Quintessential Inflation in Palatini gravity
arXiv:2503.21610 · doi:10.1140/epjp/s13360-025-07025-1
Abstract
Palatini gravity, with the inflaton kinetic term, proved to be a powerful framework for generating asymptotically flat inflaton potentials. Here we show that a quadratic Palatini restores compatibility with the observational data of the Peebles-Vilenkin quintessential inflation model. Moreover, the same can be achieved with an exponential version of the Peebles-Vilenkin potential if embedded in a Palatini of order higher than two.
12 pages, 5 figures, 3 tables, matches the published version
References in corpus (20)
- Dynamics of dark energy
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- Inflation with Non-Minimal Coupling: Metric vs. Palatini Formulations
- Ricci Reheating
- CMB constraints on the inflaton couplings and reheating temperature in -attractor inflation
- Warm Quintessential Inflation
- Gravitational reheating in quintessential inflation
- Hubble-induced phase transitions on the lattice with applications to Ricci reheating
- Curvaton reheating allows TeV Hubble scale in NO inflation
- A review of Quintessential Inflation
- Quintessential inflation in Palatini gravity
- Palatini Quintessential Inflation
- Quintessential inflation: A tale of emergent and broken symmetries
- Implications of Palatini gravity for inflation and beyond
- What is needed of a scalar field if it is to unify inflation and late time acceleration ?
- Quintessence in the Weyl-Gauss-Bonnet model
- Palatini : a new framework for inflationary attractors
- Beyond (and back to) Palatini quadratic gravity and inflation
- Natural inflation in Palatini