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