Black hole Area-Angular momentum inequality in non-vacuum spacetimes

Details Black hole Area-Angular momentum inequality in non-vacuum spacetimes Black hole Area-Angular momentum inequality in non-vacuum spacetimes

2011-06-19

arxiv.org/abs/1106.3743v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages, no figures, updated to match published version

Scientific paper

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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