Constant-Roll Inflation in modified gravity model using Palatini Formalism
arXiv:2212.00472 · doi:10.1140/epjc/s10052-023-11459-1
Abstract
In this work, we study a constant-roll inflationary model in the Palatini formalism using modified gravity. Here our action consists a non-minimal coupling of a scalar field with Ricci scalar in a general form of . Using Palatini approach, we write its equivalent scalar-tensor form in the Einstein frame and then apply the constant-roll condition in the equation of motion for the inflaton field. Later the tensor-to-scalar ratio and the spectral index are calculated using the slow-roll parameters and the results obtained are matched with the Planck 2018 data. We found that the results agree nicely with the observations within the parameter regime under consideration.
13 Pages and 10 Figures
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- Investigation of Traversable Wormhole Solutions in Modified Gravity with Scalar Potential
- Coupling Metric-Affine Gravity to the Standard Model and Dark Matter Fermions
- Testing scale-invariant inflation against cosmological data
- Observable Primordial Gravitational Waves from Non-minimally Coupled Palatini Modified Gravity
- Analytical Insights into Constant-Roll Condition: Extending the Paradigm to Non-Canonical Models
- Holographic inflation and holographic dark energy from entropy of the anti-de Sitter black hole
- Constant-roll inflation and primordial black holes within Barrow entropic framework
- Cosmic inflation in metric-affine gravity
- Inflation from a generalized exponential plateau: towards extra suppressed tensor-to-scalar ratios