Looking for the WIMP Next Door

TL;DR

This paper investigates minimal hidden sector dark matter models, especially WIMPs next door, analyzing their cosmological history, experimental signals, and how current experiments probe their parameter space.

Contribution

It introduces a minimal, predictive cosmology for hidden sector dark matter with thermal equilibrium, and maps out the experimentally accessible parameter space for WIMPs next door.

Findings

The thermalization floor for portal couplings is established as a function of equilibration temperature.

Current direct detection experiments probe the cosmological lower bound in some parameter regions.

Identifies viable parameter space for sub-GeV dark matter detection.

Abstract

We comprehensively study experimental constraints and prospects for a class of minimal hidden sector dark matter (DM) models, highlighting how the cosmological history of these models informs the experimental signals. We study simple "secluded" models, where the DM freezes out into unstable dark mediator states, and consider the minimal cosmic history of this dark sector, where coupling of the dark mediator to the SM was sufficient to keep the two sectors in thermal equilibrium at early times. In the well-motivated case where the dark mediators couple to the Standard Model (SM) via renormalizable interactions, the requirement of thermal equilibrium provides a minimal, UV-insensitive, and predictive cosmology for hidden sector dark matter. We call DM that freezes out of a dark radiation bath in thermal equilibrium with the SM a WIMP next door, and demonstrate that the parameter space for such WIMPs next door is sharply defined, bounded, and in large part potentially accessible. This parameter space, and the corresponding signals, depend on the leading interaction between the SM and the dark mediator; we establish it for both Higgs and vector portal interactions. In particular, there is a cosmological lower bound on the portal coupling strength necessary to thermalize the two sectors in the early universe. We determine this thermalization floor as a function of equilibration temperature for the first time. We demonstrate that direct detection experiments are currently probing this cosmological lower bound in some regions of parameter space, while indirect detection signals and terrestrial searches for the mediator cut further into the viable parameter space. We present regions of interest for both direct detection and dark mediator searches, including motivated parameter space for the direct detection of sub-GeV DM.