Titlebook: An Introduction to the Relativistic Theory of Gravitation; Petr Hájí?ek Book 2008 Springer-Verlag Berlin Heidelberg 2008 Albert Einstein.E

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Stationary Black Holes,In the previous chapter we studied two space–times containing black holes. First we inspected the advanced Eddington–Finkelstein space–time and second the Oppenheimer–Snyder space–time. This background now allows us to define a black hole in a more rigorous way than before (cf. p. 223)

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Book 2008mentary p- ticles, the second is the theory of gravity that concerns properties of macroscopic systems such as stars, galaxies, and the universe. The relativistic theory of gr- itation which is known as general relativity was created, at the beginning of the last century, by more or less a single ma

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,Das Fortschaffen Verunglückter (Transport),d the planets generates a measurable gravitational field. In Newton’s theory, this effect is described by the Poisson equation. This section is devoted to establish the corresponding relativistic equations for gravity and to study some of their basic properties.

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Relativistic Particle Dynamics in Gravitational Fields, the non-relativistic case, this will lead to a new theory, the so-called general relativity, which will modify the theory of special relativity as well as the theory of Newtonian gravitation. This means that general relativity predicts new physical phenomena.

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