Imprint of swampland-inspired coupled early dark energy
Hao Wang, Yun-Song Piao
astro-ph.CO
Submitted: 2026-07-07
Comments: 20 pages, 5 figures
Code: https://github.com/PoulinV/AxiCLASS
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
- DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Accelerating Universes with Scaling Dark Matter
- Exploring the Expansion History of the Universe
- Model independent cosmographic constraints from DESI 2024
- Interpreting DESI's evidence for evolving dark energy
- Does dark energy really revive using DESI 2024 data?
- Does DESI 2024 Confirm $\Lambda$CDM?
- Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
- Dark energy in light of recent DESI BAO and Hubble tension
- Dark energy after pre-recombination early dark energy in light of DESI DR2 and the latest ACT and SPT data
- Quintom cosmology and modified gravity after DESI 2024
- Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
- Assessing observational constraints on dark energy
- A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data
- DESI constraints on the varying electron mass model and axion-like early dark energy
- Cosmological constraints on curved quintessence
- Dynamical dark energy in the light of DESI 2024 data
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