Black hole Area-Angular momentum inequality in non-vacuum spacetimes
arXiv:1106.3743 · doi:10.1103/PhysRevD.84.121503
Abstract
We show that the area-angular momentum inequality A\geq 8π|J| 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 non-negative cosmological constant and whose matter content satisfies the dominant energy condition.
5 pages, no figures, updated to match published version
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