A novel derivation of the rotating black hole metric
Abstract
We derive the rotating black hole metric by appealing to ellipsoidal symmetry of space and a general guiding principle of incorporation of the Newtonian acceleration for massive and no acceleration for massless particles.
- Publication:
-
General Relativity and Gravitation
- Pub Date:
- November 2013
- DOI:
- 10.1007/s10714-013-1594-x
- arXiv:
- arXiv:1301.5314
- Bibcode:
- 2013GReGr..45.2383D
- Keywords:
-
- Kerr solution;
- Rotating black hole;
- Kerr-Newman black hole;
- Gravitational self interaction;
- Kerr–Newman black hole;
- General Relativity and Quantum Cosmology;
- Astrophysics - High Energy Astrophysical Phenomena;
- High Energy Physics - Theory
- E-Print:
- 4 pages, to agree with the published version except one additional reference, pubmished