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I review gamma-ray burst models (GRBs) and observations, and discuss thepossible production of ultra-high energy cosmic rays and neutrinos in both thestandard internal shock models and the newer generation of photospheric andhadronic GRB models, in the light of current constraints imposed by IceCube,Auger and TA observations. I then discuss models that have been proposed toexplain the recent astrophysical PeV neutrino observations, includingstar-forming and star-burst galaxies, hypernovae and galaxy accretion andmerger shocks.

Ultra-high Energy Cosmic Rays and Neutrinos from Gamma-Ray Bursts, Hypernovae and Galactic Shocks