Scalar field equations from quantum gravity during inflation

E. O. Kahya and R. P. Woodard
Phys. Rev. D 77, 084012 – Published 15 April 2008

Abstract

We exploit a previous computation of the self-mass-squared from quantum gravity to include quantum corrections to the scalar evolution equation. The plane wave mode functions are shown to receive no significant one loop corrections at late times. This result probably applies as well to the inflaton of scalar-driven inflation. If so, there is no significant correction to the φφ correlator that plays a crucial role in computations of the power spectrum.

  • Received 29 October 2007

DOI:https://doi.org/10.1103/PhysRevD.77.084012

©2008 American Physical Society

Authors & Affiliations

E. O. Kahya* and R. P. Woodard

  • Department of Physics, University of Florida, Gainesville, Florida 32611, USA

  • *emre@phys.ufl.edu
  • woodard@phys.ufl.edu

See Also

Completely regular quantum stress tensor with w<1

E. O. Kahya, V. K. Onemli, and R. P. Woodard
Phys. Rev. D 81, 023508 (2010)

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Vol. 77, Iss. 8 — 15 April 2008

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