Exact Solutions of Einstein's Field Equations. Cornelius Hoenselaers, Dietrich Kramer, Eduard Herlt, Hans Stephani, Malcolm MacCallum

Exact Solutions of Einstein's Field Equations


Exact.Solutions.of.Einstein.s.Field.Equations.pdf
ISBN: 0521461367,9780521461368 | 732 pages | 19 Mb


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Exact Solutions of Einstein's Field Equations Cornelius Hoenselaers, Dietrich Kramer, Eduard Herlt, Hans Stephani, Malcolm MacCallum
Publisher: Cambridge




They were studied because it was relatively easy to analyse them. Regarding black holes, Einstein's equations work perfectly in the interior of a black hole. The solution is a plane-fronted wave metric with a cosmological constant. The reason why black holes were predicted was because these are highly symmetrical exact solutions to Einstein's field equations. We give an exact solution of the quadratic gravity in D dimensions. A class of exact solutions of the Einstein Field Equation with Relativistic Magneto hydrodynamic aspects and as well of a Raychaudhuri-like equation for the evolution of the Universe has been obtained. Exact.Solutions.of.Einstein.s.Field. This book reviews a number of important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. In fact, the first exact solution to Einstein's field equations (discovered by Schwarzschild) precisely describes a non-rotating black hole. Models is becoming an essential tool for analyzing and understanding them. Exact Solutions of Einstein's Field Equations. Then, in 1963, New Zealand mathematician Roy Kerr calculated an exact solution for Einstein's field equations representing a Kerr black hole. While serving in the war front, he produced exact solutions to some of Einstein's work in relativity theory using field equations. Cornelius Hoenselaers, Dietrich Kramer, Eduard Herlt, Hans Stephani, Malcolm MacCallum. The special feature of a Kerr black hole is that it rotates. Einstein himself praised Karl for his excellent work.