Dark Matter Direct Detection in Materials with Spin-Orbit Coupling

Abstract

Semiconductors with $\mathcal{O}(\text{meV})$ band gaps have been shown to be promising targets to search for sub-MeV mass dark matter (DM). In this paper we focus on a class of materials where such narrow band gaps arise naturally as a consequence of spin-orbit coupling (SOC). Specifically, we are interested in computing DM-electron scattering and absorption rates in these materials using state-of-the-art density functional theory (DFT) techniques. To do this, we extend the DM interaction rate calculation to include SOC effects which necessitates a generalization to spin-dependent wave functions. We apply our new formalism to calculate limits for several DM benchmark models using an example ZrTe${}_5$ target and show that the inclusion of SOC can substantially alter projected constraints.

16 pages, 6 figures

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• Linear response theory for light dark matter-electron scattering in materials
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• Plasmon-enhanced Direct Detection Method for Boosted sub-MeV Dark Matter
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• The Non-Relativistic Effective Field Theory Of Dark Matter-Electron Interactions
• The linear response theory approach to the sub-GeV dark matter in the Sun
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