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Weyl Tensor


The Weyl tensor in dimension n>=3 is the tensor C_(abcd) defined by

 R_(abcd)=C_(abcd)+2/(n-2)(g_(a[c)R_d]b-g_(b[c)R_(d]a))
 -2/((n-1)(n-2))Rg_(a[c)g_(d]b),
(1)

where R_(abcd) is the Riemann tensor of the metric tensor g_(ab), R_(ab) is the Ricci curvature tensor, and R is the scalar curvature. Square brackets denote the normalized antisymmetric part, so that T_([ab])=1/2(T_(ab)-T_(ba)) (Wald 1984, p. 40; Carroll 1997, p. 82).

The Weyl tensor is defined so that every tensor contraction between indices gives 0. In particular,

 C^lambda_(mulambdakappa)=0
(2)

(Weinberg 1972, p. 146). The number of independent components of a Weyl tensor at a point in n dimensions for n>=3 is given by

 C_n=1/(12)n(n+1)(n+2)(n-3)
(3)

(Weinberg 1972, p. 146). For n=3, 4, ..., this gives 0, 10, 35, 84, 168, ... (OEIS A052472).


See also

Antisymmetric Part, Metric Tensor, Ricci Curvature Tensor, Riemann Tensor, Scalar Curvature

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References

Carroll, S. M. "Lecture Notes on General Relativity." 3 Dec 1997. https://arxiv.org/abs/gr-qc/9712019. https://www.preposterousuniverse.com/wp-content/uploads/grnotes-three.pdf.Eisenhart, L. P. Riemannian Geometry. Princeton, NJ: Princeton University Press, 1964.Parker, L. and Christensen, S. M. "The Ricci, Einstein, and Weyl Tensors." §2.7.1 in MathTensor: A System for Doing Tensor Analysis by Computer. Reading, MA: Addison-Wesley, pp. 30-32, 1994.Sloane, N. J. A. Sequence A052472 in "The On-Line Encyclopedia of Integer Sequences."Wald, R. M. General Relativity. Chicago, IL: University of Chicago Press, 1984.Weinberg, S. Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity. New York: Wiley, 1972.Weyl, H. "Reine Infinitesimalgeometrie." Math. Z. 2, 384-411, 1918.

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Weyl Tensor

Cite this as:

Weisstein, Eric W. "Weyl Tensor." From MathWorld--A Wolfram Resource. https://mathworld.wolfram.com/WeylTensor.html

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