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Kerr black holes have their angular momentum, $J$, bounded by their mass, $M$: $Jc\leqslant GM^2$.
R. P. Kerr, “Gravitational field of a spinning mass as an example of algebraically special metrics,” Phys. Rev. Lett. 11
1963
Earlier work this paper cites.
C. W. Misner, K. S. Thorne and J. A. Wheeler, “Gravitation,” W. H. Freeman and Company (1973)
1973
Earlier work this paper cites.
F. E. Schunck and E. W. Mielke, “General relativistic boson stars,” Class. Quant. Grav. 20
2003
Earlier work this paper cites.
S. Dain, “Angular momentum-mass inequality for axisymmetric black holes,” Phys. Rev. Lett. 96
2006
Earlier work this paper cites.
H. Elvang and P. Figueras, “Black Saturn,” JHEP 0705
2007
Cited alongside, same era.
S. Dain, “Proof of the angular momentum-mass inequality for axisymmetric black holes,” J. Diff. Geom. 79
2008
Cited alongside, same era.
2008
Cited alongside, same era.
2009
Cited alongside, same era.
Cited in the paper.
Cited in the paper.
P. K. Townsend, “Black holes: Lecture notes,” gr-qc/9707012
Cited in the paper.
2011
Later among the works it cites.
S. L. Liebling and C. Palenzuela, “Dynamical Boson Stars,” Living Rev. Rel. 15
2012
Later among the works it cites.
C. A. R. Herdeiro and E. Radu, “Kerr black holes with scalar hair,” Phys. Rev. Lett. 112
2014
Later among the works it cites.
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