Stationary Axisymmetric Solutions and their Energy Contents in Teleparallel Equivalent of Einstein Theory

Abstract

We apply the energy-momentum tensor which is coordinate independent to calculate the energy content of the axisymmetric solutions. Our results are compared with what have been obtained before within the framework of Einstein general relativity and Møler's tetrad theory of gravitation.

14 pages Latex. arXiv admin note: text overlap with arXiv:gr-qc/0609018, arXiv:0704.0488 by other authors

References in corpus (2)

• Covariance properties and regularization of conserved currents in tetrad gravity
• The angular momentum of the gravitational field and the Poincare group

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