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SPH Radiative Hydrodynamics Methods

Published online by Cambridge University Press:  27 April 2011

Hajime Susa
Hajime Susa*
Affiliation:
Departiment of Physics, Konan University, Kobe, Japan email: susa@konan-u.ac.jp
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Abstract

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In this paper, we review the radiative hydrodynamics methods based upon Smoothed Particle Hydrodynamics(SPH). There are already various implementations so far, which can be categorized into three types: moment equation solvers, Monte Carlo methods, and ray-tracing schemes. These codes have been applied to various astrophysical problems including dynamics of dense proto-stellar cores, photoionization feedback of massive stars on molecular clouds, radiative feedback in the early universe, etc. Among these different methods, we focus on the ray-tracing schemes. We also describe one particular ray-tracing code RSPH in some details.

Keywords

methods: numericalradiative transferhydrodynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S270: Computational Star Formation , May 2010 , pp. 195 - 202
Copyright
Copyright © International Astronomical Union 2011

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