1996/10/09 by Piotr T. Chruściel
Physics and Astronomy · #gr-qc
published as Helv.Phys.Acta 69 (1996) 529-552 · 24 pages, latex with amsfonts
arxiv created 1996/10/09 · arxiv updated 2009/11/30
In recent years there has been some progress in the understanding of the global structure of stationary black hole space-times. In this paper we review some new results concerning the structure of stationary black hole space-times. In particular we prove a corrected version of the ``black hole rigidity theorem'', and we prove a uniqueness theorem for static black holes with degenerate connected horizons. This paper is an expanded version of a lecture given at the Journées relativistes in Ascona, May 1996.