Energy of a Stringy Charged Black Hole in the Teleparallel Gravity
arXiv:gr-qc/0607011 · doi:10.1007/s10509-006-9208-7
Abstract
This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0212018, gr-qc/0501002, and gr-qc/9601044. This paper has excessive overlap with the following papers also written by the authors or their collaborators: gr-qc/0603108, gr-qc/0606022, gr-qc/0603027, gr-qc/0603063, gr-qc/0607083, gr-qc/0607095, gr-qc/0511030, gr-qc/0512080, gr-qc/0601141, gr-qc/0608050, gr-qc/0607082, gr-qc/0511095, gr-qc/0612016, and others.
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References in corpus (8)
- 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 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
- Energy in Reboucas-Tiomno-Korotkii-Obukhov and Godel-type Space-times in Bergmann-Thomson's Formulations
- Energy Density Associated with the Bianchi Type-II Space-Time
- Different Approaches to the Einstein Energy Associated with the de Sitter C-Space-time