One Loop Corrected Mode Functions for SQED during Inflation
arXiv:gr-qc/0608049 · doi:10.1103/PhysRevD.74.084012
Abstract
We solve the one loop effective scalar field equations for spatial plane waves in massless, minimally coupled scalar quantum electrodynamics on a locally de Sitter background. The computation is done in two different gauges: a non-de Sitter invariant analogue of Feynman gauge, and in the de Sitter invariant, Lorentz gauge. In each case our result is that the finite part of the conformal counterterm can be chosen so that the mode functions experience no significant one loop corrections at late times. This is in perfect agreement with a recent, all orders stochastic prediction.
26 pages, uses LaTeX 2 epsilon, no figures, version 2 has an updated reference list
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Cited by in corpus (49)
- Infrared effects in inflationary correlation functions
- Quantum Stability of a w < - 1 Phase of Cosmic Acceleration
- One-loop corrections to the curvature perturbation from inflation
- One-loop corrections to a scalar field during inflation
- On the One Loop Corrections to Inflation II: The Consistency Relation
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- Quantum Gravity Corrections to the One Loop Scalar Self-Mass during Inflation
- Perturbative Quantum Gravity Comes of Age
- A Maximally Symmetric Vector Propagator
- A Completely Regular Quantum Stress Tensor with
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- The Perils of Analytic Continuation
- Excitation of Photons by Inflationary Gravitons
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- Transforming to Lorentz Gauge on de Sitter
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- Non-linear sigma model in de Sitter space
- Scalar Contribution to the Graviton Self-Energy during Inflation
- Weyl-Weyl Correlator in de Donder Gauge on de Sitter
- Linearized Weyl-Weyl Correlator in a de Sitter Breaking Gauge
- Graviton Corrections to Maxwell's Equations
- The Coincidence Limit of the Graviton Propagator in de Donder Gauge on de Sitter Background
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- Covariant Vacuum Polarizations on de Sitter Background
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- The Quantum Corrected Mode Function and Power Spectrum for a Scalar Field during Inflation
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- Even the photon propagator must break de Sitter symmetry
- Inflaton Effective Potential from Photons for General
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- Longitudinal Doppler effect in de Sitter expanding universe
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