Astrophysical High-Energy Neutrinos and Gamma-Ray Bursts

High-energy neutrinos from gamma-ray bursts (GRBs) have been expected in various scenarios. Many predictions for prompt and afterglow emission were done in the pre-Swift era. After the launch of Swift, several new discoveries such as flares have allowed us to expect additional new possibilities of high-energy neutrino emission from GRBs. In this paper, we overview various predictions of GRB neutrino emission, and discuss feature prospects. High-energy neutrino signals may be detected by future-coming large neutrino detectors such as IceCube and KM3Net. If detected, they should be very useful to know the nature of cosmic-ray acceleration sites. It would also help us to reveal the possible connection between ultra-high-energy cosmic rays (UHECRs) and GRBs. Finally, we also compare a prediction of GRB neutrinos with several predictions for other sources such as active galactic nuclei (AGN) and clusters of galaxies.