Does the Prompt γ-Ray Emission of Gamma-Ray Bursts Arise from Resonant Inverse Compton Scattering?

Details Does the Prompt γ-Ray Emission of Gamma-Ray Bursts Arise from Resonant Inverse Compton Scattering? Does the Prompt γ-Ray Emission of Gamma-Ray Bursts Arise from Resonant Inverse Compton Scattering?

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008apj...680..539c&link_type=abstract

The Astrophysical Journal, Volume 680, Issue 1, pp. 539-544.

Astronomy and Astrophysics

Astronomy

4

Gamma Rays: Bursts, Methods: Analytical, Radiation Mechanisms: Nonthermal, Stars: Neutron

Scientific paper

We argue that the dominant radiation mechanism responsible for the early prompt γ-ray emission of gamma-ray bursts could be the resonant inverse Compton scattering of relativistic electrons in an intense magnetic field. By using this mechanism, some problems in the field of gamma-ray bursts could be clarified, e.g., the origin of the Amati relation, the formation of the observed broken power-law spectra, and the related deadline problem, among others. Our model also predicts that the emitted γ-rays could be highly polarized.

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