Models with Non-minimal Coupling in Primordial Universe and Cosmological Observations
Alireza Talebian, Hassan Firouzjahi, Fereshteh Felegary
astro-ph.CO, gr-qc, hep-th
Submitted: 2026-07-14
Comments: 24 pages, 7 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- Planck 2018 results. X. Constraints on inflation
- Fractional attractors in light of the latest ACT observations
- The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters
- The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models
- Minimal but non-minimal inflation and electroweak symmetry breaking
- The Palatini side of inflationary attractors
- New universal attractor in nonmininally coupled gravity: Linear inflation
- A minimal model of inflation and dark radiation
- Non-minimal (self-)running inflation: metric vs. Palatini formulation
- Dynamically induced Planck scale and inflation in the Palatini formulation
- Scale-invariance, dynamically induced Planck scale and inflation in the Palatini formulation
- Multiple point criticality principle and Coleman-Weinberg inflation
- Pseudo-Goldstone dark matter in a radiative inverse seesaw scenario
- Symmetry-breaking inflation in non-minimal metric-affine gravity
- $\tilde\xi$-attractors in metric-affine gravity
- Natural Metric-Affine Inflation
- Natural inflation in Palatini $F(R,X)$
- Generalized Hilltop Inflation
- The Standard Model Higgs boson as the inflaton
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