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gr-qcJan 1, 2007
authors
  • Istvan Racz
arXiv abstractPDF
paper

A New Way of Proving Black Hole Rigidity

arXiv:gr-qc/0701103

Abstract

This paper has been withdrawn.

This paper has been withdrawn

References in corpus (3)

  • A Higher Dimensional Stationary Rotating Black Hole Must be Axisymmetric
  • Stationary Black Holes as Holographs
  • Conditions for nonexistence of static or stationary, Einstein-Maxwell, non-inheriting black-holes
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