Alleviating the Hubble tension with the omega s CDM model

arXiv:2606.17749 · astro-ph.CO, gr-qc · Submitted 2026-06-16 · Read on arXiv

Youri Carloni

astro-ph.CO, gr-qc

Submitted: 2026-06-16

Comments: Proceeding AstroMarche2 conference, September 2025, Accepted for publication in IJMPA, 7 pages, 2 figures, 1 table

Code: https://github.com/YouriCarloni/LwsCLASS

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Hubble Tension — 17× in this paper · explained in 9 episodes
• Monte Carlo Analysis — 5× in this paper · explained in 2 episodes
• Calibration — 2× in this paper · explained in 7 episodes
• Clustering — 1× in this paper · explained in 2 episodes
• Gravitational Lensing — 1× in this paper · explained in 2 episodes
• Quintessence — 1× in this paper · explained in 2 episodes

Sources

• Resolving the Hubble tension at late times with Dark Energy
• Solving the Hubble tension at intermediate redshifts with dynamical dark energy
• A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension

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