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The path integral, which generates in-in correlation functions of a scalar field in a cosmological spacetime, is shown to admit nontrivial classical solutions as stationary phases.
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V. K. Onemli and R. P. Woodard, Quantum effects can render ω < − 1 \omega<-1 on cosmological scales, Phys. Rev. D 70 (2004) 107301, gr-qc/0406098
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R. P. Woodard, Generalizing Starobinskii’s Formalism to Yukawa Theory & to Scalar QED, J. Phys. Conf. Ser. 68 (2007) 012032, gr-qc/0608037
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