Titlebook: Black Hole Physics; Basic Concepts and N Valeri P. Frolov,Igor D. Novikov Book 1998 Springer Science+Business Media Dordrecht 1998 Gravity.

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Mhc-Molecule

Die Ellipse: Konjugierte Durchmessersehnentles down very quickly to the unique stationary state — a Kerr-Newman black hole. Dynamical deviations from this state produce the emission of gravitational radiation. This radiation interacts with the spacetime curvature. While part of it escapes to infinity, another part is backscattered and absor

戲法

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Rotating Black Holeshole when the radius of the collapsing body becomes less than the gravitational radius. Suppose the collapsing body deviates considerably from spherical symmetry and/or its angular momentum and electromagnetic field are large. Will a black hole form? If it does, what will its properties be?

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結(jié)束

Ultimate Fate of Black and White Holeshe book certainly is not a complete theory and requires modifications because of quantum effects. Quantum effects become dominant at Planck scales, and quantum gravity is required there. In this section we comment on some of the problems of black hole physics that require quantum gravity for their solutions.

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Fundamental Theories of Physicshttp://image.papertrans.cn/b/image/188946.jpg

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Black Hole Physics978-94-011-5139-9Series ISSN 0168-1222 Series E-ISSN 2365-6425

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