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25 April 2024
 
  » arxiv » 1507.5621

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StarBench: The D-type expansion of an HII region
T.G. Bisbas ; T.J. Haworth ; R.J.R. Williams ; J. Mackey ; P. Tremblin ; A.C. Raga ; S.J. Arthur ; C. Baczynski ; J.E. Dale ; T. Frostholm ; S. Geen ; T. Haugboelle ; D. Hubber ; I.T. Iliev ; R. Kuiper ; J. Rosdahl ; D. Sullivan ; S. Walch ; R. Wuensch ;
Date 20 Jul 2015
AbstractStarBench is a project focused on benchmarking and validating different star-formation and stellar feedback codes. In this first StarBench paper we perform a comparison study of the D-type expansion of an HII region. The aim of this work is to understand the differences observed between the twelve participating numerical codes against the various analytical expressions examining the D-type phase of HII region expansion. To do this, we propose two well-defined tests which are tackled by 1D and 3D grid- and SPH- based codes. The first test examines the ’early phase’ D-type scenario during which the mechanical pressure driving the expansion is significantly larger than the thermal pressure of the neutral medium. The second test examines the ’late phase’ D-type scenario during which the system relaxes to pressure equilibrium with the external medium. Although they are mutually in excellent agreement, all twelve participating codes follow a modified expansion law that deviates significantly from the classical Spitzer solution in both scenarios. We present a semi-empirical formula combining the two different solutions appropriate to both early and late phases that agrees with high-resolution simulations to $lesssim2\%$. This formula provides a much better benchmark solution for code validation than the Spitzer solution. The present comparison has validated the participating codes and through this project we provide a dataset for calibrating the treatment of ionizing radiation hydrodynamics codes.
Source arXiv, 1507.5621
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