Abstract
We show that the area-angular-momentum inequality holds for axially symmetric closed outermost stably marginally trapped surfaces. These are horizon sections (in particular, apparent horizons) contained in otherwise generic non-necessarily axisymmetric black hole spacetimes, with a non-negative cosmological constant and whose matter content satisfies the dominant energy condition.
- Received 30 June 2011
DOI:https://doi.org/10.1103/PhysRevD.84.121503
© 2011 American Physical Society