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- W3100201079 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." @default.
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- W3100201079 date "2007-03-01" @default.
- W3100201079 modified "2023-10-06" @default.
- W3100201079 title "THEORETICAL ASPECTS OF HIGH ENERGY NEUTRINOS AND GRB" @default.
- W3100201079 doi "https://doi.org/10.1142/9789812708342_0009" @default.
- W3100201079 hasPublicationYear "2007" @default.
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