Recoupled Dark Radiation reconciling CMB and DESI BAO measurements

TL;DR

This paper proposes a recoupled dark radiation model involving sterile neutrinos to reconcile discrepancies between CMB, DESI BAO measurements, and laboratory bounds, improving cosmological fits.

Contribution

It introduces a novel interacting sterile neutrino scenario that alleviates tensions in cosmological data and provides a better fit to observations than standard models.

Findings

Preference for a nonzero interacting sterile neutrino component at 2.7 sigma

Model reduces tension with SH0ES Hubble constant measurement to 2.4 sigma

Improves fit to combined CMB and DESI BAO data with a delta chi-squared of -8.98

Abstract

Recent DESI BAO measurements, combined with CMB data, reveal a tension within the $\Lambda$CDM model that leads to a discrepancy between cosmological and laboratory bounds on the summed neutrino mass. We show that a recoupled interacting radiation component can alleviate this cosmological tension, as well as the one with neutrino oscillation experiments. Sterile neutrinos interacting through a light pseudoscalar mediator provide a concrete realization of this scenario. The resulting interacting fluid modifies the CMB phenomenology, lowers the preferred matter density, and improves the consistency between CMB and DESI BAO measurements. Combining CMB with DESI DR2 BAO measurements, we find a $2.7 \sigma$ preference for a nonzero interacting sterile neutrino component, $\nsp=0.253 \pm 0.094$, corresponding to an improvement $\Delta \chi^2=-8.98$ relative to $\Lambda$CDM. The model also reduces the tension with the SH0ES determination of the Hubble constant to the $2.4\sigma$ level.