Energy problem in the Einstein–Cartan theory

被引:0
|
作者
R. F. Polishchuk
机构
[1] Lebedev Physical Institute of RAS,
来源
Gravitation and Cosmology | 2015年 / 21卷
关键词
Black Hole; Gravitational Wave; Primordial Black Hole; World Point; Matter Tensor;
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摘要
The Einstein–Cartan–Kibble–Sciama equations are presented in the following form: the codifferential of the differential of a tetrad is the tetrad current with the ordinary conservation law. This form is an analogue of the form for non-Abelian quantum field theory. A canonical gauge tetrad is proposed for six two-directions with extreme sectional Riemannian curvature. A nonlocal conservation law for the contracted Bianchi identities is presented. The physical and geometric meaning of the Gibbons-Hawking Lagrangian and surface term are proposed. Application of the tetrad current concept is illustrated for the Schwarzschild and de Sitter metrics.
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页码:220 / 235
页数:15
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