A Simple Recipe for the 111 and 128 GeV Lines
JiJi Fan, Matthew Reece

TL;DR
This paper proposes a novel dark matter model involving a multiplet of new states near 260 GeV that explains the 111 and 128 GeV gamma-ray lines through decay processes, avoiding large couplings or coincidences.
Contribution
It introduces a simple, symmetry-based dark matter model with a multiplet of states that naturally produce gamma-ray lines and fit observational data without requiring extreme parameters.
Findings
Model explains gamma-ray lines with natural mass degeneracy.
Decay of neutral states produces a box-shaped photon spectrum.
Model evades direct detection and collider constraints.
Abstract
Recently evidence for gamma ray lines at energies of approximately 111 and 128 GeV has been found in Fermi-LAT data from the center of the galaxy and from unassociated point sources. Many explanations in terms of dark matter particle pairs annihilating to gamma gamma and gamma Z have been suggested, but these typically require very large couplings or mysterious coincidences in the masses of several new particles to fit the signal strength. We propose a simple novel explanation in which dark matter is part of a multiplet of new states which all have mass near 260 GeV as a result of symmetry. Two dark matter particles annihilate to a pair of neutral particles in this multiplet which subsequently decay to gamma gamma and gamma Z. For example, one may have a triplet of pseudo-Nambu-Goldstone bosons, charged pions and a neutral pion, where the charged pions are stabilized by their charge…
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