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Radiation Processes in GRBs. Prompt Emission

Mikhail V. Medvedev

astro-pharXiv:astro-ph/0410490

Abstract

A substantial fraction of prompt GRB spectra have soft spectral indexes exceeding the maximum allowed by the synchrotron model alphamax=-2/3. Some spectra also exhibit very sharp break at Ep, inconsistent with the smooth synchrotron spectra. These facts pose a serious problem for the ``optically thin synchrotron'' interpretation of the prompt emission. We review various models suggested in order to resolve this puzzle.

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