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Violations of the Kerr and Reissner-Nordström bounds: Horizon versus asymptotic quantities
Physical Review D
A central feature of the most elementary rotating black hole (BH) solution in General Relativity is the Kerr bound, which, for vacuum Kerr BHs, can be expressed either in terms of the ADM or the horizon "charges". This bound, however, is not a fundamental properties of General Relativity and stationary, asymptotically flat, regular (on and outside an event horizon) BHs are known to violate the Kerr bound, both in terms of their ADM and horizon quantities. Examples include the recentlydoi:10.1103/physrevd.94.024006 fatcat:sy5bnp3khjf3tcsm7hrszgakvi