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On the Neutrino Flux from Gamma‐Ray Bursts
Observations imply that γ-ray bursts (GRBs) are produced by the dissipation of the kinetic energy of a highly relativistic fireball. Photomeson interactions of protons with γ-rays within the fireball dissipation region are expected to convert a significant fraction of fireball energy to greater than 1014 eV neutrinos. We present an …