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General Relativity and Gravitation

, Volume 24, Issue 10, pp 1069–1081 | Cite as

The Oppenheimer-Snyder space-time with a cosmological constant

  • Ken-ichi Nakao
Research Articles

Abstract

We investigate the Oppenheimer-Snyder space-time with a positive cosmological constant A. The interior of the dust sphere is described by the closed Friedmann-Robertson-Walker space-time while the exterior is the Schwarzschild-de Sitter space-time. Due to the cosmological constant A, when the gravitational massMo of the dust sphere is very large, there is no collapsing solution with the de Sitter-like asymptotic region which expands exponentially in the expanding universe frame. This fact suggests that the very large initial inhomogeneity does not necessarily lead to the failure of the cosmic no hair conjecture.

Keywords

Dust Cosmological Constant Differential Geometry Asymptotic Region Positive Cosmological Constant 
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

© Plenum Publishing Corporation 1992

Authors and Affiliations

  • Ken-ichi Nakao
    • 1
  1. 1.Department of PhysicsKyoto UniversityKyotoJapan

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