Radiative mechanisms in GRB prompt emission

Research output: Contribution to journalConference articlepeer-review


Motivated by the Fermi gamma-ray space telescope results, in recent years immense efforts were given to understanding the mechanism that leads to the prompt emission observed. The failure of the optically thin emission models (synchrotron and synchrotron self Compton) increased interest in alternative models. Optically thick models, while having several advantages, also face difficulty in capturing several key observables. Theoretical efforts are focused in two main directions: (1) mechanisms that act to broaden the Planck spectrum; and (2) combining the optically thin and optically thick models to a hybrid model that could explain the key observables.

Original languageEnglish
Pages (from-to)105-113
Number of pages9
JournalEAS Publications Series
StatePublished - 2013
Externally publishedYes
Event2012 Gamma-Ray Burst Symposium, GRB 2012 - Malaga, Spain
Duration: 8 Oct 201212 Oct 2012


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