6533b86cfe1ef96bd12c81d5

RESEARCH PRODUCT

Limits on a muon flux from neutralino annihilations in the sun with the IceCube 22-string detector.

E. BlaufussJenni AdamsA. SchukraftK. LaihemJ.-p. HülßS. HickfordR. G. StokstadM. C. StouferS. SchlenstedtH. S. MatisDirk RyckboschD. RutledgeR. WischnewskiH. LeichD. TurcanS. M. MovitFrancis HalzenO. FadiranP. BerghausChristopher WiebuschJ. W. NamS. EulerJ. PetrovicM. V. D'agostinoAlbrecht KarleR. M. GunasinghaD. R. NygrenD. R. NygrenK. RawlinsDamian PielothD. HubertJames MadsenJon DummM. PrikockisT. WaldenmaierTeresa MontaruliTeresa MontaruliC. Pérez De Los HerosJohn HeiseM. R. DuvoortS. OdrowskiMarek KowalskiP. RothJ. J. BeattyA. PiegsaH. LandsmanM. KrasbergJoanna KirylukJoanna KirylukKaren AndeenTodor StanevC. WendtA. WiedemannChristian BohmK. HoshinaGlenn SpiczakM. DanningerC. T. DayDavid A. SchneiderM. OlivoJ. A. GoodmanL. KöpkeA. SlipakS. TilavF. DescampsD. BrederH. MiyamotoK. MeagherReina H. MaruyamaN. MilkeGeorge JaparidzeD. BerleyG. C. HillE. A. StrahlerM. SchunckK. MaseT. KowarikS. YoshidaW. R. EdwardsY. HasegawaA. MohrLaura C. BradleySpencer KleinSpencer KleinMichael J. BakerS. J. PattonK. H. BeckerR. FrankeO. DepaepeM. TluczykontL. GladstoneP. NießenR. NahnhauerG. WikströmT. GrieselB. VoigtS. StoyanovO. EngdegårdC. WalckA. LuckeP. B. PricePeter MészárosA. R. FazelyTyce DeyoungThomas K. GaisserG. B. YodhKara HoffmanY. SestayoP. A. ToaleS. GrullonR. GozziniXinhua BaiJohn ClemT. StraszheimK. KuehnS. SeunarineM. StamatikosCarsten RottJ. LünemannD. J. BoersmaR. C. BayJuan Carlos Diaz-velezQ. SwillensS. PankninFabian KislatA. TepeJ. L. KelleyMarkus AhlersPh. HerquetKael HansonC. P. McparlandG. StephensS. WesterhoffO. TarasovaT. O. B. SchmidtM. BissokDirk LennarzD. Z. BessonA. Van OverloopE. MiddellKarl-heinz SulankeK. BeattieWolfgang RhodeR. PorrataS. BöserA. GoldschmidtXianwu XuKurt WoschnaggO. SchulzC. RoucelleElisa BernardiniR. L. ImlayChristian SpieringKonstancja SataleckaPaul EvensonM. OnoS. KnopsJustin VandenbrouckeElisa ResconiSamvel Ter-antonyanK. MünichW. HuelsnitzJ. L. Bazo AlbaPaolo DesiatiJ. P. RodriguesJ. BerdermannM. RibordyS. BechetK. HelbingH. G. SanderT. StezelbergerS. HussainChad FinleyD. BertrandDmitry ChirkinJ. K. BeckerT. FeuselsS. KlepserT. CastermansAlexander KappesAlexander KappesJ. E. JacobsenF. RothmaierP. RedlRasha AbbasiL. GerhardtL. GerhardtR. J. LauerC. HaK. HultqvistDarren GrantM. M. FoersterA. SilvestriTimo KargNathan WhitehornI. TaboadaAya IshiharaJ. AuffenbergC. De ClercqT. BurgessJ. DreyerJ. C. GallagherY. AbdouS.j. LafebreM. L. BenabderrahmaneG. W. SullivanJames E. BraunM. GurtnerDavid A. WilliamsMarkus AckermannAllan HallgrenS. W. BarwickJohan LundbergPratik MajumdarB. D. FoxR. EhrlichParaic A. KennyTakao KuwabaraB. ChristySeth M. CohenD. SeckelJ. BolmontKarl-heinz KampertR. GanugapatiA. C. PohlA. C. PohlKirill FilimonovA. OlivasD. F. CowenJ. M. JosephR. MorseSubir SarkarP. O. HulthJ. EischG. De Vries-uiterweerdB. SemburgC. TerranovaM. MerckM. WalterA. RizzoH. WissingH. WissingL. DemirörsR. W. EllsworthS. H. SeoHermann KolanoskiM. LabareK. HanAxel GroßAxel GroßOlga BotnerHenrik J. JohanssonAnna FranckowiakN. PotthoffG. KohnenD. TosiN. Van EijndhovenGerald PrzybylskiM. Inaba

subject

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsDark matterFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciences7. Clean energyNuclear physicsWIMP0103 physical sciencesddc:550010306 general physicsNeutrino oscillationNeutrino TelescopeHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonAnnihilation010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyNeutrino detector13. Climate actionNeutralinoHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics

description

A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the IceCube 22-string neutrino detector using data collected in 104.3 days of live-time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured neutralinos in the Sun and converted to limits on the WIMP-proton cross-sections for WIMP masses in the range 250 - 5000 GeV. These results are the most stringent limits to date on neutralino annihilation in the Sun.

10.1103/physrevlett.102.201302https://pubmed.ncbi.nlm.nih.gov/19519015