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Re-Scaling of Energy in the Stringy Charged Black Hole Solutions using Approximate Symmetries
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Re-Scaling of Energy in the Stringy Charged Black Hole Solutions using Approximate Symmetries
classification
gr-qc
keywords
approximateenergyblackchargedequationsholesecond-ordersolutions
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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.
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