翻訳と辞書 Words near each other ・ Weyib River ・ Weyinmi Efejuku ・ Weyl (crater) ・ Weyl algebra ・ Weyl character formula ・ Weyl curvature hypothesis ・ Weyl distance function ・ Weyl equation ・ Weyl group ・ Weyl integral ・ Weyl law ・ Weyl metrics ・ Weyl module ・ Weyl scalar ・ Weyl semimetal ・ Weyl tensor ・ Weyl transformation ・ Weyl's inequality ・ Weyl's lemma (Laplace equation) ・ Weyl's postulate ・ Weyl's theorem ・ Weyl's theorem on complete reducibility ・ Weyl's tile argument ・ Weylan Harding ・ Weyland ・ Weyland ringtail possum ・ Weylin Hotel ・ Weyl–Brauer matrices ・ Weyl–Schouten theorem ・ Weyl–von Neumann theorem Dictionary Lists mini英和辞書 mini和英辞書 Webster 1913 Latin-English FOLDOC Wikipedia English ウィキペディア

翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク Weyl tensor ： ウィキペディア英語版 Weyl tensor In differential geometry, the Weyl curvature tensor, named after Hermann Weyl, is a measure of the curvature of spacetime or, more generally, a pseudo-Riemannian manifold. Like the Riemann curvature tensor, the Weyl tensor expresses the tidal force that a body feels when moving along a geodesic. The Weyl tensor differs from the Riemann curvature tensor in that it does not convey information on how the volume of the body changes, but rather only how the shape of the body is distorted by the tidal force. The Ricci curvature, or trace component of the Riemann tensor contains precisely the information about how volumes change in the presence of tidal forces, so the Weyl tensor is the traceless component of the Riemann tensor. It is a tensor that has the same symmetries as the Riemann tensor with the extra condition that it be trace-free: metric contraction on any pair of indices yields zero. In general relativity, the Weyl curvature is the only part of the curvature that exists in free space—a solution of the vacuum Einstein equation—and it governs the propagation of gravitational radiation through regions of space devoid of matter. More generally, the Weyl curvature is the only component of curvature for Ricci-flat manifolds and always governs the characteristics of the field equations of an Einstein manifold. In dimensions 2 and 3 the Weyl curvature tensor vanishes identically. In dimensions ≥ 4, the Weyl curvature is generally nonzero. If the Weyl tensor vanishes in dimension ≥ 4, then the metric is locally conformally flat: there exists a local coordinate system in which the metric tensor is proportional to a constant tensor. This fact was a key component of Nordström's theory of gravitation, which was a precursor of general relativity. ==Definition== The Weyl tensor can be obtained from the full curvature tensor by subtracting out various traces. This is most easily done by writing the Riemann tensor as a (0,4) valence tensor (by contracting with the metric). The (0,4) valence Weyl tensor is then where ''n'' is the dimension of the manifold, ''g'' is the metric, ''R'' is the Riemann tensor, ''Ric'' is the Ricci tensor, ''s'' is the scalar curvature, and $h\; \backslash wedge\backslash !\backslash !\backslash !\backslash !\backslash !\backslash !\backslash bigcirc\; k$ denotes the Kulkarni–Nomizu product of two symmetric (0,2) tensors: The ordinary (1,3) valent Weyl tensor is then given by contracting the above with the inverse of the metric. The decomposition () expresses the Riemann tensor as an orthogonal direct sum, in the sense that :$|R|^2\; =\; |C|^2\; +\; \backslash left|\backslash frac\backslash left(\backslash mathrm\; -\; \backslash fracg\backslash right)\; \backslash wedge\backslash !\backslash !\backslash !\backslash !\backslash !\backslash !\backslash bigcirc\; g\backslash right|^2\; +\; \backslash left|\backslash fracg\; \backslash wedge\backslash !\backslash !\backslash !\backslash !\backslash !\backslash !\backslash bigcirc\; g\backslash right|^2.$ This decomposition, known as the Ricci decomposition, expresses the Riemann curvature tensor into its irreducible components under the action of the orthogonal group . In dimension 4, the Weyl tensor further decomposes into invariant factors for the action of the special orthogonal group, the self-dual and antiself-dual parts ''C''+ and ''C''−. The Weyl tensor can also be expressed using the Schouten tensor, which is a trace-adjusted multiple of the Ricci tensor, :$P\; =\; \backslash frac\backslash left(\backslash mathrm\; -\; \backslash fracg\backslash right).$ Then :$C\; =\; R\; -\; P\; \backslash wedge\backslash !\backslash !\backslash !\backslash !\backslash !\backslash !\backslash bigcirc\; g.$ In indices, :$C\_=R\_-\backslash frac(g\_R\_R\_-g\_R\_R\_)+\backslash fracR~g\_g\_g\_$ where $R\_$ is the Riemann tensor, $R\_$ is the Ricci tensor, $R$ is the Ricci scalar (the scalar curvature) and brackets around indices refers to the antisymmetric part. Equivalently, :$=\; -\; 4S\_\{\}$ where ''S'' denotes the Schouten tensor. 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Weyl tensor」の詳細全文を読む スポンサード リンク 翻訳と辞書 : 翻訳のためのインターネットリソース Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.