To CPL, or not to CPL? What we have not learned about the dark energy equation of state
astro-ph.CO, gr-qc, hep-ph, hep-th
Submitted: 2025-03-28
Updated: 2026-09-01
Code: https://github.com/snesseris/DESI_CPL
Terminology
Sources
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
- The Cosmological Constant Problem: Why it's hard to get Dark Energy from Micro-physics
- Dynamics of dark energy
- De Sitter Space and the Swampland
- Accelerating Universes with Scaling Dark Matter
- Exploring the Expansion History of the Universe
- The Dynamics of Quintessence, The Quintessence of Dynamics
- Interpreting Dark Energy Data Away from $\Lambda$
- Parameterization of Dark-Energy Properties: a Principal-Component Approach
- Expansion-history preferences of DESI DR2 and external data
- Nonparametric reconstructions of dynamical dark energy via flexknots
- Reconstructing the dark energy density in light of DESI BAO observations
- Comparison of dynamical dark energy with {\Lambda}CDM in light of DESI DR2
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
- Planck 2018 results. VI. Cosmological parameters
- Robust and model-independent cosmological constraints from distance measurements
- A tale of two (or more) $h$'s
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