The expansion of the electron-positron plasma in the GRB phenomenon is compared and contrasted in the treatments of Mészáros, 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. © 2008 Springer-Verlag Berlin Heidelberg.

Baryonic loading and e^+e^- rate equation in GRB sources / Ruffini, Remo; Bianco, C. L.; Vereshchagin, G; Xue, S. S.. - 2008:(2008), pp. 402-406. (Intervento presentato al convegno Relativistic Astrophysics Legacy and Cosmology - Einstein's, ESO Astrophysics Symposia tenutosi a Munich; Germany nel 7-11 November 2005) [10.1007/978-3-540-74713-0_92].

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

RUFFINI, Remo;
2008

Abstract

The expansion of the electron-positron plasma in the GRB phenomenon is compared and contrasted in the treatments of Mészáros, 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. © 2008 Springer-Verlag Berlin Heidelberg.
2008
Relativistic Astrophysics Legacy and Cosmology - Einstein's, ESO Astrophysics Symposia
Neutron stars; Gamma ray bursts; SN ejecta
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
Baryonic loading and e^+e^- rate equation in GRB sources / Ruffini, Remo; Bianco, C. L.; Vereshchagin, G; Xue, S. S.. - 2008:(2008), pp. 402-406. (Intervento presentato al convegno Relativistic Astrophysics Legacy and Cosmology - Einstein's, ESO Astrophysics Symposia tenutosi a Munich; Germany nel 7-11 November 2005) [10.1007/978-3-540-74713-0_92].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/367782
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