On a Penrose Inequality with Charge Gilbert Weinstein and Sumio Yamada
نویسنده
چکیده
We construct a time-symmetric asymptotically flat initial data set to the Einstein-Maxwell Equations which satisfies m− 1 2 ( R+ Q R ) < 0, where m is the total mass, R = √ A/4π 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 for charged black holes.
منابع مشابه
Extensions of the charged Riemannian Penrose inequality
In this paper we investigate the extension of the charged Riemannian Penrose inequality to the case where charges are present outside the horizon. We prove a positive result when the charge densities are compactly supported, and present a counterexample when the charges extend to infinity. We also discuss additional extensions to other matter models.
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Sergio Dain,* Marcus Khuri, Gilbert Weinstein, and Sumio Yamada Facultad de Matemática, Astronomı́a y Fı́sica, FaMAF, Universidad Nacional de Córdoba, Instituto de Fı́sica Enrique Gaviola, IFEG, CONICET, Ciudad Universitaria, 5000 Córdoba, Argentina Department of Mathematics, Stony Brook University, Stony Brook, New York 11794, USA Department of Physics; Department of Computer Science and Mathemat...
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