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On a Penrose Inequality with Charge

Gilbert Weinstein·Sumio Yamada
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Abstract

We construct a time-symmetric asymptotically flat initial data set to the Einstein-Maxwell Equations which satisfies the inequality: m - 1/2(R + Q^2/R) < 0, where m is the total mass, R=sqrt(A/4) is the area radius of the outermost horizon and Q is the total charge. This yields a counter-example to a natural extension of the Penrose Inequality to charged black holes.

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Gilbert Weinstein, Sumio Yamada. 2005-02-16. On a Penrose Inequality with Charge. https://doi.org/10.1007/s00220-005-1355-0

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