An absence of neutrinos associated with cosmic-ray acceleration in γ-ray bursts
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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...
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High Energy Astrophysical Phenomena (astro-ph.HE) , Flux , Astronomy , Physics , Search , 500 , high-energy neutrinos , FOS: Physical sciences , ddc:500.2 , info:eu-repo/classification/ddc/070 , Astrophysics , 520 , info:eu-repo/classification/ddc/500.2 , High-Energy Neutrinos , Icecube , cosmic rays , Gamma Ray Bursts , Astrophysics - High Energy Astrophysical Phenomena , Telescope