Cosmic inflation as a renormalization-group flow: the running of power spectra in quantum gravity
From MaRDI portal
Publication:5025289
DOI10.1088/1475-7516/2021/01/048zbMath1484.83095arXiv2007.15023OpenAlexW3126592022MaRDI QIDQ5025289
Publication date: 1 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2007.15023
Unified quantum theories (81V22) Relativistic cosmology (83F05) Quantization of the gravitational field (83C45) Renormalization group methods applied to problems in quantum field theory (81T17) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (3)
Renormalization-group techniques for single-field inflation in primordial cosmology and quantum gravity ⋮ High-order corrections to inflationary perturbation spectra in quantum gravity ⋮ Perturbation spectra and renormalization-group techniques in double-field inflation and quantum gravity cosmology
Cites Work
- Unnamed Item
- Unnamed Item
- \(f(R)\) theories
- A new formulation of Lee-Wick quantum field theory
- On the quantum field theory of the gravitational interactions
- Running of the scalar spectral index and observational signatures of inflation
- Quantum gravity, fakeons and microcausality
- The ultraviolet behavior of quantum gravity
- Fakeons and Lee-Wick models
- Predictions of quantum gravity in inflationary cosmology: effects of the Weyl-squared term
- A new type of isotropic cosmological models without singularity
- Fakeons and the classicization of quantum gravity: the FLRW metric
- Fakeons, microcausality and the classical limit of quantum gravity
- Universality in generalized models of inflation
- Renormalization-group running induced cosmic inflation
- Inflationary universe: A possible solution to the horizon and flatness problems
- On the running of the spectral index to all orders: a new model-dependent approach to constrain inflationary models
- The density perturbation power spectrum to second-order corrections in the slow-roll expansion
This page was built for publication: Cosmic inflation as a renormalization-group flow: the running of power spectra in quantum gravity
