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Gamma-Ray Bursts

Ultra-high-energy, >10^19 eV, cosmic-ray and high energy, ~10^14 eV, neutrino production in GRBs is discussed in the light of recent GRB and cosmic-ray observations. Emphasis is put on model predictions that can be tested with operating and planned cosmic-ray and neutrino detectors, and on the prospects of testing for neutrino properties.

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AuthorshipTopic signalTopic signalWGamma-Ray Burstspreprint / 2000AE. WaxmanResearcherThep-ph13193 worksTastro-ph500 works
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Gamma-Ray Bursts

preprint / 2000

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