Inflationary predictions of double-well, Coleman-Weinberg, and hilltop potentials with non-minimal coupling
From MaRDI portal
Publication:5023767
DOI10.1088/1475-7516/2018/05/046OpenAlexW2787648312WikidataQ129794682 ScholiaQ129794682MaRDI QIDQ5023767
Ömer Güleryüz, V. N. Şenoğuz, Nilay Bostan
Publication date: 24 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1802.04160
Related Items (12)
Non-minimally coupled quartic inflation with Coleman-Weinberg one-loop corrections in the Palatini formulation ⋮ Non-minimally coupled Natural Inflation: Palatini and Metric formalism with the recent BICEP/Keck ⋮ Realistic inflation in no-scale U(1) R symmetric flipped SU(5) ⋮ On the Trans-Planckian Censorship Conjecture and the generalized non-minimal coupling ⋮ Constraining non-minimally coupled β-exponential inflation with CMB data ⋮ Revisiting Witten-O'Raifeartaigh inflation for a non-minimally coupled scalar field ⋮ Constraints on the non-minimally coupled Witten-O'Raifeartaigh inflation ⋮ Quadratic, Higgs and hilltop potentials in Palatini gravity ⋮ Non-minimal (self-)running inflation: metric vs. Palatini formulation ⋮ Multiple point criticality principle and Coleman-Weinberg inflation ⋮ Palatini double-well and Coleman-Weinberg potentials with non-minimal coupling ⋮ A predictive SO(10) model
Cites Work
- Frame-covariant formulation of inflation in scalar-curvature theories
- On inflation with non-minimal coupling
- Higgs inflation: consistency and generalisations
- Superconformal inflationary \(\alpha\)-attractors
- A new improved energy-momentum tensor.
- Linear inflation from quartic potential
- Cosmology in scalar-tensor gravity.
- Gauged M-flation after BICEP2
- Starobinsky-like inflation from induced gravity
- A new type of isotropic cosmological models without singularity
- Higher order terms in the inflaton potential and the lower bound on the tensor to scalar ratio \(r\)
- MODEL DEPENDENCE OF THE NON-MINIMAL SCALAR-GRAVITON EFFECTIVE COUPLING CONSTANT IN CURVED SPACE-TIME
- Field theories with « Superconductor » solutions
- The Scalar-Tensor Theory of Gravitation
- THE PHASE-SPACE VIEW OF INFLATION I: THE NON-MINIMALLY COUPLED SCALAR FIELD
- Asymptotically safe non-minimal inflation
- Inflation and String Theory
- The Primordial Density Perturbation
- Inflationary universe: A possible solution to the horizon and flatness problems
This page was built for publication: Inflationary predictions of double-well, Coleman-Weinberg, and hilltop potentials with non-minimal coupling