0000000000237026

AUTHOR

E. Schneider

showing 6 related works from this author

T266 PATIENT EXPECTATIONS AND PHYSICIANS' JUDGEMENT IN THE TREATMENT OF DIABETIC PERIPHERAL NEUROPATHIC PAIN

2011

Anesthesiology and Pain Medicinebusiness.industryAnesthesiaJudgementMedicinebusinessPeripheral neuropathic painEuropean Journal of Pain Supplements
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Observation of high-energy neutrinos using Cerenkov detectors embedded deep in Antarctic ice.

2001

Neutrinos are elementary particles that carry no electric charge and have little mass. As they interact only weakly with other particles, they can penetrate enormous amounts of matter, and therefore have the potential to directly convey astrophysical information from the edge of the Universe and from deep inside the most cataclysmic high-energy regions. The neutrino's great penetrating power, however, also makes this particle difficult to detect. Underground detectors have observed low-energy neutrinos from the Sun and a nearby supernova2, as well as neutrinos generated in the Earth's atmosphere. But the very low fluxes of high-energy neutrinos from cosmic sources can be observed only by mu…

PhysicsAntarctic Muon And Neutrino Detector ArrayMultidisciplinaryPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoAstronomyAstrophysicsSolar neutrino problemCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyNature
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RECENT RESULTS FROM AMANDA

2001

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.

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 currentInternational Journal of Modern Physics A
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Anti-Inflammatory Effects of Onions: Inhibition of Chemotaxis of Human Polymorphonuclear Leukocytes by Thiosulfinates and Cepaenes

1990

Seven different synthetic thiosulfinates, and cepaene- and/or thiosulfinate-rich onion extracts were found to inhibit in vitro the chemotaxis of human granulocytes induced by formyl-methionine-leucinephenylalanine in a dose-dependent manner and at a concentration range of 0.1–100 μ<i>M</i>. Diphenylthiosulfinate showed the highest activity and was found to be more active than prednisolone. The anti-inflammatory properties of onion extracts are related, at least in part, to the inhibition of inflammatory cell influx by thiosulfinates and cepaenes.

AdultNeutrophilsmedicine.drug_classImmunologyInflammationIn Vitro TechniquesBiologyGranulocyteAnti-inflammatoryAlliumMicrobiologymedicineHumansImmunology and AllergyDisulfidesThiosulfinatePlant ExtractsLiliaceaeAnti-Inflammatory Agents Non-SteroidalChemotaxisGeneral Medicinebiology.organism_classificationIn vitroN-Formylmethionine Leucyl-PhenylalanineChemotaxis Leukocytemedicine.anatomical_structureBiochemistrySulfoxidesImmunologymedicine.symptomInternational Archives of Allergy and Immunology
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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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Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector

2002

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.

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 oscillation
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