Deus ex H 0 -- Is evidence for dynamical dark energy conditioned on early cosmology?
Nils Schöneberg, Rodrigo Calderón, Julien Lesgourgues
astro-ph.CO
Submitted: 2026-08-07
Updated: 2026-08-11
Comments: 6 pages, 6 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Extended Dark Energy analysis using DESI DR2 BAO measurements
- DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data
- Dynamical Dark Energy in light of the DESI DR2 Baryonic Acoustic Oscillations Measurements
- Constraints on neutrino mass and dark energy agnostic to the sound horizon
- Model-Independent Indication for a Localized Anomaly in the Late-Time Expansion History
- DESI and the Hubble tension in light of modified recombination
- Is Dynamical Dark Energy Necessary? DESI BAO and Modified Recombination
- Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO
- SPT-3G D1: Axion Early Dark Energy with CMB experiments and DESI
- Disentangling cosmic distance tensions with early and late dark energy
- The H 0 world cup. II. A comprehensive competition between proposed Hubble tension solutions
- The BAO scale -- how standard is the standard ruler?
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Phantom-Crossing Dark Energy and the m Tug-of-War
- The $H_0$ Olympics: A fair ranking of proposed models
- Review of Hubble tension solutions with new SH0ES and SPT-3G data
- On the implications of the `cosmic calibration tension' beyond $H_0$ and the synergy between early- and late-time new physics
- Accelerating Universes with Scaling Dark Matter
- Exploring the Expansion History of the Universe
- The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration
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