Ginzburg Conference on Physics May 28 - June 2, 2012 in Moscow

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Event horizon (BH boundary) is almost everywherenull surface (Penrose, ‘68)Black hole surface topology is (Hawking, ‘72 )Its surface area never decreases (Hawking,’71,72)Soon after their formation black holes becomestationary (the `balding phase’ T r / c ) .Stationary black holes are either static(Schwarzschild) or axially symmetric (Kerr).S2g
Uniqueness theorem: Stationary isolated BHsare uniquely specified by their mass and angularmomentum and are described by the Kerr metric(Israel ’67, Carter ‘71,73, Robinson ‘75)Geodesic equations of motion in Kerr ST arecompletely integrable (Carter ‘68)The Kerr metric besides the evident STsymmetries has also hidden symmetry (Killingand Killing-Yano tensors) (Penrose&Walker ‘70,Penrose&Floyd ‘73)
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Ginzburg Conference on Physics May 28 - June 2, 2012 in Moscow

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