3 - D Relativistic SPH


In this paper we present the equations and some basic applications of relativistic SPH. The equations are generated under the assumption that there are no interaction terms between the fluid modelled and the background space-time, i.e. we are neglecting the perturbations to the metric produced by the modelled fluid. This corresponds to a stationary metric… (More)


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@inproceedings{Muir20033D, title={3 - D Relativistic SPH}, author={S. Muir and Jacqueline Monaghan}, year={2003} }