Energy distribution of the Einstein-Klein-Gordon system for a static spherically symmetric space-time in (2+1) dimensions
Date
2006Sujet
Résumé
We use Moller'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.