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The Relaxation Effect in Dissipative Relativistic Fluid Theories

General Relativity and Quantum Cosmology 2009-10-28 v1

Abstract

The dynamics of the fluid fields in a large class of causal dissipative fluid theories is studied. It is shown that the physical fluid states in these theories must relax (on a time scale that is characteristic of the microscopic particle interactions) to ones that are essentially indistinguishable from the simple relativistic Navier-Stokes descriptions of these states. Thus, for example, in the relaxed form of a physical fluid state the stress energy tensor is in effect indistinguishable from a perfect fluid stress tensor plus small dissipative corrections proportional to the shear of the fluid velocity, the gradient of the temperature, etc.

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Cite

@article{arxiv.gr-qc/9508058,
  title  = {The Relaxation Effect in Dissipative Relativistic Fluid Theories},
  author = {Lee Lindblom},
  journal= {arXiv preprint arXiv:gr-qc/9508058},
  year   = {2009}
}

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