6533b823fe1ef96bd127ea2a
RESEARCH PRODUCT
RECENT RESULTS FROM AMANDA
W. WuE. SchneiderD. M. LowderG. C. HillD. SchneiderY. D. HeK. RawlinsP. AskebjerP. B. PriceD. BierenbaumT. ScheiderT. O. B. SchmidtJames MadsenM. HellwigE. AndresH. G. SanderGlenn SpiczakH. RubinsteinKurt WoschnaggP. EkströmM. M. BoyceR. SchwarzF. M. NewcomerC. WalckR. HardtkeR. PorrataG. B. YodhC. Pérez De Los HerosAlbrecht KarleI. LiubarskyA. MihalyiStaffan CariusP. LindahlR. C. BayP. NiessenS. YoungP. RomeneskoAriel GoobarChristian SpieringN. StarinskyB. ErlandssonH. S. MatisD. SteeleD. F. CowenD. ChirkinS. HundertmarkA. BironStefan RichterMarek KowalskiM. SolarzT. MikolajskiS. TilavH. HeukenkampP. C. MockP. MiocinovicC. H. WiebuschJ. LudvigD. RossK. H. BeckerL. GrayXinhua BaiJ. BoothL. ThollanderA. SilvestriI. TaboadaR. G. StokstadR. WischnewskiH. LeichT. C. MillerR. MorseJ. E. JacobsenB. KociT. ThonLars BergströmKael HansonJ. Rodríguez MartinoHakki ÖGelmanAdam BouchtaSteven W. BarwickA. RichardsFrancis HalzenPaolo DesiatiAllan HallgrenJ. P DewulfOle StreicherT. NeunhöfferM. Vander DoncktOlga BotnerV. KandhadaiWolfgang RhodeP. LoaizaA. GoldschmidtY. MinaevaG. BarouchM. GaugCaroline CostaCh. WeinheimerMatthias LeutholdD. R. NygrenP. SteffenL. KöpkeJan ConradT. FeserH. HaaseJodi CooleyE. DalbergD. BertrandA. ChenJoakim EdsjöQ. SunC. ReedJ. DailingP. DoksusNicholas G. UsechakJ. KimT. De YoungP. O. HulthH. WissingPawel Marciniewskisubject
PhysicsNuclear and High Energy PhysicsMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsAstrophysicsSolar neutrino problemAtomic and Molecular Physics and OpticsNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationPhysics::Atmospheric and Oceanic PhysicsCharged currentdescription
We present results based on data taken in 1997 with the 302-PMT Antarctic Muon and Neutrino Detector Array-B10 ("AMANDA-B10") array. Atmospheric neutrinos created in the northern hemisphere are observed indirectly through their charged current interactions which produce relativistic, Cherenkov-light-emitting upgoing muons in the South Pole ice cap. The reconstructed angular distribution of these events is in good agreement with expectation and demonstrates the viability of this ice-based device as a neutrino telescope.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2001-09-01 | International Journal of Modern Physics A |