inconsistencies in the zenith angle distribution of events were found which indicate the presence of an unexplained effect outside the currently applied range of detector systematics. The underlying cause could be related to the hadronic interaction models used to describe muon production in air showers.
year | journal | country | edition | language |
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2015-06-26 |