0000000000529745

AUTHOR

R. Stroem

showing 1 related works from this author

An absence of neutrinos associated with cosmic-ray acceleration in gamma-ray bursts

2012

Gamma-Ray Bursts (GRBs) have been proposed as a leading candidate for acceleration of ultra high-energy cosmic rays, which would be accompanied by emission of TeV neutrinos produced in proton-photon interactions during acceleration in the GRB fireball. Two analyses using data from two years of the IceCube detector produced no evidence for this neutrino emission, placing strong constraints on models of neutrino and cosmic-ray production in these sources.

Physics::Instrumentation and DetectorsAstronomyAstrophysics::High Energy Astrophysical PhenomenaElectronvoltFOS: Physical sciencesFluxhigh-energy neutrinosCosmic rayddc:500.2AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesddc:070IcecubeAccelerationPioncosmic rays0103 physical sciencesTelescope010303 astronomy & astrophysicsVery EnergeticHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsFluxMultidisciplinary010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologySearchAstrophysics::Instrumentation and Methods for Astrophysics13. Climate actionGamma Ray BurstsHigh Energy Physics::ExperimentNeutrinoGamma-ray burstAstrophysics - High Energy Astrophysical PhenomenaNATURE
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