0000000000332287

AUTHOR

J Ziemann

showing 2 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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