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Some cylindrically-symmetric cosmological models in general relativity representing viscous fluid and perfect fluid with heat conduction

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Publication:1114565
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DOI10.1007/BF00641717zbMath0662.76154MaRDI QIDQ1114565

S. H. Smith

Publication date: 1988

Published in: Astrophysics and Space Science (Search for Journal in Brave)


zbMATH Keywords

Einstein's field equationsinhomogeneous space-timesperfect fluid with heat conductiontwo-parameter group of motions


Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)


Related Items (3)

Bulk viscous L.R.S. Bianchi type V tilted stiff fluid cosmological model in general relativity ⋮ Tilted LRS Bianchi type-I mesonic stiff fluid cosmological model ⋮ LRS Bianchi type II tilted barotropic fluid cosmological model with heat conduction in general relativity



Cites Work

  • Topology and cosmology
  • Isentropic Hydrodynamics in Plane Symmetric Space-Times
  • Empty space-times admitting a three parameter group of motions


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