Revisiting the Hubble tension with an inverse power-law early dark energy
astro-ph.CO, hep-th
Submitted: 2026-08-27
Updated: 2026-09-04
Code: https://github.com/lesgourg/class_publichttps:
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder
- The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023
- Early Dark Energy Can Resolve The Hubble Tension
- Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
- Rock 'n' Roll Solutions to the Hubble Tension
- Unified framework for Early Dark Energy from $\alpha$-attractors
- New Early Dark Energy
- Resolving the Hubble Tension with New Early Dark Energy
- Hot New Early Dark Energy
- Hot New Early Dark Energy: Towards a Unified Dark Sector of Neutrinos, Dark Energy and Dark Matter
- Profiling Cold New Early Dark Energy
- Hot New Early Dark Energy bridging cosmic gaps: Supercooled phase transition reconciles (stepped) dark radiation solutions to the Hubble tension with BBN
- Hot New Early Dark Energy: Dark Radiation Matter Decoupling
- Double the axions, half the tension: multi-field early dark energy eases the Hubble tension
- Ultralight Scalar Decay and the Hubble Tension
- Towards Early Dark Energy in String Theory
- Constraints on Early Dark Energy from the Axion Weak Gravity Conjecture
- Cosmological implications of ultra-light axion-like fields
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation