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The cosmic field tensor in bimetric general relativity
Foundations of Physics 15 (3):379-386 (1985)
Abstract
We construct all cosmic field tensors which are symmetric rank-two tensor concomitants of a metric and a background metric and which have zero divergence when the background metric satisfies the generalized De Donder condition. The resulting background cosmic field represents an Einstein space-timeMy notes
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References found in this work
General relativity with a background metric.Nathan Rosen - 1980 - Foundations of Physics 10 (9-10):673-704.
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