Saddle point inflation from \(f(R)\) theory

DOI10.1016/j.physletb.2015.09.076zbMath1364.83028arXiv1508.05150OpenAlexW1888758454MaRDI QIDQ2357328

Zygmunt Lalak, Marek Lewicki, Michal Artymowski

Publication date: 13 June 2017

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1508.05150

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items (4)

Endlessly flat scalar potentials and \(\alpha\)-attractors ⋮ Precision predictions for the primordial power spectra from \(f(R)\) models of inflation ⋮ Implications of extreme flatness in a general \(f(R)\) theory ⋮ Multi-phase induced inflation in theories with non-minimal coupling to gravity

Cites Work

• \(f(R)\) theories
• A new type of isotropic cosmological models without singularity
• Slow-roll inflation in the ( R + R ⁴ ) gravity

This page was built for publication: Saddle point inflation from \(f(R)\) theory