Energy distribution of the Einstein-Klein-Gordon system for a static spherically symmetric spacetime in (2+1)-dimensions

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.

9 pages, 1 figure

References in corpus (1)

• An Exact Solution for Static Scalar Fields Coupled to Gravity in $(2+1)$-Dimensions

Cited by in corpus (16)

• Energy distribution of 2+1 dimensional black holes with nonlinear electrodynamics
• 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 in a Schwarzschild-like Spacetime
• Energy and Momentum Distributions of Kantowski and Sachs Space-time
• Energy Momentum of Marder Universe in Teleparallel gravity
• Energy-momentum Prescriptions in General Spherically Symmetric Space-times
• Energy Distribution of a Regular Class of Exact Black Hole Solutions
• On Energy Distribution of Two Space-times with Planar and Cylindrical Symmetries
• Energy Distribution for Non-commutative Radiating Schwarzschild Black Holes
• Gravitational Energy in Van Stockum Space-Time
• Electric and Magnetic Black Hole Solutions of Moller's Four-Momentum
• Topological Black Holes and Momentum Four Vector
• Møller Energy-Momentum Complex in General Relativity for Higher Dimensional Universes
• The Momentum Four-Vector in Brans-Dicke Wormholes