P. Veres, B. -B. Zhang, P. Mészáros
The Fermi observations of GRB 110721A (The Fermi LAT Collaboration et al. 2012) have revealed an unusually high peak energy $\sim 15$ MeV in the first time bin of the prompt emission. We find that an interpretation is unlikely in terms of internal shock models, and confirm that a standard black-body photospheric model also falls short. We show that dissipative photospheric synchrotron models, on the other hand, are able to accommodate such high peak values.
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http://arxiv.org/abs/1208.1790
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