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For the first time we present the general formalism and results of calculation of the two-loop effective action in Einstein quantum gravity on the background M N × T k , where M N is Minkowski space and T k is a k-dimensional torus. We discuss the case of a zero cosmological constant as well as of a nonzero one. The method of calculating variations of the action on a metric tensor and the technique of calculating momentum integrals in dimensional regularization are presented. Some applications to spontaneous compactification are discussed, as well as some prospects.
Buchbinder et al. (Wed,) studied this question.