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Theoretical Aspects of High Energy Neutrinos and GRB

P. Meszaros·S. Razzaque
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Abstract

Neutrinos at energies ranging from sub-TeV to EeV from astrophysical sources can yield interesting physical information about fundamental interactions, about cosmic rays and about the nature of the sources and their environment. Gamma-ray bursts are a leading candidate source, and their expected neutrino emission can address a number of current questions, which may be answered with forthcoming experiments such as IceCube, Auger, ANITA and KM3NeT.

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P. Meszaros, S. Razzaque. 2006-05-05. Theoretical Aspects of High Energy Neutrinos and GRB. https://doi.org/10.1142/9789812708342_0009

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