Diffuse Extragalactic Gamma Rays and Gamma Ray Bursts

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dc.creatorVázquez, R. A.
dc.date1998-10-15
dc.date1998-10-19
dc.date.accessioned2026-07-07T02:28:24Z
dc.date.available2026-07-07T02:28:24Z
dc.descriptionIf 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.
dc.descriptionlatex, 8 pages, no figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9810231
dc.identifierhttp://arxiv.org/abs/astro-ph/9810231
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13108
dc.subjectAstrophysics
dc.titleDiffuse Extragalactic Gamma Rays and Gamma Ray Bursts
dc.typetext

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