Numerical tests of causal relativistic dissipative fluid dynamics
E. Moln\'ar, H. Niemi, D. H. Rischke

TL;DR
This paper develops and tests numerical methods for solving the Israel-Stewart equations of causal relativistic dissipative fluid dynamics, focusing on the Riemann problem in multiple dimensions, with applications to realistic 3+1D modeling.
Contribution
The paper introduces numerical schemes for Israel-Stewart equations and demonstrates their effectiveness through multidimensional Riemann problem tests.
Findings
Numerical methods successfully solve 1+1 and 2+1 dimensional Riemann problems.
Schemes are applicable to realistic 3+1 dimensional relativistic fluid simulations.
Results support the stability and accuracy of the proposed numerical approaches.
Abstract
We present numerical methods to solve the Israel-Stewart (IS) equations of causal relativistic dissipative fluid dynamics with bulk and shear viscosities. We then test these methods studying the Riemann problem in (1+1)-- and (2+1)-dimensional geometry. The numerical schemes investigated here are applicable to realistic (3+1)--dimensional modeling of a relativistic dissipative fluid.
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