0000000000982666

AUTHOR

S Patton

showing 2 related works from this author

Measurement of the b hadron lifetime with the dipole method

1993

A measurement of the average lifetime of b hadrons has been performed with the dipole method on a sample of 260000 hadronic Z decays recorded with the ALEPH detector during 1991. The dipole is the distance between the vertices built in the opposite hemispheres. The mean dipole is extracted from all the events without attempting b enrichment. Comparing the average of the data dipole distribution with a Monte Carlo calibration curve obtained with different b lifetimes, an average b hadron lifetime of 1.51 +/- 0.08 ps is extracted. RI ANTONELLI, ANTONELLA/C-6238-2011; Buttar, Craig/D-3706-2011; Stahl, Achim/E-8846-2011; Passalacqua, Luca/F-5127-2011; Murtas, Fabrizio/B-5729-2012; St.Denis, Ric…

Nuclear and High Energy Physics[PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex]Calibration curveElectron–positron annihilationMonte Carlo methodHadronElementary particleDiscrete dipole approximation01 natural sciencesinformationNuclear physicsALEPH Experiment0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]mutualisation.010306 general physicsALEPH experimentPhysics010308 nuclear & particles physicsPhysicsmediologyterritoryDipoleHigh Energy Physics::Experimentterritorial intelligenceParticle Physics - Experiment
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The search for Muon neutrinos from northern hemisphere gamma-ray bursts with AMANDA

2007

We present the results of the analysis of neutrino observations by the Antarctic Muon and Neutrino Detector Array (AMANDA) correlated with photon observations of more than 400 gamma-ray bursts (GRBs) in the Northern Hemisphere from 1997 to 2003. During this time period, AMANDA's effective collection area for muon neutrinos was larger than that of any other existing detector. Based on our observations of zero neutrinos during and immediately prior to the GRBs in the dataset, we set the most stringent upper limit on muon neutrino emission correlated with gamma-ray bursts. Assuming a Waxman-Bahcall spectrum and incorporating all systematic uncertainties, our flux upper limit has a normalizatio…

Antarctic Muon And Neutrino Detector ArrayPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural sciencesGamma rays: bursts; Neutrinos0103 physical sciencesMuon neutrinoNeutrinos010306 general physics010303 astronomy & astrophysicsPhysicsGamma rays: burstsMuonAstrophysics (astro-ph)Order (ring theory)Astronomy and AstrophysicsSpace and Planetary ScienceAstronomiaHigh Energy Physics::ExperimentNeutrinoGamma-ray burstEnergy (signal processing)
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