The Escape of High-Energy Photons from Gamma-Ray Bursts

Abstract

Eleven bright gamma-ray bursts (GRBs) detected by BATSE have also been seen at much higher energies by EGRET, six at energies above 10 MeV. Such observations imply that these bursts are optically thin to photon-photon pair production at all observed energies. For bursts more than about 30pc away, internal transparency can be achieved only if the source is moving with a relativistic bulk Lorentz factor $\Gamma\gg 1$, or if the radiation is highly beamed. Early calculations of $\gamma\gamma\to e^+e^-$ considerations for GRBs were limited to cases of a beam with opening half-angle $\Thetab\sim 1/\Gamma$, or expansions of infinitely thin spherical shells. This paper presents our extension of pair production optical depth calculations in relativistically expanding sources to more general geometries, including shells of finite thickness and arbitrary opening angle. The problem is reduced analytically to a single integral in the broadly applicable case of observing photons along the axis of the expansion. We find that the minimum bulk Lorentz factor for the EGRET sources to be optically thin is only moderately dependent on the shell thickness and virtually independent of its opening solid angle if $\Thetab\gtrsim 1/\Gamma$. This insensitivity to $\Thetab$ relieves the commonly-perceived number problem for non-repeating sources at cosmological distances, i.e. it is not necessary to invoke small $\Thetab$ to effect photon escape.