Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-11-24
Astrophys.J.693:1637-1644,2009
Astronomy and Astrophysics
Astrophysics
16 pages, 10 figures, accepted for publication in The Astrophysical Journal
Scientific paper
10.1088/0004-637X/693/2/1637
In the dynamic diffusion limit of radiation hydrodynamics, advection dominates diffusion; the latter primarily affects small scales and has negligible impact on the large scale flow. The radiation can thus be accurately regarded as an ideal fluid, i.e., radiative diffusion can be neglected along with other forms of dissipation. This viewpoint is applied here to an analysis of simple waves in an ideal radiating fluid. It is shown that much of the hydrodynamic analysis carries over by simply replacing the material sound speed, pressure and index with the values appropriate for a radiating fluid. A complete analysis is performed for a centered rarefaction wave, and expressions are provided for the Riemann invariants and characteristic curves of the one-dimensional system of equations. The analytical solution is checked for consistency against a finite difference numerical integration, and the validity of neglecting the diffusion operator is demonstrated. An interesting physical result is that for a material component with a large number of internal degrees of freedom and an internal energy greater than that of the radiation, the sound speed increases as the fluid is rarefied. These solutions are an excellent test for radiation hydrodynamic codes operating in the dynamic diffusion regime. The general approach may be useful in the development of Godunov numerical schemes for radiation hydrodynamics.
No associations
LandOfFree
Simple Waves in Ideal Radiation Hydrodynamics does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Simple Waves in Ideal Radiation Hydrodynamics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Simple Waves in Ideal Radiation Hydrodynamics will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-645818