Monte Carlo simulations of the photospheric emission in GRBs

Abstract

We studied the decoupling of photons from ultra-relativistic spherically symmetric outflows expanding with constant velocity by means of Monte-Carlo (MC) simulation. For outflows with finite width we confirm the existence of two regimes: photon thick and photon thin introduced recently by Ruffini, Siutsou, Vereshchagin (2011), hereafter RSV. The probability density function of photon last scattering is shown to be very different in these two cases. We also obtained spectra as well as light curves. In photon thick case, the time integrated spectrum is much broader than the Planck function and its shape is well described by the fuzzy photosphere approximation introduced by RSV. In the photon thin case we confirm the crucial role of photon diffusion, hence the probability density of decoupling has a maximum near the diffusion radius, well below the photosphere. Its spectrum has Band shape. It is produced when the outflow is optically thick and its peak is formed at diffusion radius.

6 pages, 9 figures, accepted to ApJ. Correction of typos in formulae 4 and 7

References in corpus (3)

• Temporal Evolution Of Thermal Emission From Relativistically Expanding Plasma
• Quasi-blackbody component and radiative efficiency of the prompt emission of gamma-ray bursts
• The Blackholic energy and the canonical Gamma-Ray Burst IV: the "long", "genuine short" and "fake - disguised short" GRBs

Cited by in corpus (5)

• Poynting flux dominated jets challenged by their photospheric emission
• Spectral and Polarization Properties of Photospheric Emission From Stratified Jets
• Emission from accelerating jets in gamma-ray bursts: Radiation dominated flows with increasing mass outflow rates
• Testing a model for subphotospheric dissipation in GRBs: fits to Fermi data constrain the dissipation scenario
• Random walks and effective optical depth in relativistic flow