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Rotating Black Holes

  • Norbert Straumann
Part of the Texts and Monographs in Physics book series (TMP)

Abstract

All stars rotate more or less rapidly. When a horizon is formed during gravitational collapse, a Schwarzschild black hole is thus never produced. One expects, however, that the horizon will quickly settle down to a stationary state as a result of the emission of gravitational waves. The geometry of the stationary black hole is of course no longer spherically symmetric.

Keywords

Black Hole Static Limit Gravitational Wave Trap Surface Kerr Solution 
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-Verlag Berlin Heidelberg 1984

Authors and Affiliations

  • Norbert Straumann
    • 1
  1. 1.Institut für Theoretische PhysikUniversität ZürichZürichSwitzerland

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