Energy and Momentum Densities Associated with Solutions Exhibiting Directional Type Singularities
arXiv:gr-qc/0404108 · doi:10.1007/s10714-006-0230-4
Abstract
We obtain the energy and momentum densities of a general static axially symmetric vacuum space-time described by the Weyl metric, using Landau-Lifshitz and Bergmann-Thomson energy-momentum complexes. These two definitions of the energy-momentum complex do not provide the same energy density for the space-time under consideration, while give the same momentum density. We show that, in the case of Curzon metric which is a particular case of the Weyl metric, these two definitions give the same energy only when . Furthermore, we compare these results with those obtained using Einstein, Papapetrou and Møller energy momentum complexes.
10 pages, references added, minor corrections [Admin note: substantial overlap with gr-qc/0403097 , gr-qc/0403039 ]
References in corpus (4)
Cited by in corpus (12)
- Energy distribution in the dyadosphere of a Reissner-Nordstrom black hole in Moller's prescription
- Bergmann-Thomson energy-momentum complex for solutions more general than the Kerr-Schild class
- Energy and momentum of Bianchi Type VI_h Universes
- On the energy of charged black holes in generalized dilaton-axion gravity
- The Energy of Regular Black Hole in General Relativity Coupled to Nonlinear Electrodynamics
- On the energy of Hořava-Lifshitz black holes
- Moeller's Energy-Momentum Complex for a Spacetime Geometry on a Noncommutative Curved D3-Brane
- Energy and Momentum densities of cosmological models, with equation of state , in general relativity and teleparallel gravity
- Energy and Momentum Distributions of Kantowski and Sachs Space-time
- Møller Energy-Momentum Complex of a Static Axially Symmetric Vacuum Space-Time
- Energy Distribution of a Regular Class of Exact Black Hole Solutions
- Gravitational Energy in Van Stockum Space-Time