6533b7d4fe1ef96bd1262a4e
RESEARCH PRODUCT
Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector
J. AhrensE. AndrésO. BotnerM. Vander DoncktC. WalckC. WeinheimerC. H. WiebuschC. WiedemannR. WischnewskiH. WissingK. WoschnaggW. WuG. YodhA. BouchtaS. YoungAmanda CollaborationS. CariusA. ChenD. ChirkinJ. ConradJ. CooleyC. G. S. CostaD. F. CowenE. DalbergX. BaiC. De ClercqT. DeyoungP. DesiatiJ.-p. DewulfP. DoksusJ. EdsjöP. EkströmT. FeserT. K. GaisserM. GaugG. BarouchL. GerhardtA. GoldschmidtA. GoobarA. HallgrenF. HalzenK. HansonR. HardtkeT. HauschildtM. HellwigG. C. HillS. W. BarwickP. O. HulthS. HundertmarkJ. JacobsenA. KarleJ. KimB. KociL. KöpkeM. KowalskiJ. I. LamoureuxH. LeichR. C. BayM. LeutholdP. LindahlP. LoaizaD. M. LowderJ. LudvigJ. MadsenP. MarciniewskiH. S. MatisC. P. McparlandT. C. MillerT. BeckaY. MinaevaP. MiočinovićP. C. MockR. MorseT. NeunhöfferP. NiessenD. R. NygrenH. OgelmanPh. OlbrechtsC. Pérez De Los HerosK.-h. BeckerA. PohlR. PorrataP. B. PriceG. T. PrzybylskiK. RawlinsW. RhodeM. RibordyS. RichterJ. Rodríguez MartinoP. RomeneskoD. BertrandD. RossH.-g. SanderT. SchmidtD. SchneiderE. SchneiderR. SchwarzA. SilvestriM. SolarzG. M. SpiczakC. SpieringA. BironD. SteeleP. SteffenR. G. StokstadO. StreicherP. SudhoffK. H. SulankeI. TaboadaL. ThollanderT. ThonS. Tilavsubject
PhysicsNuclear and High Energy PhysicsParticle physicsAnnihilationPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDark matterDetectorAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesSupersymmetryAstrophysicsHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Neutrino detectorWIMPNeutralinoHigh Energy Physics::Experimentddc:530Neutrino oscillationdescription
A search for nearly vertical up-going muon-neutrinos from neutralino annihilations in the center of the Earth has been performed with the AMANDA-B10 neutrino detector. The data sample collected in 130.1 days of live-time in 1997, ~10^9 events, has been analyzed for this search. No excess over the expected atmospheric neutrino background is oberved. An upper limit at 90% confidence level on the annihilation rate of neutralinos in the center of the Earth is obtained as a function of the neutralino mass in the range 100 GeV-5000 GeV, as well as the corresponding muon flux limit.
year | journal | country | edition | language |
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2002-02-20 |