Precision predictions for the primordial power spectra from \(f(R)\) models of inflation
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Publication:318766
DOI10.1016/j.nuclphysb.2016.08.010zbMath1346.83064arXiv1606.05879OpenAlexW2464555872MaRDI QIDQ318766
Sergei D. Odintsov, D. J. Brooker, Richard Woodard
Publication date: 5 October 2016
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1606.05879
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (14)
Inflationary attractors in \(F(R)\) gravity ⋮ Kuchowicz gravastars in the braneworld formalism ⋮ Probing the existence of the ZTF Casimir wormholes in the framework of \(f(\mathcal{R})\) gravity ⋮ On the Trans-Planckian Censorship Conjecture and the generalized non-minimal coupling ⋮ Traversable wormholes with charge and non-commutative geometry in the \(f(Q)\) gravity ⋮ Exact inflationary solutions in exponential gravity ⋮ Constant-roll inflation in F( R ) gravity ⋮ The reconstruction of \(f(\phi)R\) and mimetic gravity from viable slow-roll inflation ⋮ Hubble diagrams in the Jordan and Einstein frames ⋮ Improving the single scalar consistency relation ⋮ \(R^2\) inflation to probe non-perturbative quantum gravity ⋮ Inflation from the finite scale gauged Nambu-Jona-Lasinio model ⋮ Deceleration versus acceleration universe in different frames of \(F(R)\) gravity ⋮ From non-trivial geometries to power spectra and vice versa
Cites Work
- Viable mimetic \(F(R)\) gravity compatible with Planck observations
- Nonperturbative models for the quantum gravitational back-reaction on inflation
- Saddle point inflation from \(f(R)\) theory
- Corrigendum to ``Generating scale-invariant tensor perturbations in the non-inflationary universe [Phys. Lett. B 736 (2014) 488-493]
- A new type of isotropic cosmological models without singularity
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- PARAMETRIZATIONS OF THE DARK ENERGY DENSITY AND SCALAR POTENTIALS
- CURVATURE QUINTESSENCE
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