Secluded Dark Sector and Muon $(g-2)$ in the Light of Fast Expanding Universe

TL;DR

This paper explores how a fast-expanding early universe can accommodate a secluded dark sector that explains the muon g-2 anomaly and dark matter relic density through specific gauge extensions and cosmological phases.

Contribution

It introduces a non-standard cosmological model with a new species affecting expansion, enabling larger dark-visible sector couplings and reconciling dark matter and muon g-2.

Findings

Dark sector couples to mu and tau leptons via kinetic mixing.

Parameter space satisfies relic density and muon g-2 constraints.

Fast expansion allows larger portal couplings than standard cosmology.

Abstract

The lack of information before Big Bang Neucleosynthesis (BBN) allow us to assume the presence of a new species $\phi$ whose energy density redshifts as $a^{-(4+n)}$ where $n>0$ and $a$ is the scale factor. This non-standard cosmological setup facilitates a larger portal coupling $(\epsilon)$ between the dark and the visible sectors even when the two sectors are not in thermal equilibrium. Here, we have considered $U(1)_{L_\mu-L_\tau}\otimes U(1)_X$ gauge extension of the Standard Model (SM) and studied different phases of the cosmological evolution of a thermally decoupled dark sector such as leak-in, freeze-in, reannihilation, and late-time annihilation in the presence of fast expansion. Due to the tree level kinetic mixing between $U(1)_X$ and $U(1)_{L_\mu-L_\tau}$ gauge bosons, the dark sector couples with the $\mu$ and $\tau$ flavored leptons of the SM. We show that in our scenario it is possible to reconcile the dark matter relic density and muon $(g-2)$ anomaly. In particular, we show that for $2\times 10^{-4} \lesssim \epsilon \lesssim 10^{-3}$, $5.5{\rm MeV} \lesssim m_{Z^\prime} \lesssim 200{\rm MeV}$, $n=4$, and $1{\rm TeV} \lesssim m_\chi \lesssim 10{\rm TeV}$ relic density constraint of dark matter, constraint from muon $(g-2)$ anomaly, and other cosmological, astrophysical constraints are satisfied.