arXiv · 1106.3743
Black hole Area-Angular momentum inequality in non-vacuum spacetimes
Abstract
We show that the area-angular momentum inequality A\geq 8\pi|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.
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José Luis Jaramillo, Martín Reiris, Sergio Dain. 2011-06-19. Black hole Area-Angular momentum inequality in non-vacuum spacetimes. https://doi.org/10.1103/physrevd.84.121503
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