Arxiv:Gr-Qc/0309008V2 9 Feb 2004
The Cotton tensor in Riemannian spacetimes Alberto A. Garc´ıa∗ Departamento de F´ısica, CINVESTAV–IPN, Apartado Postal 14–740, C.P. 07000, M´exico, D.F., M´exico Friedrich W. Hehl† Institute for Theoretical Physics, University of Cologne, D–50923 K¨oln, Germany, and Department of Physics and Astronomy, University of Missouri-Columbia, Columbia, MO 65211, USA Christian Heinicke‡ Institute for Theoretical Physics, University of Cologne, D–50923 K¨oln, Germany Alfredo Mac´ıas§ Departamento de F´ısica, Universidad Aut´onoma Metropolitana–Iztapalapa Apartado Postal 55–534, C.P. 09340, M´exico, D.F., M´exico (Dated: 20 January 2004) arXiv:gr-qc/0309008v2 9 Feb 2004 1 Abstract Recently, the study of three-dimensional spaces is becoming of great interest. In these dimensions the Cotton tensor is prominent as the substitute for the Weyl tensor. It is conformally invariant and its vanishing is equivalent to conformal flatness. However, the Cotton tensor arises in the context of the Bianchi identities and is present in any dimension n. We present a systematic derivation of the Cotton tensor. We perform its irreducible decomposition and determine its number of independent components as n(n2 4)/3 for the first time. Subsequently, we exhibit its characteristic properties − and perform a classification of the Cotton tensor in three dimensions. We investigate some solutions of Einstein’s field equations in three dimensions and of the topologically massive gravity model of Deser, Jackiw, and Templeton. For each class examples are given. Finally we investigate the relation between the Cotton tensor and the energy-momentum in Einstein’s theory and derive a conformally flat perfect fluid solution of Einstein’s field equations in three dimensions.
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