Probing Curvature Effects in the Fermi GRB 110920
arXiv:1304.4168 · doi:10.1088/0004-637X/778/1/3
Abstract
Curvature effects in Gamma-ray bursts (GRBs) have long been a source of considerable interest. In a collimated relativistic GRB jet, photons that are off-axis relative to the observer arrive at later times than on-axis photons and are also expected to be spectrally softer. In this work, we invoke a relatively simple kinematic two-shell collision model for a uniform jet profile and compare its predictions to GRB prompt-emission data for observations that have been attributed to curvature effects such as the peak-flux--peak-frequency relation, i.e., the relation between the F flux and the spectral peak, E in the decay phase of a GRB pulse, and spectral lags. In addition, we explore the behavior of pulse widths with energy. We present the case of the single-pulse Fermi GRB 110920, as a test for the predictions of the model against observations.
8 pages, 11 figures, Accepted for publication in ApJ
References in corpus (3)
Cited by in corpus (17)
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