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Focusing on the numerical aspects and accuracy we study a class of bulkviscosity driven expansion scenarios using the relativistic Navier-Stokes andtruncated Israel-Stewart form of the equations of relativistic dissipativefluids in 1+1 dimensions. The numerical calculations of conservation andtransport equations are performed using the numerical framework of fluxcorrected transport. We show that the results of the Israel-Stewart causalfluid dynamics are numerically much more stable and smoother than the resultsof the standard relativistic Navier-Stokes equations.

european physical journal. c, particles and fields

Comparing the first and second order theories of relativistic  dissipative fluid dynamics using the 1+1 dimensional relativistic flux  corrected transport algorithm