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Maximally Symmetric Spin-Two Bitensors on S3S^3 and H3H^3

Abstract

The transverse traceless spin-two tensor harmonics on S3S^3 and H3H^3 may be denoted by T(kl)abT^{(kl)}{}_{ab}. The index kk labels the (degenerate) eigenvalues of the Laplacian \square and ll the other indices. We compute the bitensor lT(kl)ab(x)T(kl)ab(x)\sum_l T^{(kl)}{}_{ab}(x) T^{(kl)}{}_{a'b'}(x')^* where x,xx,x' are distinct points on a sphere or hyperboloid of unit radius. These quantities may be used to find the correlation function of a stochastic background of gravitational waves in spatially open or closed Friedman-Robertson-Walker cosmologies.Comment: 12 pages, RevTeX, uuencoded compressed .tex file, minor typos correcte

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