Titlebook: Einstein Equations: Local Energy, Self-Force, and Fields in General Relativity; Domoschool 2019 Sergio Luigi Cacciatori,Alexander Kamenshch

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Geborgenheit: Quelle der St?rkerent reference frames. This leads to two new volume elements on submanifolds: a length-contracted volume and a “de-contraction” volume, built up using wedge products. This approach conveniently handles the vorticity in the rotating disc scenario. For Schwarzschild spacetime, we derive volumes and ra

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Christiane Andersen,Christine Fredrikssontwo approaches to the problem. The first one is to solve Einstein–Maxwell equations in 4D, and the second one relies on dimensional reduction from 5D. We examine the geometry of the solutions, their horizons and singularities and compare them.

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,Die Diversifikation als sozialer Proze?,neous energy (mass) density is present. In the first solution, the pressure is isotropic, while in the second solution the tangential components of the pressure are equal to zero. In both cases, the pressure vanishes at the boundaries of the slab. Outside the slab, these solutions are matched with t

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https://doi.org/10.1007/978-3-658-03511-2eometry of black hole spacetimes, and the analysis of fields on black hole backgrounds. The Kerr model of a rotating black hole in vacuum is expected to be unique and stable. The problem of proving these fundamental facts provides the background for the material presented in these notes.

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Geometry and Analysis in Black Hole Spacetimeseometry of black hole spacetimes, and the analysis of fields on black hole backgrounds. The Kerr model of a rotating black hole in vacuum is expected to be unique and stable. The problem of proving these fundamental facts provides the background for the material presented in these notes.

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