The photospheric radiation model for the prompt emission of Gamma-ray Bursts: Interpreting four observed correlations
arXiv:1204.4881 · doi:10.1088/2041-8205/755/1/L6
Abstract
We show that the experiential , , and correlations (where is the time-averaged luminosity of the prompt emission, is the spectral peak energy, is the bulk Lorentz factor and is the emission efficiency of Gamma-ray bursts) are well consistent with the relations between the resembling parameters predicted in the photospheric radiation model of the prompt emission of Gamma-ray bursts. The time-resolved thermal radiation of GRB 090902B does follow the and correlations. A reliable interpretation of the four correlations in alternative models is still lacking. These facts may point towards a photospheric origin of prompt emission of some Gamma-ray Bursts.
9 pages, 1 figure, accepted for publication in ApJL
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