Radiative efficiency in gamma-ray bursts and afterglows

Details Radiative efficiency in gamma-ray bursts and afterglows Radiative efficiency in gamma-ray bursts and afterglows

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..428..771p&link_type=abstract

Fourth Huntsville gamma-ray burst symposium. AIP Conference Proceedings, Volume 428, pp. 771-775 (1998).

Astronomy and Astrophysics

Astrophysics

Gamma-Ray Sources, Gamma-Ray Bursts, Fundamental Aspects Of Astrophysics

Scientific paper

We present numerical simulations of gamma-ray bursts arising from external shocks in the impulsive and wind models, including a weak or a strong coupling between electrons and protons+magnetic fields, and analyze their features in each scenario. The dynamics of the fireball-external medium is followed until later times in order to simulate the hydrodynamics of the remnant and the temporal and spectral evolution of the afterglow.

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