Palatini inflationary (non-)attractors: Universal mapping of observables
Abstract
We study single-field slow-roll inflation in the context of Palatini gravity for the class of non-minimally coupled ξ-attractors, i.e.,\ models where the same function f(ϕ) fixes both the non-minimal coupling, 1+ξf(ϕ), and the inflationary potential, V(ϕ) = M4 f(ϕ)2. For an arbitrary f(ϕ), the number of e-folds is, at leading order, independent of ξ. Thanks to this, we provide an immediate mapping between the observables of the non-minimally coupled setup and those of the minimally coupled one. In the strong coupling limit, the tensor-to-scalar ratio is, as usual, suppressed, while the scalar spectral index is shifted towards larger values, with the magnitude of the shift depending only on the tensor-to-scalar ratio associated with the original potential V(ϕ).
Related
- Tachyonic Encore: A universal shift of inflationary observables
- Swampland diagnostics and observational tests of the inflationary universe in the Palatini formalism
- Inflationary attractors in metric-affine gravity
- Pulsar Timing Response and Spatial Correlations of Shear Modes in Torsionless Palatini Spacetime
- Gravitational Wave Birefringence in generalized Palatini Chern Simons
BibTeX
@misc{dioguardi2026palatini,
title = {{Palatini inflationary (non-)attractors: Universal mapping of observables}},
author = {Christian Dioguardi and Francesco Gianesello and Antonio Racioppi},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.20622},
eprint = {2609.20622},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.20622},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Palatini inflationary (non-)attractors: Universal mapping of observables
AU - Christian Dioguardi
AU - Francesco Gianesello
AU - Antonio Racioppi
PY - 2026
DA - 2026/09/28
PB - arXiv
DO - 10.48550/arxiv.2609.20622
UR - https://arxiv.org/abs/2609.20622
AB - We study single-field slow-roll inflation in the context of Palatini gravity for the class of non-minimally coupled ξ-attractors, i.e.,\ models where the same function f(ϕ) fixes both the non-minimal coupling, 1+ξf(ϕ), and the inflationary potential, V(ϕ) = M^4 f(ϕ)^2. For an arbitrary f(ϕ), the number of e-folds is, at leading order, independent of ξ. Thanks to this, we provide an immediate mapping between the observables of the non-minimally coupled setup and those of the minimally coupled one. In the strong coupling limit, the tensor-to-scalar ratio is, as usual, suppressed, while the scalar spectral index is shifted towards larger values, with the magnitude of the shift depending only on the tensor-to-scalar ratio associated with the original potential V(ϕ).
ER -