A novel derivation of the rotating black hole metric
arXiv:1301.5314 · doi:10.1007/s10714-013-1594-x
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.
4 pages, to agree with the published version except one additional reference, pubmished
References in corpus (5)
Cited by in corpus (11)
- The Kerr Metric
- Energetics and optical properties of -dimensional rotating black hole in pure Gauss-Bonnet gravity
- Schwarzschild and Kerr Solutions of Einstein's Field Equation -- an introduction
- Physically motivated ansatz for the Kerr spacetime
- Consistent derivation of the Hawking effect for both non-extremal and extremal Kerr black holes
- Rotating black hole in Einstein and pure Lovelock gravity
- Hawking effect in an extremal Kerr black hole spacetime
- Newtonian wormholes
- Thermal radiation in curved spacetime using influence functional formalism
- Constructing vacuum spacetimes by generating manifolds of revolution around a curve
- Novel way to the metric of higher dimensional rotating black holes