The Equivalence Principle in the Dark Sector in light of DESI
astro-ph.CO, hep-ph
Submitted: 2026-09-15
Updated: 2026-09-15
Comments: 11 pages, 6 figures, 2 tables
Code: https://github.com/CobayaSampler/cobaya
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Planck 2018 results. VI. Cosmological parameters
- The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters
- SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
- DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
- DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
- DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
- DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
- Extended Dark Energy analysis using DESI DR2 BAO measurements
- DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data
- Interpreting DESI's evidence for evolving dark energy
- Quintom cosmology and modified gravity after DESI 2024
- Assessing observational constraints on dark energy
- Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements
- Matching current observational constraints with nonminimally coupled dark energy
- Preference for evolving dark energy in light of the galaxy bispectrum
- Dynamical Dark Energy in light of the DESI DR2 Baryonic Acoustic Oscillations Measurements
- Assessing cosmological evidence for non-minimal coupling
- Braneworld Dark Energy in light of DESI DR2
- Monodromic Dark Energy and DESI
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