Unification of polynomial and exponential cosmological attractors
hep-th, astro-ph.CO, gr-qc, hep-ph
Submitted: 2026-07-08
Updated: 2026-09-05
Comments: 3 page, 2 figures, reference added
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Minimal Supergravity Models of Inflation
- Superconformal Inflationary $\alpha$-Attractors
- The Standard Model Higgs boson as the inflaton
- SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
- Inflation at the End of 2025: Constraints on $r$ and $n_s$ Using the Latest CMB and BAO Data
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters
- The BAO-CMB Tension and Implications for Inflation
- The spectrum of $n_s$ constraints from DESI and CMB data
- Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension
- On the Present Status of Inflationary Cosmology
- Mutated Hybrid Inflation
- Brane Inflation
- Towards Inflation in String Theory
- Encyclopaedia Inflationaris
- The Unity of Cosmological Attractors
- Planck 2018 and Brane Inflation Revisited
- Generalized Pole Inflation: Hilltop, Natural, and Chaotic Inflationary Attractors
- CMB targets after the latest Planck data release
- Polynomial $\alpha$-attractors
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