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Cosmological Models

Cargèse Lectures 1998
  • George F. R. Ellis
  • Henk Van Elst
Part of the NATO Science Series book series (ASIC, volume 541)

Abstract

The aim of this set of lectures is a systematic presentation of a 1 + 3 covariant approach to studying the geometry, dynamics, and observational properties of relativistic cosmological models. In giving (i) the basic 1+ 3 covariant relations for a cosmological fluid, the present lectures cover some of the same ground as a previous set of Cargèse lectures [7], but they then go on to give (ii) the full set of corresponding tetrad equations, (iii) a classification of cosmological models with exact symmetries, (iv) a brief discussion of some of the most useful exact models and their observational properties, and (v) an introduction to the gauge-invariant and 1 + 3 covariant perturbation theory of almost-Friedmann—LemaîtreRobertson—Walker universes, with a fluid description for the matter and a kinetic theory description of the radiation.

Keywords

Perfect Fluid Weyl Tensor Bianchi Type Past Light Cone Real Universe 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media Dordrecht 1999

Authors and Affiliations

  • George F. R. Ellis
    • 1
  • Henk Van Elst
    • 1
  1. 1.Cosmology Group Department of Mathematics and Applied MathematicsUniversity of Cape TownCape TownSouth Africa

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