Viscous Boundary Layers of Radiation-dominated, Relativistic Jets. I. The Two-stream Model
Abstract
Using the relativistic equations of radiation hydrodynamics in the viscous limit, we analyze the boundary layers that develop between radiation-dominated jets and their environments. In this paper we present the solution for the self-similar, 2D, plane-parallel two-stream problem, wherein the jet and the ambient medium are considered to be separate, interacting fluids, and we compare our results to those of previous authors. (In a companion paper we investigate an alternative scenario, known as the free-streaming jet model.) Consistent with past findings, we show that the boundary layer that develops between the jet and its surroundings creates a region of low-density material. These models may be applicable to sources such as super-Eddington tidal disruption events and long gamma-ray bursts.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- August 2015
- DOI:
- arXiv:
- arXiv:1506.08824
- Bibcode:
- 2015ApJ...809....1C
- Keywords:
-
- galaxies: jets;
- gamma-ray burst: general;
- radiation: dynamics;
- relativistic processes;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 9 pages, 6 figures, paper II to appear tomorrow. Accepted for publication in ApJ