2010/04/09 by G. G. L. Nashed · 55 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Classical mechanics #Cosmology #Cosmology and Gravitation Theories #Einstein #Exact solutions in general relativity #General relativity #Geometry #Gravitation #Gravitational energy #Introduction to the mathematics of general relativity #Mathematical physics #Mechanics #Numerical relativity #Physics #Quantum mechanics #Relativity and Gravitational Theory #Rotational symmetry #Stress–energy tensor #Tensor (intrinsic definition) #Tetrad #Theoretical physics #Theory of relativity #gr-qc
paper · pdf · doi:10.1007/s10509-010-0375-1
published in Astrophysics and Space Science 330(1), 173-181 (Springer Science+Business Media) · 14 pages Latex. arXiv admin note: text overlap with arXiv:gr-qc/0609018, arXiv:0704.0488 by other authors
openalex publication_date 2010/04/09 · arxiv created 2015/03/03 · arxiv updated 2015/03/05 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
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.