The Hubble tension: Relativistic dark matter production from long-lived particles

The tension between direct measurements of the Hubble constant and those stemming from Cosmic Microwave Background probes has triggered a multitude of studies. The connection between cosmology and particle physics has shown to be a valuable approach to addressing the Hubble tension. In particular, increasing the number of relativistic degrees of freedom in the early universe helps alleviate the problem. In this work, we write down effective field theory describing relativistic dark matter production in association with neutrinos leading to a larger H 0 . We derive limits on the effective energy scale that governs this relativistic production of dark matter as a function of the dark matter mass for fermion, vector, and scalar dark matter fields. In particular, scalar dark matter particles are more effective in increasing the effective number of relativistic species. Also, if they have GeV scale masses, then the relativistic production of dark matter should be governed by Planck scale effective operators in order to alleviate the Hubble tension. • Effective theories for dark matter production coupled with neutrinos are derived. • Dimension-five operators for the dark matter production channel are constructed. • Limits on the effective energy scale governing the dark matter production are found. • Enhanced constraints on Nef f are considered to address the Hubble tension. • Weak scale masses imply dark matter production governed by Planck scale operators.