Horizon area-angular momentum inequality in higher dimensional spacetimes
arXiv:1110.5814 · doi:10.1088/0264-9381/29/6/065006
Abstract
We consider -dimensional spacetimes which are axisymmetric--but not necessarily stationary (!)--in the sense of having isometry group , and which satisfy the Einstein equations with a non-negative cosmological constant. We show that any black hole horizon must have area $A \ge 8π|J_+ J_-|^\half$, where are distinguished components of the angular momentum corresponding to linear combinations of the rotational Killing fields that vanish somewhere on the horizon. In the case of , where there is only one angular momentum component , we recover an inequality of 1012.2413 [gr-qc]. Our work can hence be viewed as a generalization of this result to higher dimensions. In the case of with horizon of topology , the quantities are the same angular momentum component (in the direction). In the case of with horizon topology , the quantities are the distinct components of the angular momentum. We also show that, in all dimensions, the inequality is saturated if the metric is a so-called ``near horizon geometry''. Our argument is entirely quasi-local, and hence also applies e.g. to any stably outer marginally trapped surface.
16 pages, Latex, no figures
References in corpus (4)
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