By integrating the relativistic hydrodynamic equations introduced by Taub, we have determined the exact equitemporal surfaces for the gamma-ray burst afterglows. These surfaces are compared and contrasted to the ones obtained, using approximate methods, by Panaitescu & Meszaros, Sari, and Granot et al.

Exact versus approximate equitemporal surfaces in gamma-ray burst afterglows / Bianco, Carlo Luciano; Ruffini, Remo. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - STAMPA. - 605:1 II(2004), pp. L1-L4. [10.1086/386367]

Exact versus approximate equitemporal surfaces in gamma-ray burst afterglows

BIANCO, Carlo Luciano;RUFFINI, Remo
2004

Abstract

By integrating the relativistic hydrodynamic equations introduced by Taub, we have determined the exact equitemporal surfaces for the gamma-ray burst afterglows. These surfaces are compared and contrasted to the ones obtained, using approximate methods, by Panaitescu & Meszaros, Sari, and Granot et al.
2004
black hole physics; gamma rays : bursts; gamma rays : observations; gamma rays : theory; gamma rays: bursts; gamma rays: observations; gamma rays: theory; relativity
01 Pubblicazione su rivista::01a Articolo in rivista
Exact versus approximate equitemporal surfaces in gamma-ray burst afterglows / Bianco, Carlo Luciano; Ruffini, Remo. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - STAMPA. - 605:1 II(2004), pp. L1-L4. [10.1086/386367]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/359657
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