Lower Limits on the Strengths of Gamma Ray Lines from WIMP Dark Matter Annihilation
Kevork N. Abazajian, Prateek Agrawal, Zackaria Chacko, Can Kilic

TL;DR
This paper derives fundamental lower bounds on the ratio of gamma ray line strength to continuum in dark matter annihilation, based on unitarity, providing model-independent constraints relevant for interpreting gamma ray signals.
Contribution
It establishes exact lower bounds on gamma ray line strengths relative to continuum for dark matter models, using unitarity relations, applicable under specific symmetry and annihilation conditions.
Findings
Lower bounds depend on dark matter mass and spin.
Results agree with MSSM predictions.
Bounds translate into upper limits on annihilation cross sections.
Abstract
We study the spectra of gamma ray signals that arise from dark matter annihilation in the universe. We focus on the large class of theories where the photon spectrum includes both continuum spectrum of gamma rays that arise from annihilation into Standard Model states at tree level, as well as monochromatic gamma rays arising from annihilation directly into two photons at the one loop level. In this class of theories we obtain lower bounds on the ratio of the strength of the gamma ray line relative to the gamma ray continuum as a function of the dark matter mass and spin. These limits are obtained from the unitarity relation between the tree level amplitude of the primary annihilation channel and the imaginary part of the loop level amplitude for annihilation directly into photons, with the primary decay products running in the loop. These results are exact in the limit that dark matter…
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