Reconsidering Schwarzschild's original solution
arXiv:gr-qc/0102084 · doi:10.1002/1521-3994(200107)322:3<137::AID-ASNA137>3.0.CO;2-1
Abstract
We analyse the Schwarzschild solution in the context of the historical development of its present use, and explain the invariant definition of a singular surface at the Schwarzschild's radius, that can be applied to the Kerr-Newman solution too.
9 pages, added references and a remark on the norm of the timelike Killing vector. Accepted for publication by Astronomische Nachrichten
Cited by in corpus (13)
- Quantum corrections to the thermodynamics of Schwarzschild-Tangherlini black hole and the generalized uncertainty principle
- Corrections to the thermodynamics of Schwarzschild-Tangherlini black hole and the generalized uncertainty principle
- Sgr A* and General Relativity
- General form of entropy on the horizon of the universe in entropic cosmology
- Radiative processes of two entangled atoms outside a Schwarzschild black hole
- Obstruction of black hole singularity by quantum field theory effects
- The Klein-Gordon Equation of a Rotating Charged Hairy Black Hole in (2+1) Dimensions
- Screening an extremal black hole with a thin shell of exotic matter
- On singularities, horizons, invariants, and the results of Antoci, Liebscher and Mihich (GRG 38, 15 (2006) and earlier)
- Riemann curvature of a boosted spacetime geometry
- Free fall and self-force: an historical perspective
- The physical meaning of the "boost-rotation symmetric" solutions within the general interpretation of Einstein's theory of gravitation
- Interpreting solutions with nontrivial Killing groups in general relativity