Abstract
The general solution for a symmetric second-order tensorX of the equationX e(a R e b cd=0 whereR is the Riemann tensor of a space-time manifold, andX is obtained in terms of the curvature 2-form structure ofR by a straightforward geometrical technique, and agrees with that given by McIntosh and Halford using a different procedure. Two results of earlier authors are derived as simple corollaries of the general theorem.
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Hall, G.S., McIntosh, C.B.G. Algebraic determination of the metric from the curvature in general relativity. Int J Theor Phys 22, 469–476 (1983). https://doi.org/10.1007/BF02083290
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DOI: https://doi.org/10.1007/BF02083290