Partial Relief of the Hubble Tension and a Natural Self-Interacting Dark Matter Candidate From Staged Symmetry Breaking

TL;DR

This paper proposes a dark matter model with staged symmetry breaking that partially alleviates the Hubble tension and introduces a self-interacting dark matter candidate with a velocity-dependent cross section, addressing multiple cosmological issues.

Contribution

It introduces a novel dark sector symmetry breaking mechanism that modifies dark matter properties and provides a plausible UV-complete effective field theory.

Findings

Partial reduction of the Hubble tension due to dark matter decay dynamics.

Identification of a self-interacting dark matter candidate with velocity-dependent interactions.

Potential resolution of small-scale structure problems like the core-cusp issue.

Abstract

The values of the Hubble constant ($\rm{H_0}$) inferred from the cosmic microwave background (CMB) and local measurements via the distance ladder exhibit a $\sim5\sigma$ tension. In this work we propose that the tension might be partially alleviated if a subcomponent of the dark matter undergoes decays triggered by spontaneous symmetry breaking in the dark sector, so that the equation of state parameter of the subcomponent shifts from $w \approx 0$ at early times to $w \approx -1/3$ at late times. We provide an effective field theory whose structure is partially motivated by the desire for a plausible UV completion. We find that such a construction naturally produces a possible self-interacting dark matter candidate with a velocity-dependent scattering cross section as a by-product of gauge invariance. This is relevant for addressing tensions between the predictions of $\Lambda$CDM and observations of small-scale structure, such as the core-cusp problem.