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Titlebook: General Relativity; With Applications to Norbert Straumann Textbook 20041st edition Springer-Verlag Berlin Heidelberg 2004 EFE.Gravity.RMS.

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31#
發(fā)表于 2025-3-26 23:57:01 | 只看該作者
32#
發(fā)表于 2025-3-27 04:48:43 | 只看該作者
Differential FormsCartan’s calculus of differential forms is particularly useful in general relativity (but also in other fields of physics). We begin our discussion by repeating some algebraic preliminaries.
33#
發(fā)表于 2025-3-27 05:35:11 | 只看該作者
Affine ConnectionsIn this section we introduce an important additional structure on differentiable manifolds, thus making it possible to define a “covariant derivative” which transforms tensor fields into other tensor fields.
34#
發(fā)表于 2025-3-27 09:29:54 | 只看該作者
Summary of Results and Further Research,eads naturally to the kinematical framework of general relativity and determines, suitable interpreted, the coupling of physical systems to external gravitational fields. This will be discussed in detail in the present chapter.
35#
發(fā)表于 2025-3-27 16:08:58 | 只看該作者
36#
發(fā)表于 2025-3-27 21:05:51 | 只看該作者
Research Joint Venture Cartels and Welfare,expects, however, that the horizon will quickly settle down to a stationary state as a result of the emission of gravitational waves. The geometry of the stationary black hole is of course no longer spherically symmetric.
37#
發(fā)表于 2025-3-27 23:07:51 | 只看該作者
38#
發(fā)表于 2025-3-28 04:56:58 | 只看該作者
39#
發(fā)表于 2025-3-28 09:59:24 | 只看該作者
Einstein’s Field Equationsystems. The hard core of the theory, however, consists of ., which relate the metric field to matter. After a discussion of the physical meaning of the curvature tensor, we shall first give a simple physical motivation for the field equations and will then show that they are determined by only a few natural requirements’.
40#
發(fā)表于 2025-3-28 14:26:58 | 只看該作者
Black Holesexpects, however, that the horizon will quickly settle down to a stationary state as a result of the emission of gravitational waves. The geometry of the stationary black hole is of course no longer spherically symmetric.
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