The transverse traceless spin-two tensor harmonics on S3 and H3 may be
denoted by T(kl)ab. The index k labels the (degenerate) eigenvalues
of the Laplacian □ and l the other indices. We compute the bitensor
∑lT(kl)ab(x)T(kl)a′b′(x′)∗ where x,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
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