The angular momentum and mass formulas for rotating stationary quasi-black holes
arXiv:0901.3860 · doi:10.1103/PhysRevD.79.044020
Abstract
We consider the quasi-black hole limit of a stationary body when its boundary approaches its own gravitational radius, i.e., its quasi-horizon. It is shown that there exists a perfect correspondence between the different mass contributions and the mass formula for quasi-black and black holes in spite of difference in derivation and meaning of the formulas in both cases. For extremal quasi-black holes the finite surface stresses give zero contribution to the total mass. Conclusions similar to those for the properties of mass are derived for the angular momentum.
arXiv comment14 pages
References in corpus (14)
- Fate of gravitational collapse in semiclassical gravity
- Black hole mimickers: regular versus singular behavior
- Dirty black holes: Symmetries at stationary non-static horizons
- Quasi-black holes: definition and general properties
- Magnetic Monopoles Near the Black Hole Threshold
- Quasi-Black Holes from Extremal Charged Dust
- Gravitational Properties of Monopole Spacetimes Near the Black Hole Threshold
- Bonnor stars in d spacetime dimensions
- Classical model of elementary particle with Bertotti-Robinson core and extremal black holes
- Self-Renormalization of the Classical Quasilocal Energy
- Gravitational magnetic monopoles and Majumdar-Papapetrou stars
- On the black hole limit of rotating fluid bodies in equilibrium
- Quasistationary collapse to the extreme Kerr black hole
- The mass formula for quasi-black holes
Cited by in corpus (11)
- Entropy of quasiblack holes
- Quasiblack holes with pressure: relativistic charged spheres as the frozen stars
- Entropy of extremal black holes from entropy of quasiblack holes
- Dirty rotating black holes: regularity conditions on stationary horizons
- Quasiblack holes with pressure: General exact results
- Compact objects in general relativity: From Buchdahl stars to quasiblack holes
- On the black hole limit of rotating discs and rings
- What happens to Petrov classification on horizons of axisymmetric dirty black holes
- Acceleration of particles by quasiblack holes
- Black hole mass formula in the membrane paradigm
- Rotating charged fluids: Theorems and results for Weyl-type systems