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- W1750146052 abstract "If gamma ray bursts produce a total energy of 10^54 ergs and this energy is concentrated on the high energy tail of the spectrum E> 1 TeV, then they may account for the observed diffuse extragalactic gamma ray emission for energies > 100 MeV. Such an energy could be released if the GRB's are produced by the burning of the total mass of a neutron star in a phase transition which violates baryon number." @default.
- W1750146052 created "2016-06-24" @default.
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- W1750146052 date "1998-10-15" @default.
- W1750146052 modified "2023-09-27" @default.
- W1750146052 title "Diffuse Extragalactic Gamma Rays and Gamma Ray Bursts" @default.
- W1750146052 hasPublicationYear "1998" @default.
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