Hubble tension: a short review of theoretical explanations
Jia-Qi Wang, Zong-Kuan Guo
astro-ph.CO, gr-qc
Submitted: 2026-07-23
Comments: 49 pages, 13 figures, a short review prepared by invitation for RAA special topics
Journal ref: Res. Astron. Astrophys. 26 (2026) 084009
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
- The Hubble Constant
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- The Cosmological Constant and Dark Energy
- Observational Probes of Cosmic Acceleration
- Cosmic Microwave Background Anisotropies
- Planck 2018 results. VI. Cosmological parameters
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- A Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data Set
- The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters
- Tensions between the Early and the Late Universe
- In the Realm of the Hubble tension $-$ a Review of Solutions
- Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- 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
- Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes
- The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
- Absolute Calibration of Cluster Mira Variables to Provide a New Anchor for the Hubble Constant Determination
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