The cosmic field tensor in bimetric general relativity

Foundations of Physics 15 (3):379-386 (1985)
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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-time

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10.1007/bf00737325

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General relativity with a background metric.Nathan Rosen - 1980 - Foundations of Physics 10 (9-10):673-704.

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