Relativistic Fluid Mechanics

@article{Taub1978RelativisticFM,
  title={Relativistic Fluid Mechanics},
  author={A. H. Taub},
  journal={Annual Review of Fluid Mechanics},
  year={1978},
  volume={10},
  pages={301-332}
}
  • A. Taub
  • Published 1978
  • Physics
  • Annual Review of Fluid Mechanics
fluid mechanics may be characterized as a theory that describes the state of a fluid by means of five functions of at most four independent variables. The latter variables are of two kinds: three variables determining a point in a three­ dimensional Euclidean space and a fourth one labeling absolute time on some sta ndard universal clock. The five functions, the dependent variables of the theory, are also of two kinds: three of them are kinematic variables, vi (i = 1,2,3), the 
A Relativistic Model of Fluids Motion
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Two explicit solutions in a reducible relativistic system
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On the classical and quantum irrotational motions of a relativistic perfect fluid I. Classical theory
  • S. Matarrese
  • Physics, Mathematics
    Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences
  • 1985
Some aspects of perfect-fluid general-relativistic hydrodynamics under the assumptions of irrotationality and isentropicity are analysed. A new derivation of the known fact that the Lagrangian for
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Thermodynamical equilibrium and spacetime geometry
In relativistic theory of irreversible thermodynamical processes near equilibrium, generally a series of assumptions is made having, in particular, the consequence that the temperature vector is a
Poisson type relativistic perfect fluid spheres
Static spherically symmetric solutions of the Einstein's field equations in isotropic coordinates representing perfect fluid matter distributions from Newtonian potential-density pairs are
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References

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