0000000000363189

AUTHOR

K. Munich

showing 4 related works from this author

Search for neutralino pair production at root s = 189 GeV

2001

A search for pair-production of neutralinos at a LEP centre-of-mass energy of 189 GeV gave no evidence for a signal. This limits the neutralino production cross-section and excludes regions in the parameter space of the Minimal Supersymmetric Standard Model (MSSM).

GRAVITINOSParticle physicsCOLLISIONSPhysics and Astronomy (miscellaneous)LOWEST ORDER CALCULATIONSMONTE-CARLO SIMULATIONFOS: Physical sciences2-PHOTON PROCESSESParameter space01 natural sciencesSignalPartícules (Física nuclear)High Energy Physics - ExperimentPHYSICSHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesEVENT GENERATOR[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RADIATIVE-CORRECTIONS010306 general physicsEngineering (miscellaneous)SUPERSYMMETRYDELPHIHIGH-ENERGIESPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLARGE ELECTRON POSITRON COLLIDERPair productionPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHINeutralinoPARTICLE PHYSICSFísica nuclearMONTE-CARLO SIMULATION; LOWEST ORDER CALCULATIONS; RADIATIVE-CORRECTIONS; 2-PHOTON PROCESSES; EVENT GENERATOR; HIGH-ENERGIES; SUPERSYMMETRY; PHYSICS; GRAVITINOS; COLLISIONSHigh Energy Physics::ExperimentEnergy (signal processing)Particle Physics - ExperimentMinimal Supersymmetric Standard ModelEUROPEAN PHYSICAL JOURNAL C
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Search for Extraterrestrial Point Sources of Neutrinos with AMANDA-II

2003

We present the results of a search for point sources of high energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several AGN blazars, microquasars, magnetars and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.

AMANDAcosmic radiation [neutrino]Solar neutrinoAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]General Physics and AstronomyFOS: Physical sciencesAstrophysicsmagnetic [matter]Astrophysicsnumerical methodsddc:550quasarBlazarAstroparticle physicsPhysicsphotomultipliercosmic radiation [muon]water [Cherenkov counter]Astrophysics (astro-ph)AstronomySolar neutrino problemCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::Experimentflux [cosmic radiation]blazar [AGN]data managementNeutrinoupper limitexperimental results
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Search for Neutrino-Induced Cascades with AMANDA

2004

We report on a search for electro-magnetic and/or hadronic showers (cascades) induced by high energy neutrinos in the data collected with the AMANDA II detector during the year 2000. The observed event rates are consistent with the expectations for atmospheric neutrinos and muons. We place upper limits on a diffuse flux of extraterrestrial electron, tau and muon neutrinos. A flux of neutrinos with a spectrum $\Phi \propto E^{-2}$ which consists of an equal mix of all flavors, is limited to $E^2 \Phi(E)=8.6 x 10^{-7} GeV/(cm^{2} s sr)$ at a 90% confidence level for a neutrino energy range 50 TeV to 5 PeV. We present bounds for specific extraterrestrial neutrino flux predictions. Several of t…

PhysicsAMANDAParticle physicsMuonPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHadronHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)FluxFOS: Physical sciencesAstronomy and AstrophysicsElectronAstrophysicsNeutrino astronomyAMANDA; Neutrino astronomy; Neutrino telescopesHigh Energy Physics::ExperimentNeutrino telescopesNeutrino astronomyNeutrinoEvent (particle physics)
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Consistent measurements of alpha(s) from precise oriented event shape distributions

2000

An updated analysis using about 1.5 million events recorded at $\sqrt{s} = M_Z$ with the DELPHI detector in 1994 is presented. Eighteen infrared and collinear safe event shape observables are measured as a function of the polar angle of the thrust axis. The data are compared to theoretical calculations in ${\cal O} (\alpha_s^2)$ including the event orientation. A combined fit of $\alpha_s$ and of the renormalization scale $x_{\mu}$ in $\cal O(\alpha_s^2$) yields an excellent description of the high statistics data. The weighted average from 18 observables including quark mass effects and correlations is $\alpha_s(M_Z^2) = 0.1174 \pm 0.0026$. The final result, derived from the jet cone energ…

QuarkParticle physicsPhysics and Astronomy (miscellaneous)OPTIMIZED PERTURBATION-THEORY; JET CROSS-SECTIONS; E+ E ANNIHILATION; QUANTUM CHROMODYNAMICS; E(+)E(-) ANNIHILATION; QCD CALCULATIONS; Z0 RESONANCE; MONTE-CARLO; DECAYS; ALPHA(S)(M(Z)(2))QCD CALCULATIONSFOS: Physical sciencesScale (descriptive set theory)01 natural sciences7. Clean energyDECAYSPartícules (Física nuclear)High Energy Physics - ExperimentRenormalizationHigh Energy Physics - Experiment (hep-ex)MONTE-CARLO0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Engineering (miscellaneous); Physics and Astronomy (miscellaneous)010306 general physicsEngineering (miscellaneous)ALPHA(S)(M(Z)(2))DELPHIPhysicsQUANTUM CHROMODYNAMICS010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyOrder (ring theory)ObservableFunction (mathematics)E(+)E(-) ANNIHILATIONLARGE ELECTRON POSITRON COLLIDEROrientation (vector space)Experimental uncertainty analysisOPTIMIZED PERTURBATION-THEORYPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSJET CROSS-SECTIONSFísica nuclearHigh Energy Physics::ExperimentE+ E ANNIHILATIONZ0 RESONANCEParticle Physics - Experiment
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