On the Moller Energy Associated with Black Holes
arXiv:gr-qc/0603027 · doi:10.1007/s10773-006-9212-2
Abstract
This paper has been removed by arXiv administrators because of overlap with gr-qc/9601044, gr-qc/0212018, hep-th/0310151, gr-qc/0011066, gr-qc/0404001, gr-qc/0304081, gr-qc/0501002, and gr-qc/0109017. This paper also has excessive overlap with the following papers also written by the authors or their collaborators: gr-qc/0606022, gr-qc/0512080, gr-qc/0511030, gr-qc/0603063, gr-qc/0603108, gr-qc/0511095, gr-qc/0607095, gr-qc/0608050, gr-qc/0601141, gr-qc/0607011, gr-qc/0607082, gr-qc/0603044, gr-qc/0607083, and others.
This submission has been withdrawn by arXiv administrators due to inappropriate text reuse from external sources
References in corpus (7)
- General Formula for the Momentum Imparted to Test Particles in Arbitrary Spacetimes
- Energy distribution in a BTZ black hole spacetime
- Energy-Momentum in viscous Kasner-type Universe in Bergmann-Thomson Formulations
- Energy-Momentum in the Viscous Kasner-type Universe in Teleparallel Gravity
- Relative Energy-Momentum of the Bianchi-I Type Universes in Teleparallel Gravity
- Energy of the Universe in Bianchi-type I Models in Moller's Tetrad Theory of Gravity
- Different Approaches for Moller's Energy in the Kasner-type Space-time