Inflation in simple one-loop effective potentials of perturbative quantum gravity
arXiv:2307.02214 · doi:10.1142/S0218271824500287
Abstract
We study inflation in scalar-tensor perturbative quantum gravity driven by a one-loop effective potential. We consider effective potentials generated by three models. The first model describes a single scalar field with a non-vanishing mass. The second model describes a massless scalar field with non-minimal coupling to the Einstein tensor. The third model generalises the Coleman-Weinberg model for the gravitational case. The first model can be consistent with the observational data for e-foldings. The second model can be consistent with the observational data for e-foldings. We did not find parameters that make the generalised Coleman-Weinberg model consistent with the observational data. We discuss the implications of these results and ways to improve them with other terms of effective action.
19 pages, 30 figures. International Journal of Modern Physics, 2024
References in corpus (10)
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- Higgs inflation: consistency and generalisations
- G-inflation: inflation driven by the Galileon field
- Inflation scenario via the Standard Model Higgs boson and LHC
- Recent Advances on Inflation
- A Refined Einstein-Gauss-Bonnet Inflationary Theoretical Framework
- Planck and BICEP/Keck Array 2018 constraints on primordial gravitational waves and perspectives for future B-mode polarization measurements
- Quantum Corrected Scalar Field Inflation
- Effective potential of scalar-tensor gravity with quartic self-interaction of scalar field
- Ruling out an inflation driven by a power law potential: kinetic coupling does not help