General relativity in two- and three-dimensional space-times

Physics

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We consider the general relativity field equations in two- and three-dimensional space-times. We find that in a two-dimensional space-time we can have curvature but not matter. In a three-dimensional space-time we find that empty space must be flat, that a de Sitter solution exists, and that finite mass distributions with constant surface density must have zero ''surface tension.'' Finally, an expanding dust-filled universe turns out to be like Milne's model.

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