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Gamma-ray burst models with general dynamics and fits to Fermi LAT bursts

We present a dissipative photospheric model for gamma-ray bursts where the usual Band peak around MeV energies arises as synchrotron emission from around the photosphere. We treat the initial acceleration in a general way and the GeV emission arises as the interaction of photospheric radiation and the shocked electrons at the deceleration radius. We show some applications of this model.

preprint2013arXivOpen access
Péter VeresPéter MészárosBin-Bin Zhang
astro-ph.HE
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Open access3 authors1 topic
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Péter VeresPéter MészárosBin-Bin Zhang

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