0000000001101937

AUTHOR

C Ha

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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Oral Semaglutide Versus Empagliflozin in Patients With Type 2 Diabetes Uncontrolled on Metformin: The PIONEER 2 Trial

2019

OBJECTIVE Efficacy and safety of the glucagon-like peptide 1 (GLP-1) analog oral semaglutide and the sodium–glucose cotransporter 2 inhibitor empagliflozin were compared in patients with type 2 diabetes uncontrolled on metformin. RESEARCH DESIGN AND METHODS Patients were randomized to once-daily open-label treatment with oral semaglutide 14 mg (n = 412) or empagliflozin 25 mg (n = 410) in a 52-week trial. Key end points were change from baseline to week 26 in HbA1c (primary) and body weight (confirmatory secondary). Two estimands addressed efficacy-related questions: treatment policy (regardless of trial product discontinuation or rescue medication) and trial product (on trial product with…

MaleSettore MED/09 - Medicina InternaEndocrinology Diabetes and MetabolismGlucagon-Like PeptidesAdministration OralType 2 diabeteslaw.inventionSettore MED/13 - Endocrinologia0302 clinical medicineGlucosidesRandomized controlled triallaw030212 general & internal medicineSettore MED/49 - Scienze Tecniche Dietetiche ApplicateBenzhydryl CompoundMiddle AgedMetforminMetforminTreatment Outcomediabetes mellitusDrug Therapy CombinationFemalemedicine.drugHumanAdultmedicine.medical_specialtyGlucagon-Like PeptideGlucosideUrology030209 endocrinology & metabolism03 medical and health sciencesPharmacotherapyDouble-Blind MethodWeight Loss.Diabetes mellitusWeight LossInternal MedicinemedicineEmpagliflozinHumansHypoglycemic AgentsBenzhydryl CompoundsGlycated HemoglobinAdvanced and Specialized NursingHypoglycemic Agentbusiness.industrySemaglutidemedicine.diseaseDiscontinuationDiabetes Mellitus Type 2business
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Search for correlations between the arrival directions of IceCube neutrino events and ultrahigh-energy cosmic rays detected by the Pierre Auger Obser…

2016

This paper presents the results of different searches for correlations between very high-energy neutrino candidates detected by IceCube and the highest-energy cosmic rays measured by the Pierre Auger Observatory and the Telescope Array. We first consider samples of cascade neutrino events and of high-energy neutrino-induced muon tracks, which provided evidence for a neutrino flux of astrophysical origin, and study their cross-correlation with the ultrahigh-energy cosmic ray (UHECR) samples as a function of angular separation. We also study their possible directional correlations using a likelihood method stacking the neutrino arrival directions and adopting different assumptions on the size…

AstronomyAstrophysicsNeutrino experiments ultra high energy cosmic rays cosmic ray experiments neutrino astronomy.01 natural sciencesASTROPHYSICAL SOURCESultra high energy cosmic raylaw.inventionIceCubeAstronomi astrofysik och kosmologimagnetic [deflection]lawAstronomy Astrophysics and Cosmologycosmic ray experiments; neutrino astronomy; neutrino experiments; ultra high energy cosmic rays; Astronomy and Astrophysics010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAngular distanceAstrophysics::Instrumentation and Methods for AstrophysicsVHE [neutrino]GALACTIC MAGNETIC-FIELDcascadeAugerobservatorycosmic radiationCascadestackingcosmic ray experi- mentsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical Phenomenaphysics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical Phenomenacosmic ray experimentFOS: Physical sciencesCosmic rayultra high energy cosmic raysSURFACE DETECTORTelescopeneutrino astronomyneutrino experiments0103 physical sciencesddc:530Angular resolutionHigh Energy PhysicsPierre Auger ObservatorySPECTRUMMuon010308 nuclear & particles physicsAstronomy and Astrophysicsflux [neutrino]ASTROFÍSICAPhysics and Astronomyangular resolutioncorrelationExperimental High Energy Physicsneutrino experimenttracks [muon]cosmic ray experiments
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