Non-equilibrium effects in steady relativistic $e^+e^-γ$ winds

Ole M. Grimsrud; Ira Wasserman

doi:10.1046/j.1365-8711.1998.02004.x

paper

Non-equilibrium effects in steady relativistic $e^{+} e^{-} γ$ winds

arXiv:astro-ph/9805138 · doi:10.1046/j.1365-8711.1998.02004.x

Abstract

We consider an ultra-relativistic wind consisting of electron-positron pairs and photons with the principal goal of finding the asymptotic Lorentz factor $γ_{\infty}$ for zero baryon number. The wind is assumed to originate at radius $r_{i}$ where it has a Lorentz factor $γ_{i}$ and a temperature $T_{i}$ sufficiently high to maintain pair equilibrium. As $r$ increases, $T$ decreases and becomes less than the temperature corresponding to the electron mass $m_{e}$ , after which non-equilibrium effects become important. Further out in the flow the optical depth $τ$ drops below one, but the pairs may still be accelerated by the photons until $τ$ falls below $\sim 2 \times 1 0^{- 5} γ_{i}^{3/4}$ . Radiative transfer calculations show that only at this point do the radiation flux and pressure start to deviate significantly from their blackbody values. The acceleration of the pairs increases $γ$ by a factor $\sim 45$ as compared to its value at the photosphere; it is shown to approach $γ_{\infty} \sim 1.4\times 10^3 (r_i/10^6\mbox{cm})^{1/4} γ_{i}^{3/4} T_i/m_e$.

41 pages, 9 figures. Submitted to MNRAS

Non-equilibrium effects in steady relativistic e+e−γ winds

Abstract

Cited by in corpus (27)

Non-equilibrium effects in steady relativistic $e^{+} e^{-} γ$ winds