Energy Distribution of Black Plane Solutions

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.

9 pages

References in corpus (3)

• Energy and Momentum Distributions of a (2+1)-dimensional black hole background
• Energy-Momentum in viscous Kasner-type Universe in Bergmann-Thomson Formulations
• Topological Charged Black Holes in High Dimensional Spacetimes and Their Formation from Gravitational Collapse of a Type II Fluid

Cited by in corpus (8)

• Energy distribution in the dyadosphere of a Reissner-Nordstrom black hole in Moller's prescription
• Moeller's Energy-Momentum Complex for a Spacetime Geometry on a Noncommutative Curved D3-Brane
• Energy of the Taub Cosmological Solution
• On Energy Distribution of Two Space-times with Planar and Cylindrical Symmetries
• Energy Distribution of a Charged Black Hole with a Minimally Coupled Scalar Field
• Brane-World Black Holes and Energy-Momentum Vector
• An ASSF and the Teleparallelisim
• The Lukash Plane-Wave Attractor and Relative Energy