Journal
EUROPEAN PHYSICAL JOURNAL C
Volume 60, Issue 3, Pages 413-429Publisher
SPRINGER
DOI: 10.1140/epjc/s10052-009-0927-0
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Focusing on the numerical aspects and accuracy we study a class of bulk viscosity driven expansion scenarios using the relativistic Navier-Stokes and truncated Israel-Stewart form of the equations of relativistic dissipative fluids in 1+1 dimensions. The numerical calculations of conservation and transport equations are performed using the numerical framework of flux corrected transport. We show that the results of the Israel-Stewart causal fluid dynamics are numerically much more stable and smoother than the results of the standard relativistic Navier-Stokes equations.
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