Energy Distribution in a Schwarzschild-like Spacetime
arXiv:gr-qc/0602105 · doi:10.1007/s10773-006-9259-0
Abstract
In this paper, utilizing Møller's energy-momentum complex, we explicitly evaluate the energy and momentum density associated with a metric describing a four-dimensional, Schwarzschild-like, spacetime derived from an effective gravity coupled with a U(1) gauge field in the context of a D3-brane dynamics in the classical regime, i.e., between the asymptotic and the Planck regime.
10 pages; title changed; references updated; content revised
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Cited by in corpus (6)
- On the energy of charged black holes in generalized dilaton-axion gravity
- On the energy of Hořava-Lifshitz black holes
- Moeller's Energy-Momentum Complex for a Spacetime Geometry on a Noncommutative Curved D3-Brane
- Energy Distribution of a Regular Class of Exact Black Hole Solutions
- Energy-Momentum Distribution in General Relativity for a Phantom Black Hole Metric
- Energy Distribution for Non-commutative Radiating Schwarzschild Black Holes