Abstract
We present a nonperturbative proof of the no-hair theorems corresponding to scalar and Proca fields for stationary axisymmetric de Sitter black hole spacetimes. Our method also applies to asymptotically flat and under a reasonable assumption, to asymptotically anti-de Sitter spacetimes.
- Received 1 February 2011
DOI:https://doi.org/10.1103/PhysRevD.83.124017
© 2011 American Physical Society