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We prove that in Einstein-Maxwell theory the inequality $(8\pi J)^2+(4\pi Q^2)^2 < A^2$ holds for any sub-extremal axisymmetric and stationary black hole with arbitrary surrounding matter.
Bardeen, J.M.: Rapidly rotating stars, disks, and black holes Black holes
1973
Earlier work this paper cites.
Carter, B.: Black hole equilibrium states Black Holes
1973
Earlier work this paper cites.
Rauch, J.: Partial Differential Equations
1991
Earlier work this paper cites.
Yosida, K.: Functional Analysis
1995
Cited alongside, same era.
Buttazzo, G., Giaquinta, M. and Hildebrandt, S.: One-dimensional variational problems
1998
Cited alongside, same era.
Evans, L.C.: Partial Differential Equations
2002
Cited alongside, same era.
Ansorg, M. and Pfister, H.: A universal constraint between charge and rotation rate for degenerate black holes surrounded by matter. Class. Quantum Grav. 25
2008
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Booth, I. and Fairhurst, S.: Extremality conditions for isolated and dynamical horizons. Phys. Rev. D 77
2008
Closest in time.
Hennig, J., Ansorg, M. and Cederbaum, C: A universal inequality between the angular momentum and horizon area for axisymmetric and stationary black holes with surrounding matter. Class. Quantum Grav. 25
2008
Closest in time.
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