Re-Scaling of Energy in the Stringy Charged Black Hole Solutions using Approximate Symmetries
arXiv:1009.5280 · doi:10.1139/P10-072
Abstract
This paper is devoted to study the energy problem in general relativity using approximate Lie symmetry methods for differential equations. We evaluate second-order approximate symmetries of the geodesic equations for the stringy charged black hole solutions. It is concluded that energy must be re-scaled by some factor in the second-order approximation.
18 pages, accepted for publication in Canadian J. Physics
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