Composite magnetic dark matter and the 130 GeV line
James M. Cline, Andrew R. Frey, Guy D. Moore

TL;DR
This paper proposes a composite dark matter model with a magnetic dipole moment to explain the 130 GeV gamma-ray line, predicting specific collider signatures and addressing challenges in model realization.
Contribution
It introduces a novel composite dark matter model with a large magnetic dipole moment to account for the gamma-ray line, highlighting its naturalness and collider implications.
Findings
Dark matter with a magnetic dipole can explain the 130 GeV line.
Predicted collider signature includes 4-photon events from bound state decays.
Model faces challenges in achieving the required dipole moment.
Abstract
We propose an economical model to explain the apparent 130 GeV gamma ray peak, found in the Fermi/LAT data, in terms of dark matter annihilation through a dipole moment interaction. The annihilating dark matter particles represent a subdominant component, with mass density 7-17% of the total DM density; and they only annihilate into gamma gamma, gamma Z, and ZZ, through a magnetic (or electric) dipole moment. Annihilation into other standard model particles is suppressed, due to a mass splitting in the magnetic dipole case, or to p-wave scattering in the electric dipole case. In either case, the observed signal requires a dipole moment of strength mu ~ 2/TeV. We argue that composite models are the preferred means of generating such a large dipole moment, and that the magnetic case is more natural than the electric one. We present a simple model involving a scalar and fermionic…
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