Direct detection of dark matter with resonant annihilation
Bo Li, Yu-Feng Zhou

TL;DR
This paper analyzes the detectability of dark matter particles that annihilate through a resonance, showing that in certain models the scattering cross section can be below neutrino backgrounds, making direct detection challenging.
Contribution
It provides an improved analytical calculation of relic density for resonant dark matter annihilation and explores conditions under which direct detection is feasible.
Findings
For s-wave annihilation, the cross section scales with the resonance width-to-mass ratio.
In p-wave annihilation, the cross section remains above neutrino backgrounds for lighter DM.
The real singlet DM model exemplifies the theoretical findings.
Abstract
In the scenario where the dark matter (DM) particles pair annihilate through a resonance particle , the constraint from DM relic density makes the corresponding cross section for DM-nuclei elastic scattering extremely small, and can be below the neutrino background induced by the coherent neutrino-nuclei scattering, which makes the DM particle beyond the reach of the conventional DM direct detection experiments. We present an improved analytical calculation of the DM relic density in the case of resonant DM annihilation for - and -wave cases and invesitgate the condition for the DM-nuclei scattering cross section to be above the neutrino background. We show that in Higgs-portal type models, for DM particles with -wave annihilation, the spin-independent DM-nucleus scattering cross section is proportional to , the ratio of the decay width and…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Cosmology and Gravitation Theories
