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We exploit a previous computation of the self-mass-squared from quantumgravity to include quantum corrections to the scalar evolution equation. Theplane wave mode functions are shown to receive no significant one loopcorrections at late times. This result probably applies as well to the inflatonof scalar-driven inflation. If so, there is no significant correction to the$\phi \phi$ correlator that plays a crucial role in computations of the powerspectrum.

Scalar Field Equations from Quantum Gravity during Inflation