Moller's Energy in the Dyadosphere of a Charged Black Hole
arXiv:gr-qc/0606022 · doi:10.1007/s12043-006-0068-z
Abstract
This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0304081, gr-qc/0212018, gr-qc/0501002, gr-qc/9601044, and gr-qc/0109017. This paper also has excessive overlap with the following papers also written by the authors or their collaborators: gr-qc/0603027, gr-qc/0511030, gr-qc/0512080, gr-qc/0607011, gr-qc/0603108, gr-qc/0601141, gr-qc/0603063, gr-qc/0608050, gr-qc/0607095, gr-qc/0607082, gr-qc/0511095, gr-qc/0601070, gr-qc/0505078, gr-qc/0607083, gr-qc/0607116, gr-qc/0612016, and others.
This submission has been withdrawn by arXiv administrators due to inappropriate text reuse from external sources
References in corpus (9)
- The energy of the universe in teleparallel gravity
- Energy Distribution in 2d Stringy Black Hole Backgrounds
- General Formula for the Momentum Imparted to Test Particles in Arbitrary Spacetimes
- Energy-Momentum in viscous Kasner-type Universe in Bergmann-Thomson Formulations
- Energy Distribution of a Stringy Charged Black Hole
- Energy of the Universe in Bianchi-type I Models in Moller's Tetrad Theory of Gravity
- Energy-Momentum in the Viscous Kasner-type Universe in Teleparallel Gravity
- Relative Energy-Momentum of the Bianchi-I Type Universes in Teleparallel Gravity
- Different Approaches for Moller's Energy in the Kasner-type Space-time