The Inflaton Effective Potential for General
arXiv:1908.03814 · doi:10.1103/PhysRevD.102.025024
Abstract
We develop an analytic approximation for the coincidence limit of a massive scalar propagator in an arbitrary spatially flat, homogeneous and isotropic geometry. We employ this to compute the one loop corrections to the inflaton effective potential from a quadratic coupling to a minimally coupled scalar. We also extend the Friedmann equations to cover potentials that depend locally on the Hubble parameter and the first slow roll parameter.
arXiv comment21 pages, 9 figures, uses LaTeX 2e. Version 2 revised for publication, including 2 new figures and 6 pages of new text to show, among other things, that our approximations apply as well to plateau potentials
References in corpus (21)
- Inflationary paradigm in trouble after Planck2013
- Stochastic Inflationary Scalar Electrodynamics
- Inflationary paradigm after Planck 2013
- Generation of fluctuations during inflation: comparison of stochastic and field-theoretic approaches
- Leading Log Solution for Inflationary Yukawa
- Inflationary schism after Planck2013
- One Loop Graviton Self-Energy In A Locally De Sitter Background
- Quantum Gravity Corrections to the One Loop Scalar Self-Mass during Inflation
- Scalar Field Equations from Quantum Gravity during Inflation
- Precision Predictions for the Primordial Power Spectra from f(R) Models of Inflation
- Reheating Closed String Inflation
- The Hubble Effective Potential
- Cosmological Coleman-Weinberg Potentials and Inflation
- Fine Tuning May Not Be Enough
- Computing the Primordial Power Spectra Directly
- Precision Predictions for the Primordial Power Spectra of Scalar Potential Models of Inflation
- Final Thoughts on the Power Spectra of Scalar Potential Models
- Ricci Subtraction for Cosmological Coleman-Weinberg Potentials
- Inflaton Effective Potential from Photons for General
- From Non-trivial Geometries to Power Spectra and Vice Versa
- Non-Gaussianity from Features
Cited by in corpus (9)
- Ricci Subtraction for Cosmological Coleman-Weinberg Potentials
- Inflaton Effective Potential from Photons for General
- Coincident Massless, Minimally Coupled Scalar Correlators on General Cosmological Backgrounds
- When tadpoles matter: One-loop corrections for spectator Higgs in inflation
- Inflaton Effective Potential from Fermions for General
- Photon propagator for inflation in the general covariant gauge
- Reheating with Effective Potentials
- Perturbative Quantum Gravity Induced Scalar Coupling to Electromagnetism
- K-Essence Induced by Derivative Couplings of the Inflaton