0000000001219906

AUTHOR

N. Starinski

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The AMANDA neutrino detector - Status report

2000

Abstract The first stage of the AMANDA High Energy Neutrino Detector at the south Pole, the 302 PMT array AMANDA-B10, is taking data since 1997. We describe results on atmospheric neutrinos, limits on indirect WIMP detection, seasonal muon flux variation, relativistic monopole flux limits, a search for gravitational collapse neutrinos, and a depth scan of the optical ice properties. The next stage 19-string detector AMANDA-II with ∼650 PMTs will be completed in spring 2000.

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorCosmic rayAtomic and Molecular Physics and OpticsParticle detectorMassless particleWIMPNeutrino detectorHigh Energy Physics::ExperimentNeutrinoLeptonNuclear Physics B - Proceedings Supplements
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