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

Entropy Manifold Vorticity Eter Sine 

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Copyright information

© Springer-Verlag Berlin Heidelberg 2004

Authors and Affiliations

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

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