Multi-component dark matter and Galactic 511 keV ${\hat{I}}^3$-ray emission

Abstract

We study multi-component dark matter scenarios and the Galactic 511 keV ${\hat{I}}^3$-ray emission line signal in the framework of a local, dark $U(1{)}_D$ extension of the Standard Model. A light vector dark matter particle associated with the dark $U(1{)}_D$ may decay and annihilate to electron-positron pairs. The produced positrons may in turn form positroniums that subsequently annihilate to two photons, accounting for the observed line signal of the Galactic 511 keV ${\hat{I}}^3$-ray emission. Three scenarios are investigated. First, we consider the minimal $U(1{)}_D$ extension where a dark gauge boson and a dark Higgs boson are newly introduced to the particle content. As a second scenario, we consider WIMP-type dark matter with the introduction of an extra dark fermion which, in addition to the dark gauge boson, may contribute to the dark matter relic abundance. It is thus a multi-component dark matter scenario with a UV-complete dark $U(1{)}_D$ symmetry. In particular, the vector dark matter may account for a small fraction of the total dark matter relic abundance. Finally, we consider the scenario where the dark matter particles are of the FIMP-type. In this case, both the light vector and fermion dark matter particles may be produced via the freeze-in and super-WIMP mechanisms. Considering theoretical and observational constraints, we explore the allowed parameter space where the Galactic 511 keV ${\hat{I}}^3$-ray line signal and the dark matter relic can both be explained. We also discuss possible observational signatures.

v1: 29 pages, v2: 31 pages, JHEP-accepted version