Physics
Scientific paper
Feb 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..555..461d&link_type=abstract
Cosmology and Particle Physics: CAPP 2000. AIP Conference Proceedings, Volume 555, pp. 461-464 (2001).
Physics
Gamma-Ray Sources, Gamma-Ray Bursts, Radiation Mechanisms, Polarization
Scientific paper
The spectra of Gamma-Ray Burst (GRB) emission have been investigated theoretically by a number of authors (e.g., [1-3]) for different versions of a general fireball-shock scenario [4,5]. However, the existing analytical works give rather coarse predictions and suffer from many uncertainties. We develop a refined analytical model of synchrotron-self-Compton emission, in which we take into account both synchrotron and inverse Compton cooling of relativistic electrons. The principal role of Klein-Nishina cut-off is shown. We discuss the delay of inverse Compton (IC) component of GRB emission with respect to sub-MeV radiation and describe its energy dependence. .
Derishev Evgeny V.
Kocharovsky Vitaly V.
Kocharovsky Vl. V.
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