Kinematic self-similar locally rotationally symmetric models
arXiv:gr-qc/9708019 · doi:10.1088/0264-9381/15/11/026
Abstract
A brief summary of results on kinematic self-similarities in general relativity is given. Attention is focussed on locally rotationally symmetric models admitting kinematic self-similar vectors. Coordinate expressions for the metric and the kinematic self-similar vector are provided. Einstein's field equations for perfect fluid models are investigated and all the homothetic perfect fluid solutions admitting a maximal four-parameter group of isometries are given.
12 pages, LaTeX, final version, to appear in Class. Quantum Grav
References in corpus (3)
Cited by in corpus (8)
- Self-Similarity in General Relativity \endtitle
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- Bi-conformal vector fields and their applications
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- Infinite Kinematic Self-Similarity and Perfect Fluid Spacetimes
- A geometric description of the intermediate behaviour for spatially homogeneous models
- About Bianchi I with VSL