Abstract
We present a new approach to doing Eulerian computational fluid dynamics that is designed to work at high Mach numbers encountered in hydrodynamical simulations of the IGM. In conventional Eulerian CFD, the thermal energy is poorly tracked in supersonic bulk flows where local fluid variables cannot be accurately separated from the much larger bulk flow components. We describe a method in which local quantities can be directly tracked and the Eulerian fluid equations solved in a local frame moving with the flow. The new algorithm has been used to run large hydrodynamical simulations on a 10243 grid to study the kinetic SZ effect. The KSZ power spectrum is broadly peaked at l ∼ 104 with temperature fluctuations ∼ 1μK.
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Trac, H., Zhang, P., Pen, U. (2003). Hydrodynamical Simulations of the IGM at High Mach Numbers. In: Rosenberg, J.L., Putman, M.E. (eds) The IGM/Galaxy Connection. Astrophysics and Space Science Library, vol 281. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0115-1_12
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DOI: https://doi.org/10.1007/978-94-010-0115-1_12
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3978-9
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