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.File allegati a questo prodotto
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