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We show how causal relativistic Navier-Stokes equations arise from the relativistic Boltzmann equation: the causality is preserved via a judicious choice of the zero modes of the collision operator.
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2008
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F.S. Bemfica, M.M. Disconzi and J. Noronha, General-Relativistic Viscous Fluid Dynamics , 2009.11388
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J. Erdmenger, M. Haack, M. Kaminski and A. Yarom, Fluid dynamics of R-charged black holes , JHEP 01
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2018
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2021
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2021
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