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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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發(fā)表于 2025-3-21 17:14:20 | 只看該作者 |倒序瀏覽 |閱讀模式
期刊全稱Black Hole Physics
期刊簡稱Basic Concepts and N
影響因子2023Valeri P. Frolov,Igor D. Novikov
視頻videohttp://file.papertrans.cn/189/188946/188946.mp4
學科分類Fundamental Theories of Physics
圖書封面Titlebook: Black Hole Physics; Basic Concepts and N Valeri P. Frolov,Igor D. Novikov Book 1998 Springer Science+Business Media Dordrecht 1998 Gravity.
影響因子It is not an exaggeration to say that one of the most exciting predictions of Einstein‘s theory of gravitation is that there may exist "black holes": putative objects whose gravitational fields are so strong that no physical bodies or signals can break free of their pull and escape. The proof that black holes do exist, and an analysis of their properties, would have a significance going far beyond astrophysics. Indeed, what is involved is not just the discovery of yet another even if extremely remarkable, astro- physical object, but a test of the correctness of our understanding of the properties of space and time in extremely strong gravitational fields. Theoretical research into the properties of black holes, and into the possible corol- laries of the hypothesis that they exist, has been carried out with special vigor since the beginning of the 1970‘s. In addition to those specific features of black holes that are important for the interpretation of their possible astrophysical manifestations, the theory has revealed a number of unexpected characteristics of physical interactions involving black holes. By the middle of the 1980‘s a fairly detailed understanding had been achieved
Pindex Book 1998
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Lehrbuch der darstellenden Geometrieack hole (of a given mass .) is determined unambiguously by its electric charge . and rotation parameter .. If the charged black hole does not rotate, its electromagnetic field reduces to the radial electric field of the charge . and is static. Any multipoles higher than the monopole are absent.
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Die Ellipse: Konjugierte Durchmessersehnentional radiation. This radiation interacts with the spacetime curvature. While part of it escapes to infinity, another part is backscattered and absorbed by the resulting black hole. In the end all deviations from the Kerr-Newman field decay to zero.
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The Interior of a Black Holetional radiation. This radiation interacts with the spacetime curvature. While part of it escapes to infinity, another part is backscattered and absorbed by the resulting black hole. In the end all deviations from the Kerr-Newman field decay to zero.
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Book 1998putative objects whose gravitational fields are so strong that no physical bodies or signals can break free of their pull and escape. The proof that black holes do exist, and an analysis of their properties, would have a significance going far beyond astrophysics. Indeed, what is involved is not jus
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