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Gamma-ray lines may reveal the CP nature of the dark matter particle

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arxiv 1810.07068 v1 pith:SGPYSJC4 submitted 2018-10-16 hep-ph

Gamma-ray lines may reveal the CP nature of the dark matter particle

classification hep-ph
keywords darkmattergammaparticlelinesnaturepropertiesdecay
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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abstract

Determining the fundamental properties of the dark matter is one of the most important open problems in particle physics today. If the dark matter particle has spin zero, one of these properties is its CP nature. That is, whether it is CP-even (scalar), CP-odd (pseudoscalar), or if its interactions violate CP. In this paper, we show that the observation of $\gamma$-ray lines arising from the decay of a spin-zero dark matter particle could be used to discriminate among these possibilities. We consider a general setup where dark matter decay is induced by effective operators and demonstrate that, due to gauge invariance, there exists correlations among the branching ratios into gauge boson final states ($\gamma\gamma$, $\gamma Z$, $W^+W^-$, $ZZ$) that depend on the mass and the CP properties of the dark matter. Consequently, the future observation of $\gamma$-ray lines may in principle be used to establish the CP nature of the dark matter particle.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO

    hep-ph 2025-09 conditional novelty 4.0

    Using CTAO projected line sensitivity, the paper forecasts lower bounds on effective dark matter interaction scales above 10 TeV for TeV mass dark matter, with direct detection dominating the fermionic dipole operator.