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Viscous phenomena in cosmology

Author

Listed:
  • Van Leeuwen, W.A.
  • Salvati, G.A.Q.
  • Schelling, E.E.

Abstract

The six viscosity coefficients characterizing a magnetized pe- γ-plasma are calculated on the basis of relativistic kinetic theory.

Suggested Citation

  • Van Leeuwen, W.A. & Salvati, G.A.Q. & Schelling, E.E., 1986. "Viscous phenomena in cosmology," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 136(2), pages 417-431.
    • Handle: RePEc:eee:phsmap:v:136:y:1986:i:2:p:417-431
    DOI: 10.1016/0378-4371(86)90259-1
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    References listed on IDEAS

    as
    1. van Erkelens, H., 1981. "Relativistic Boltzmann theory for a plasma," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 107(1), pages 48-70.
    2. Van Erkelens, H. & Van Leeuwen, W.A., 1980. "Relativistic Boltzmann-theory for a plasma," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 101(1), pages 205-222.
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    Cited by:

    1. Hageman, T. & van Leeuwen, W.A., 1987. "Viscous Bianchi type II universes with intergalactic magnetic field," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 146(3), pages 506-524.

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