“... that near-extremal black holes are characterized by a finite mass gap above the corresponding zero...”
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“...Abstract It is conjectured that stationary black holes are characterized by the inverse hoop...”
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“...}},{\bar{Q}})$$ τ(a¯,Q¯) of these canonical black-hole spacetimes can be described by a two-dimensional...”
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“...Spinning Kerr black holes are known to be superradiantly unstable to massive scalar perturbations...”
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“...The elegant ‘no short hair’ theorem states that, if a spherically-symmetric static black hole has...”
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“... temperature of black holes. The suggested bound is supported by a gedanken experiment in which a charged...”
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“...Abstract The physical and mathematical properties of the non-linearly coupled black-hole-orbiting...”
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“... confined between the black hole and the mirror. A remarkable feature of this composed black-hole–mirror...”
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“... black holes is characterized by the dimensionless ratio η≡τgap/τemission≫1, where τgap...”
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“...It is proved that dynamically formed Reissner-Nordström-de Sitter (RNdS) black holes, which have...”
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“...Bekenstein and Mukhanov (BM) have suggested that, in a quantum theory of gravity, black holes may...”
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“... (the “photonsphere”) of the corresponding black-hole spacetime: rfield>rnull. In this paper we provide compelling...”
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“...Abstract It is often stated in the physics literature that maximally-spinning Kerr black-hole...”
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“...–Nordström–de Sitter (RNdS) black-hole spacetime is studied analytically. Interestingly, it is proved...”
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“...It is well known that the U(1) Reissner–Nordström black hole is stable within the framework...”
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“...We provide a remarkably compact proof that spherically symmetric neutral black holes cannot support...”
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“...It has recently been demonstrated that charged black holes can support spatially regular matter...”
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“... an extrinsic orbital angular momentum is captured by a spinning Kerr black hole. The gravitational spin-orbit...”
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“...Abstract The semi-classical Hawking evaporation process of Reissner–Nordström black holes...”
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“..., Bekenstein and Mayo have pointed out that three-dimensional Schwarzschild black holes are characterized by a...”
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