Accuracy and Efficiency of Raytracing Photoionisation Algorithms

Details Accuracy and Efficiency of Raytracing Photoionisation Algorithms Accuracy and Efficiency of Raytracing Photoionisation Algorithms

2012-01-26

arxiv.org/abs/1201.5651v2

Astronomy & Astrophysics, 2012, 539, A147

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

14 pages, minor updates to match published version

Scientific paper

10.1051/0004-6361/201117984

Three non-equilibrium photoionisation algorithms for hydrodynamical grid-based simulation codes are compared in terms of accuracy, timestepping criteria, and parallel scaling. Explicit methods with first-order time accuracy for photon conservation must use very restrictive timestep criteria to accurately track R-type ionisation fronts. A second-order accurate algorithm is described which, although it requires more work per step, allows much longer timesteps and is consequently more efficient. Implicit methods allow ionisation fronts to cross many grid cells per timestep while maintaining photon conservation accuracy. It is shown, however, that errors are much larger for multi-frequency radiation than for monochromatic radiation with the implicit algorithm used here, and large errors accrue when an ionisation front crosses many optical depths in a single step. The accuracy and convergence rates of the different algorithms are tested with a large number of timestepping criteria to identify the best criterion for each algorithm. With these criteria selected, the second-order explicit algorithm is the most efficient of the three, and its parallel scaling is significantly better than that of the implicit algorithm. The upgrade from first- to second-order accuracy in explicit algorithms could be made very simply to fixed-grid and adaptive mesh-refinement codes which currently use a first-order method.

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