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Energy Distribution of Black Plane Solutions

Paul Halpern
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Abstract

We use the Einstein energy-momentum complex to calculate the energy distribution of static plane-symmetric solutions of the Einstein-Maxwell equations in 3+1 dimensions with asymptotic anti-de Sitter behavior. This solution is expressed in terms of three parameters: the mass, electric charge and cosmological constant. We compare the energy distribution to that of the Reissner-Nordstrom-anti-de Sitter solution, pointing to qualitative differences between the models. Finally, we examine these results within the context of the Cooperstock hypothesis.

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Paul Halpern. 2006-03-27. Energy Distribution of Black Plane Solutions. https://doi.org/10.1142/s0217732306019748

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