Spectral modeling of GRB pulses

Details Spectral modeling of GRB pulses Spectral modeling of GRB pulses

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..526..441p&link_type=abstract

GAMMA-RAY BURSTS: 5th Huntsville Symposium. AIP Conference Proceedings, Volume 526, pp. 441-445 (2000).

Computer Science

Gamma-Ray Sources, Gamma-Ray Bursts, Cosmic Rays, Jets And Bursts, Galactic Winds And Fountains

Scientific paper

The energy spectra of pulses of GRBs are modeled for synchrotron and multiple self-inverse Compton scattering from a population of thermal and non-thermal electrons. The contribution from pairs that result from annihilation is also taken into account. A high particle density (enhanced by the pairs) will increase absorption but, if the pairs are not accelerated, the absorption frequency cannot lie in the BATSE window. Pairs will contribute in upscattering and will most likely increase the population of cold particles that will downscatter hard photons and thus suppress hard (e.g., above 300 keV) emission. .

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