0000000001064770

AUTHOR

J Jacobsen

showing 4 related works from this author

Lateral distribution of muons in IceCube cosmic ray events

2013

In cosmic ray air showers, the muon lateral separation from the center of the shower is a measure of the transverse momentum that the muon parent acquired in the cosmic ray interaction. IceCube has observed cosmic ray interactions that produce muons laterally separated by up to 400 m from the shower core, a factor of 6 larger distance than previous measurements. These muons originate in high pT (>2  GeV/c) interactions from the incident cosmic ray, or high-energy secondary interactions. The separation distribution shows a transition to a power law at large values, indicating the presence of a hard pT component that can be described by perturbative quantum chromodynamics. However, the ra…

Nuclear and High Energy PhysicsENERGIESPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsddc:500.201 natural sciences7. Clean energyPower lawIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciencescosmic radiation : interactionddc:530Charm (quantum number)Ultra-high-energy cosmic ray010306 general physicsZenithPhysicsQuantum chromodynamicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsGluonMODELPhysics and Astronomy13. Climate actionTEVHigh Energy Physics::ExperimentGLUONAstrophysics - High Energy Astrophysical Phenomena
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Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector

2013

We report on results of an all-sky search for high-energy neutrino events interacting within the IceCube neutrino detector conducted between May 2010 and May 2012. The search follows up on the previous detection of two PeV neutrino events, with improved sensitivity and extended energy coverage down to approximately 30 TeV. Twenty-six additional events were observed, substantially more than expected from atmospheric backgrounds. Combined, both searches reject a purely atmospheric origin for the twenty-eight events at the $4\sigma$ level. These twenty-eight events, which include the highest energy neutrinos ever observed, have flavors, directions, and energies inconsistent with those expected…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General Science & TechnologyPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2AstrophysicsIceCube Collaboration01 natural sciences7. Clean energyHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - Experiment (hep-ex)MD Multidisciplinary0103 physical sciences010303 astronomy & astrophysicsastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Multidisciplinaryhep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyneutrinosSolar neutrino problemKM3NeTNeutrino detector13. Climate actionastro-ph.COMeasurements of neutrino speedHigh Energy Physics::Experimentddc:500NeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaphysicsAstrophysics - Cosmology and Nongalactic AstrophysicsScience
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Precision electroweak measurements on the Z resonance

2005

We report on the final electroweak measurements performed with data taken at the Z resonance by the experiments operating at the electron-positron colliders SLC and LEP. The data consist of 17 million Z decays accumulated by the ALEPH, DELPHI, L3 and OPAL experiments at LEP, and 600 thousand Z decays by the SLD experiment using a polarised beam at SLC. The measurements include cross-sections, forward-backward asymmetries and polarised asymmetries. The mass and width of the Z boson, $\MZ$ and $\GZ$, and its couplings to fermions, for example the $\rho$ parameter and the effective electroweak mixing angle, are precisely measured. The number of light neutrino species is determined to be 2.9840…

Top quarkFORWARD-BACKWARD ASYMMETRYPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; ALEPH; DELPHI; L3; OPALGeneral Physics and Astronomy01 natural sciences7. Clean energyHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)electron-positron physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Electroweak interactionPhysicsQuantum chromodynamicsOPALElectron–positron physics; Electroweak interactions; Decays of heavy intermediate gauge bosons; Fermion–antifermion production; Precision measurements at the Z resonance; Tests of the Standard Model; Radiative corrections; Effective coupling constants; Neutral weak current; Z boson; W boson; Top quark; Higgs bosonParticle physics - ExperimentPhysicsSettore FIS/01 - Fisica SperimentaleElectroweak interactionFORWARD-BACKWARD ASYMMETRY; FERMION-PAIR PRODUCTION; HADRONIC-Z-DECAYS; TOP-QUARK MASS; ANGLE BHABHA SCATTERING; W-BOSON MASS; CROSS-SECTION ASYMMETRY; Z-LINE-SHAPE; SEMILEPTONIC BRANCHING RATIOS; CARLO EVENT GENERATORdecays of heavy intermediate gauge bosons; effective coupling constants; electron-positron physics; electroweak interactions; fermion-antifermion production; higgs boson; neutral weak current; precision measurements at the z resonance; radiative corrections; tests of the standard model; top quark; w boson; z bosonRadiative correctionsALEPHLARGE ELECTRON POSITRON COLLIDERRadiative correctionHigh Energy Physics - PhenomenologyFIS/01 - FISICA SPERIMENTALEDecays of heavy intermediate gauge bosonsL3Z-LINE-SHAPEHiggs bosonFERMION-PAIR PRODUCTIONPARTICLE PHYSICSFísica nuclearNeutrinoFermion–antifermion productionPrecision measurements at the Z resonanceTests of the Standard ModelParticle physicsZ bosonfermion-antifermion productionElectroweak interactionsHiggs bosonFOS: Physical sciencesddc:500.2Elementary particle physics ; z boson ; LEP ; electroweakDecays of heavy intermediate gauge bosonEffective coupling constantPartícules (Física nuclear)Standard ModelNeutral weak currentelectroweak theory Z boson DELPHI ALEPH OPAL L30103 physical sciencesANGLE BHABHA SCATTERINGCROSS-SECTION ASYMMETRYSEMILEPTONIC BRANCHING RATIOS010306 general physicsTOP-QUARK MASSEffective coupling constantsDELPHICoupling constantElectron–positron physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFermionCARLO EVENT GENERATORTop quarkW-BOSON MASSFORWARD-BACKWARD ASYMMETRY FERMION-PAIR PRODUCTION HADRONIC-Z-DECAYS TOP-QUARK MASS ANGLE BHABHA SCATTERING W-BOSON MASS CROSS-SECTION ASYMMETRY Z-LINE-SHAPE SEMILEPTONIC BRANCHING RATIOS CARLO EVENT GENERATOR[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Experimental High Energy PhysicsElectron–positron physicW bosonHigh Energy Physics::ExperimentFIS/04 - FISICA NUCLEARE E SUBNUCLEAREHADRONIC-Z-DECAYSPHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS
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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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