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Annali di Matematica Pura ed Applicata

, Volume 98, Issue 1, pp 239–255 | Cite as

Model universes with spherical symmetry

  • J. L. Synge
Article

Summary

Spherically symmetric universes are defined, and spherically symmetric solutions of Einstein's field equations in vacuo are explored in terms of suitable coordinates. The Kruskal metric is thus obtained in a systematic way, with possibilities of generalisation.

Keywords

Field Equation Spherical Symmetry Symmetric Solution Symmetric 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.

Bibliografia

  1. (1).
    M. D. Kruskal, Phys. Rev.,119 (1960), p. 1743, where references will be found to earlier work by others. See alsoS. Mavridès,L'univers relativiste, Masson (Paris, 1973), p. 338.CrossRefzbMATHMathSciNetGoogle Scholar
  2. (1).
    In respect to signs, the Riemann tensor and the Ricci tensor are defined as inJ. L. Synge,Relativity: the General Theory, North-Holland, Amsterdam 1964, pp. 15–17.Google Scholar

Copyright information

© Nicola Zanichelli Editore 1974

Authors and Affiliations

  • J. L. Synge
    • 1
  1. 1.Dublin

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