Energy distribution of the Einstein-Klein-Gordon system for a static spherically symmetric spacetime in (2+1)-dimensions
General Relativity and Quantum Cosmology
2010-11-05 v1
Abstract
We use Moeller's energy-momentum complex in order to explicitly compute the energy and momentum density distributions for an exact solution of Einstein's field equations with a negative cosmological constant minimally coupled to a static massless scalar field in a static, spherically symmetric background in (2+1)-dimensions.
Keywords
Cite
@article{arxiv.gr-qc/0508005,
title = {Energy distribution of the Einstein-Klein-Gordon system for a static spherically symmetric spacetime in (2+1)-dimensions},
author = {I. Radinschi and Th. Grammenos},
journal= {arXiv preprint arXiv:gr-qc/0508005},
year = {2010}
}
Comments
9 pages, 1 figure