Baryonic loading and e^+e^- rate equation in GRB sources

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dc.creatorRuffini, Remo
dc.creatorBianco, Carlo Luciano
dc.creatorVereshchagin, Gregory
dc.creatorXue, She-Sheng
dc.date2006-05-16
dc.date.accessioned2026-07-07T08:46:58Z
dc.date.available2026-07-07T08:46:58Z
dc.descriptionThe expansion of the electron-positron plasma in the GRB phenomenon is compared and contrasted in the treatments of Meszaros, Laguna and Rees, of Shemi, Piran and Narayan, and of Ruffini et al. The role of the correct numerical integration of the hydrodynamical equations, as well as of the rate equation for the electron-positron plasma loaded with a baryonic mass, are outlined and confronted for crucial differences.
dc.description5 pages, 3 figures, to appear in the proceedings of "Relativistic Astrophysics and Cosmology - Einstein's Legacy" meeting, November 7-11, 2005, Munich, Germany, edited by B. Aschenbach, V. Burwitz, G. Hasinger, and B. Leibundgut
dc.identifierhttps://arxiv.org/abs/astro-ph/0605385
dc.identifierhttp://arxiv.org/abs/astro-ph/0605385
dc.identifierdoi:10.1007/978-3-540-74713-0_92
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143434
dc.subjectAstrophysics
dc.titleBaryonic loading and e^+e^- rate equation in GRB sources
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