Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity
gr-qc, astro-ph.CO, hep-th
Submitted: 2026-05-14
Updated: 2026-08-06
Sources
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- Chameleon Early Dark Energy and the Hubble Tension
- Resolving the Hubble tension with Early Dark Energy
- Double the axions, half the tension: multi-field early dark energy eases the Hubble tension
- Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
- Can interacting dark energy solve the $H_0$ tension?
- Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models
- Observational constraints on one-parameter dynamical dark-energy parametrizations and the $H_0$ tension
- Interacting dark energy with time varying equation of state and the $H_0$ tension
- Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
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