Gravitational collapse and spacetime singularities by Pankaj S. Joshi PDF

By Pankaj S. Joshi

ISBN-10: 0511378904

ISBN-13: 9780511378904

ISBN-10: 0521871042

ISBN-13: 9780521871044

Actual phenomena in astrophysics and cosmology contain gravitational cave in in a primary method. the ultimate destiny of a big big name while it collapses below its personal gravity on the finish of its existence cycle is among the most crucial questions in gravitation idea and relativistic astrophysics, and is the root of black gap physics. normal relativity predicts that continuous gravitational cave in supplies upward thrust to a space-time singularity. Quantum gravity might take over in such regimes to unravel the classical space-time singularity. This ebook investigates those matters, and indicates how the noticeable ultra-dense areas come up obviously and generically as an end result of dynamical gravitational cave in. it is going to be of curiosity to graduate scholars and educational researchers in gravitation physics, basic physics, astrophysics, and cosmology. It incorporates a unique evaluate of modern study into gravitational cave in, and a number of other examples of cave in versions are investigated intimately.

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Then T is called symmetric if T (V , W ) = T (W , V ). 2 The metric tensor 21 If {ei } is a basis for the tangent space, this implies T (ei , ej ) = T (ej , ei ), that is Tij = Tji . 40) Similarly, T is called antisymmetric if Tij = −Tji . 41) One can formulate this in terms of symmetric and antisymmetric parts of T . For Tij , its symmetric part is written as T(ij) = 1 (Tij + Tji ), 2! 42) and its antisymmetric part is written as T[ij] = 1 (Tij − Tji ). 2! 43) Then, T is called symmetric if T(ij) = Tij , and antisymmetric if T[ij] = Tij .

If T is a (0, 2) type tensor, it acts on the pairs of vectors V , W to produce a real number T (V , W ) = Tij V i W j . Then T is called symmetric if T (V , W ) = T (W , V ). 2 The metric tensor 21 If {ei } is a basis for the tangent space, this implies T (ei , ej ) = T (ej , ei ), that is Tij = Tji . 40) Similarly, T is called antisymmetric if Tij = −Tji . 41) One can formulate this in terms of symmetric and antisymmetric parts of T . For Tij , its symmetric part is written as T(ij) = 1 (Tij + Tji ), 2!

It turned out, however, that the singularity was a fairly general feature of general relativity and would occur under rather general physical assumptions, as shown by the singularity theorems. Some of the solutions also have interesting applications. For example, the Minkowski spacetime is both the geometry of special relativity and locally that of any general relativistic model, and the Schwarzschild spacetime is used to test physical predictions of general relativity. JOSHI: “CHAP02” — 2007/8/18 — 17:16 — PAGE 43 — #34 44 The spacetime manifold Some of the most interesting and physically relevant solutions to the Einstein equations are spherically symmetric; these include the Friedman– Robertson–Walker models in cosmology, and the Schwarzschild solution that can model an isolated star.

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Gravitational collapse and spacetime singularities by Pankaj S. Joshi


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