\(\mathcal{R}^2\) quantum corrected scalar field inflation
DOI10.1016/j.nuclphysb.2022.115779zbMath1495.83026arXiv2204.02454OpenAlexW4224961646MaRDI QIDQ2131855
V. K. Oikonomou, Ifigeneia Giannakoudi
Publication date: 27 April 2022
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2204.02454
Unified quantum theories (81V22) String and superstring theories in gravitational theory (83E30) Geometrodynamics and the holographic principle (83E05) Quantization of the gravitational field (83C45) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Lagrangian formalism and Hamiltonian formalism in mechanics of particles and systems (70S05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Conformal structures on manifolds (53C18)
Cites Work
- Unnamed Item
- Black holes, cosmological solutions, future singularities, and their thermodynamical properties in modified gravity theories
- Higgs scalaron mixed inflation
- Unification of constant-roll inflation and dark energy with logarithmic \(R^{{2}}\)-corrected and exponential \(F(R)\) gravity
- Scalaron the healer: removing the strong-coupling in the Higgs- and Higgs-Dilaton inflations
- Power-law \(f(R)\) gravity corrected canonical scalar field inflation
- Canonical scalar field inflation with string and \(R^2\)-corrections
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- A new type of isotropic cosmological models without singularity
- PALATINI APPROACH TO MODIFIED GRAVITY: f(R) THEORIES AND BEYOND
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Higgs-R2 inflation—full slow-roll study at tree-level
- On the covariant formalism of the effective field theory of gravity and leading order corrections
This page was built for publication: \(\mathcal{R}^2\) quantum corrected scalar field inflation
