Deformations of three-dimensional metrics

被引:0
|
作者
Pugliese, Daniela [1 ]
Stornaiolo, Cosimo [2 ]
机构
[1] Silesian Univ Opava, Inst Phys, Fac Philosophy & Sci, Opava 74601, Czech Republic
[2] INFN, Sez Napoli, I-80126 Naples, Italy
关键词
Space-time deformations; Scalar fields; Three-dimensional metrics; Conformal methods; BLACK-HOLE; REFERENCE FRAMES; RIGID MOTIONS; COSMOLOGIES; RELATIVITY; SPACETIME;
D O I
10.1007/s10714-015-1864-x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine three-dimensional metric deformations based on a tetrad transformation through the action the matrices of scalar field. We describe by this approach to deformation the results obtained by Coll et al. (Gen. Relativ. Gravit. 34: 269, 2002), where it is stated that any three-dimensional metric was locally obtained as a deformation of a constant curvature metric parameterized by a 2-form. To this aim, we construct the corresponding deforming matrices and provide their classification according to the properties of the scalar sigma and of the vector s used in Coll et al. (Gen Relativ Gravit 34: 269, 2002) to deform the initial metric. The resulting causal structure of the deformed geometries is examined, too. Finally we apply our results to a spherically symmetric three geometry and to a space sector of Kerr metric.
引用
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页数:23
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