Thermal Friction as a Solution to the Hubble Tension
Kim V. Berghaus, Tanvi Karwal

TL;DR
This paper proposes a particle physics model involving a rolling axion coupled to a non-Abelian gauge group as a new component that can resolve the Hubble tension by behaving like a cosmological constant early on and diluting later.
Contribution
It introduces a natural particle-physics model with a rolling axion that mimics a cosmological constant early and then dilutes, providing a novel solution to the Hubble tension.
Findings
The model behaves like a cosmological constant at early times.
CMB observables are similar for the model and phenomenological fluid approximation.
The model offers a viable particle-physics-based solution to the Hubble tension.
Abstract
A new component added to the standard model of cosmology that behaves like a cosmological constant at early times and then dilutes away as radiation or faster can resolve the Hubble tension. We show that a rolling axion coupled to a non-Abelian gauge group exhibits the behavior of such an extra component at the background level and can present a natural particle-physics model solution to the Hubble tension. We compare the contribution of this bottom-up model to the phenomenological fluid approximation and determine that CMB observables sensitive only to the background evolution of the Universe are expected to be similar in both cases, strengthening the case for this model to provide a viable solution to the Hubble tension.
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