The inequality between mass and angular momentum for axially symmetric black holes
arXiv:0707.3118 · doi:10.1142/S021827180801219X
Abstract
In this essay I first discuss the physical relevance of the inequality for axially symmetric (non-stationary) black holes, where m is the mass and J the angular momentum of the spacetime. Then, I present a proof of this inequality for the case of one spinning black hole. The proof involves a remarkable characterization of the extreme Kerr black hole as an absolute minimum of the total mass. Finally, I conjecture on the physical implications of this characterization for the non linear stability problem for black holes.
8 pages, Honorable Mention in the Gravity Research Foundation Essay Competition 2007
References in corpus (4)
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- Proof of the (local) angular momemtum-mass inequality for axisymmetric black holes
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Cited by in corpus (17)
- From Geometry to Numerics: interdisciplinary aspects in mathematical and numerical relativity
- Geometric inequalities for axially symmetric black holes
- Mass, angular-momentum, and charge inequalities for axisymmetric initial data
- A Dain Inequality with charge
- Axisymmetric evolution of Einstein equations and mass conservation
- Extreme throat initial data set and horizon area--angular momentum inequality for axisymmetric black holes
- Geometric inequalities for black holes
- Numerical evidences for the angular momentum-mass inequality for multiple axially symmetric black holes
- Extreme Bowen-York initial data
- Total angular momentum from Dirac eigenspinors
- On well-posedness, linear perturbations and mass conservation for axisymmetric Einstein equation
- Small deformations of extreme Kerr black hole initial data
- On a mass functional for initial data in 4+1 dimensional spacetime
- Linear perturbations for the vacuum axisymmetric Einstein equations
- Avenues for Analytic exploration in Axisymmetric Spacetimes. Foundations and the Triad Formalism
- Axially symmetric spacetimes: numerical and analytical perspectives
- Angular momentum-mass inequality for axisymmetric black holes