Energy Distribution in Reissner-Nordstrom anti-de Sitter black holes in Moller Prescription

This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0010068, gr-qc/9911018, gr-qc/0303034, and gr-qc/0212018.Comment: This submission has been withdrawn by arXiv administrators due to inappropriate text reuse from external source

Energy Momentum of Marder Universe in Teleparallel gravity

This paper has been removed by arXiv administrators because of overlap with gr-qc/0408043 and 0706.3245. This paper has excessive overlap with the following papers also written by the authors or their collaborators: gr-qc/0607110, gr-qc/0607126, gr-qc/0608024, gr-qc/0603044, gr-qc/0505078, gr-qc/0502042, gr-qc/0502031, gr-qc/0606028, gr-qc/0508018, gr-qc/0511095, and others.Comment: This submission has been withdrawn by arXiv administrators due to inappropriate text reuse from external source

On the Gravitational Energy Associated with Spacetimes of Diagonal Metric

This paper also has excessive overlap with the following papers also written by the authors or their collaborators: gr-qc/0608014, gr-qc/0511095, gr-qc/0505078, gr-qc/0502060, gr-qc/0603027, gr-qc/0606028, gr-qc/0607109, gr-qc/0607110, gr-qc/0508018, gr-qc/0502031, and others.Comment: This submission has been withdrawn by arXiv administrators due to inappropriate text reuse from external source

An axially symmetric scalar and the Teleparallelism

An axially symmetric scalar field is considered in teleparallel gravity. We calculate, respectively, the tensor, the vector and the axial-vector parts of torsion and energy, momentum and angular momentum in the ASSF. We find the vector parts are in the radial and e^θ directions, the axial-vector, momentum and angular momentum vanish identically, but the energy distribution is different from zero. The vanishing axial-vector part of torsion gives us the result that there occurs no deviation in the spherical symmetry of the spacetime. Consequently, there exists no inertia field with respect to a Dirac particle, and the spin vector of a Dirac particle becomes constant. The result for the energy is the same as obtained by Radinschi. Next, this work also (a) supports the viewpoint of Lessner that the Møller energy-momentum complex is a powerful concept for the energy-momentum, (b) sustains the importance of the energy-momentum definitions in the evaluation of the energy distribution of a given spacetime, and (c) supports the hypothesis by Cooperstock that the energy is confined to the region of non-vanishing energy-momentum tensor of the matter and all non-gravitational fields

The Lukash Plane-Wave Attractor and Relative Energy

This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0411070, "Structure and stability of the Lukash plane-wave spacetime," by John D. Barrow and Christos G. Tsagas; and gr-qc/0205028, "Gravitational Energy of Kerr and Kerr Anti-de Sitter Space-times in the Teleparallel Geometry," by J. F. da Rocha-neto and K. H. Castello-Branco.Comment: This submission has been withdrawn by arXiv administrators due to inappropriate text reuse from external source

Different Approaches for Moller's Energy in the Kasner-type Space-time

This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0011027, "Viscous cosmologies in scalar-tensor theories for Kasner type metrics," by M. Cataldo, S. del Campo and P. Salgado; Phys. Rev. D 41, 1086 (1990), "Energy associated with a Kerr-Newman black hole," by K.S. Virbhadra; and gr-qc/0303034, "The energy of the universe in teleparallel gravity," by T. Vargas.Comment: This submission has been withdrawn by arXiv administrators due to inappropriate text reuse from external source