Abstract
We review the evolution of the numerical techniques applied in relativistic hydrodynamics since the sixties until today. We focus our attention on the state-of- the-art high-resolution shock-capturing methods and the astrophysical applications involving three-dimensional simulations.
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Aloy, M.A., Martí, J.M. (2002). 3D Relativistic Hydrodynamics. In: Guthmann, A.W., Georganopoulos, M., Manolakou, K., Marcowith, A. (eds) Relativistic Flows in Astrophysics. Lecture Notes in Physics, vol 589. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-46025-X_9
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