Inverse Compton scattering in a strong magnetic field and the spectrum of gamma-ray bursts

Details Inverse Compton scattering in a strong magnetic field and the spectrum of gamma-ray bursts Inverse Compton scattering in a strong magnetic field and the spectrum of gamma-ray bursts

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cha%26a..17..136z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 17, Issue 2, p. 136-143.

Astronomy and Astrophysics

Astrophysics

Γ Ray Burst-Radiation Mechanism-Inverse Compton Scattering

Scientific paper

We believe that inverse Compton scattering in strong magnetic field may be the main emission mechanism of γ ray bursts. Protons in the source region generate low-frequency photons which, through Compton scattering by nonthermal electrons in a strong magnetic field, gives rise to the spectrum. Using the Compton scattering cross section under a strong magnetic field in the non-relativistic case (B/Bcr << 1, hνi/mec2 << 1), we have successfully fitted the observed spectrum of typical burst GB 811016.

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