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Making a connection between observations of cosmological correlation functions and those calculated from theories of the early universe requires that these quantities are conserved through the periods of the universe which we do not understand.
R. L. Arnowitt, S. Deser, and C. W. Misner, (1962), gravitation: an introduction to current research, Louis Witten ed. (Wilew 1962), chapter 7, pp 227-265, arXiv:gr-qc/0405109 [gr-qc]
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