Metastable dark matter mechanisms for INTEGRAL 511 keV $\gamma$ rays and DAMA/CoGeNT events
James M. Cline, Andrew R. Frey, Fang Chen (McGill University)

TL;DR
This paper proposes a dark matter model with nearly degenerate states that can simultaneously explain galactic 511 keV gamma rays, DAMA/LIBRA modulation, and CoGeNT excess, through decay and inelastic scattering mechanisms.
Contribution
It introduces a three-state dark matter framework with specific mass splittings and decay channels, linking astrophysical signals to a simple SU(2) hidden sector model.
Findings
The model reproduces the observed 511 keV gamma-ray distribution.
It accounts for direct detection signals via inelastic scattering.
Predicts a keV X-ray line as an additional signature.
Abstract
We explore dark matter mechanisms that can simultaneously explain the galactic 511 keV gamma rays observed by INTEGRAL/SPI, the DAMA/LIBRA annual modulation, and the excess of low-recoil dark matter candidates observed by CoGeNT. It requires three nearly degenerate states of dark matter in the 4-7 GeV mass range, with splittings respectively of order an MeV and a few keV. The top two states have the small mass gap and transitions between them, either exothermic or endothermic, can account for direct detections. Decays from one of the top states to the ground state produce low-energy positrons in the galaxy whose associated 511 keV gamma rays are seen by INTEGRAL. This decay can happen spontaneously, if the excited state is metastable (longer-lived than the age of the universe), or it can be triggered by inelastic scattering of the metastable states into the shorter-lived ones. We focus…
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