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Nonthermal Synchrotron and Synchrotron Self-Compton Emission from GRBs: Predictions for Swift and GLAST

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.2943490· OSTI ID:21137201
 [1];  [2];  [3]
  1. U.S. Naval Research Laboratory, Code 7653, Washington, DC 20375 (United States) and NRL/NRC Research Associate
  2. U.S. Naval Research Laboratory, Code 7653, Washington, DC 20375 (United States)
  3. Astrophysical Institute, Department of Physics and Astronomy, Athens, Ohio 45701 (United States)
Results of a leptonic jet model for the prompt emission and early afterglows of GRBs are presented. The synchrotron component is modeled with the canonical Band spectrum and the synchrotron self-Compton component is calculated from the implied synchrotron-emitting electron spectrum in a relativistic plasma blob. In the comoving frame the magnetic field is assumed to be tangled and the electron and photon distributions are assumed to be isotropic. The Compton-scattered spectrum is calculated using the full Compton cross-section in the Thomson through Klein-Nishina using the Jones formula. Pair production photoabsorption, both from ambient radiation in the jet and from the extragalactic background light (EBL), is taken into account. Results are presented as a function of a small set of parameters: the Doppler factor, the observed variability timescale, the comoving magnetic field, the peak synchrotron flux, and the redshift of the burst. Model predictions will be tested by multiwavelength observations, including the Swift and GLAST satellites, which will provide unprecedented coverage of GRBs.
OSTI ID:
21137201
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1000; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English

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