Does the prompt γ-ray emission of GRB arise from RICS?

Details Does the prompt γ-ray emission of GRB arise from RICS? Does the prompt γ-ray emission of GRB arise from RICS?

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1065..211l&link_type=abstract

2008 NANJING GAMMA-RAY BURST CONFERENCE. AIP Conference Proceedings, Volume 1065, pp. 211-217 (2008).

Computer Science

Gamma-Ray Sources, Gamma-Ray Bursts, Radiation Detectors, Interactions Of Particles And Radiation With Matter, Neutron Stars

Scientific paper

We argue that the dominant radiation mechanism responsible for the early prompt γ-rayemission of gamma-ray bursts could be the resonant inverse Compton scattering(RICS) of relativistic electrons in an intense magnetic field. By using this mechanism, some problems in the GRB study 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,'' the solution of the ``compactness problem,'' etc.. Our model also predicts that the emitted γ-rayscould be highly polarized.

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