6533b835fe1ef96bd12a00c6

RESEARCH PRODUCT

Search for dark matter from the Galactic halo with the IceCube neutrino telescope

Christian SpieringC. HaM. L. BenabderrahmaneJustin VandenbrouckeAlbrecht KarleB. D. FoxParaic A. KennyJuanan AguilarK. MeagherTakao KuwabaraT. StraszheimB. ChristyJ. J. BeattyMartin WolfA. IshiharaJohn ClemM. LabarePeter MészárosJ. PosseltP. NiessenAnatoli FedynitchA. PiegsaA. MarottaReina H. MaruyamaSegev BenzviRasha AbbasiSpencer KleinSpencer KleinS. BoeserI. TaboadaT. DengerH. TaavolaAongus O'murchadhaW. HuelsnitzJ. L. KelleyMarkus AhlersN. Van EijndhovenG. StephensS. WesterhoffM. DierckxsensM. StüerR. J. LauerC. De ClercqE. BlaufussJ. C. DavisJ. P. HuelssK. HelbingO. TarasovaL. DemiroersD. BertrandK. H. KampertM. StamatikosM. StamatikosR. PorrataP. B. PriceT. O. B. SchmidtD. BerleyG. C. HillG. KrollDavid A. WilliamsKara HoffmanN. MilkeGeorge JaparidzeH. S. MatisSamvel Ter-antonyanMichael J. BakerD. HeinenC. ColnardKurt WoschnaggTim RuheM. WalterD. TurcanFrancis HalzenP. ZarzhitskyO. FadiranL. GladstoneTimo KargM. SchunckA. GoldschmidtA. SchultesJon DummD. SeckelM. VogePaul EvensonM. WallraffM. GurtnerJ. AuffenbergDmitry ChirkinM. PrikockisT. WaldenmaierJoanna KirylukJoanna KirylukM. KowalskiA. R. FazelyTyce DeyoungP. A. ToaleO. EngdegårdA. Van OverloopD. BoseAlexander KappesElisa ResconiK. KuehnS. H. SeoM. DanningerWolfgang RhodeCh. WeaverF. RothmaierMatthias GeislerK. HultqvistDarren GrantS. M. MovitJ. BerdermannT. KowarikKaren AndeenK. BeattieO. SchulzChad FinleyS. W. BarwickC. Pérez De Los HerosA. TamburroB. VoigtJ. PetrovicXinhua BaiM. OnoK. RawlinsP. RothJ. L. Bazo AlbaP. BerghausM. KrasbergJames MadsenJ. LuenemannD. Z. BessonS. EulerT. GrieselT. FeuselsT. Abu-zayyadK. WiebeQ. SwillensDamian PielothB. RuzybayevD. HubertA. M. BrownPratik MajumdarJ. E. JacobsenMarcos SantanderL. GerhardtL. GerhardtA. RizzoMontaruli26 TeresaTeresa MontaruliO. DepaepeS. StoyanovS. YoshidaM. VehringD. F. CowenA. SlipakS. TilavNathan WhitehornS. CohenR. NahnhauerA. HomeierS. BechetChristopher WiebuschR. C. BayP. RedlTodor StanevC. WendtK.-h. BeckerJuan Carlos Diaz-velezF. DescampsJ. DaughheteeA. TepeKirill FilimonovT. Fischer-waselsA. SchukraftK. LaihemJ. H. KoehneR. FrankeC. WalckF. ClevermannDirk RyckboschThomas K. GaisserG. B. YodhP. O. HulthJ. EischJ. K. BeckerG. De Vries-uiterweerdS. SeunarineG. W. SullivanJames E. BraunD. RutledgeCarsten RottB. SemburgJ. MillerM. BissokPh. HerquetXianwu XuC. BohmH. WissingM. M. FoersterJ. C. GallagherDaniel BindigKael HansonKael HansonJ. Van SantenAllan HallgrenSandro KopperPaolo DesiatiJ. P. RodriguesT. StezelbergerA. GrossJ. DreyerY. AbdouM. V. D'agostinoA. SilvestriM. OlivoM. OlivoJ. A. GoodmanK. MaseSubir SarkarE. MiddellElisa BernardiniM. RibordyJenni AdamsS. HickfordA. SchoenwaldR. G. StokstadR. WischnewskiS. PankninJ. W. NamJ. M. JosephD. R. NygrenS. OdrowskiThomas MeuresS. GrullonM. J. CarsonM. J. LarsonM. MerckFabian KislatA. FranckowiakStijn BuitinkK. HoshinaL. KoepkeGlenn SpiczakR. MorseU. NaumannT. GluesenkampSimona ToscanoS. HussainD. J. KoskinenR. W. EllsworthD. J. BoersmaS.j. LafebreH. G. SanderChun XuHenrik J. JohanssonR. EhrlichA. OlivasH. LandsmanK. SchattoG. KohnenYolanda Sestayo De La CerraT. KringsE. A. StrahlerHermann KolanoskiD. TosiGerald PrzybylskiJ. BlumenthalK. HanOlga BotnerLarissa Paul

subject

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesIceCubeGalactic halo0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsGamma-Ray EmissionHot dark matterAstronomyCosmic-Rays004Dark matter haloParticlesNeutrino detectorAnisotropyHigh Energy Physics::ExperimentHaloDwarf Spheroidal GalaxiesNeutrinoNeutrino astronomyinfo:eu-repo/classification/ddc/004

description

Self-annihilating or decaying dark matter in the Galactic halo might produce high energy neutrinos detectable with neutrino telescopes. We have conducted a search for such a signal using 276 days of data from the IceCube 22-string configuration detector acquired during 2007 and 2008. The effect of halo model choice in the extracted limit is reduced by performing a search that considers the outer halo region and not the Galactic Center. We constrain any large-scale neutrino anisotropy and are able to set a limit on the dark matter self-annihilation cross section of ⟨σAv⟩≃10-22 cm3 s-1 for weakly interacting massive particle masses above 1 TeV, assuming a monochromatic neutrino line spectrum.

10.1103/physrevd.84.022004http://hdl.handle.net/11577/3310571