Probing low-mass dark matter from sub-MeV to sub-GeV with germanium-based quantum phononic spectroscopy
D. -M. Mei, N. Budhathoki, S. A. Panamaldeniya, K. -M. Dong, S. Bhattarai, A. Warren, A. Prem, S. Chhetri
TL;DR
This work proposes GeQuLEP, a germanium-based phonon-to-charge sensor that marries a near-surface slow-phonon phononic crystal with RF-QPC readout at 4 K to reach sub-eV thresholds for low-mass dark matter. The authors develop a calibrated efficiency pipeline linking phonon generation, geometric collection, propagation survival, and local capture, enabling selection-corrected thresholds in the $10^{-3}$–$10^{-2}$ eV range and background models informed by timing and GHz PSD windows. Projected sensitivities for DM–electron and DM–nucleon scattering span sub-MeV to sub-GeV DM masses under heavy- and light-mediator benchmarks, with a staged kg·yr plan to approach the solar CEνNS background floor. The work also identifies dominant systematics (threshold, phonon $Q$, and bulk defect densities) and outlines a practical roadmap from cm-scale coupons to kg-scale arrays, highlighting the potential for sub-eV DM discovery and novel solar CEνNS measurements using phonon spectroscopy.
Abstract
We present a germanium phonon-to-charge transducer that integrates a slow-phonon phononic-crystal (PnC) region with radio-frequency quantum point-contact (RF-QPC) readout at 4 K, and we evaluate its dark-sector reach. A calibrated signal-collection model, which combines geometric guiding, propagation survival, and multiplicity-assisted primary-phonon detection, provides selection-corrected thresholds in the $10^{-3}$-$10^{-2}$~eV range and a background model informed by nanosecond timing gates and GHz-band power-spectral-density windows. Under standard halo assumptions, a 100 g module achieves projected sensitivity to DM-electron and DM-nucleon scattering at recoil energies below $10^{-2}$~eV, probing cross sections below $10^{-43}\,\mathrm{cm}^{2}$ for $m_χ\in [0.01,100]~\mathrm{MeV}/c^{2}$ (with efficiencies and thresholds folded in). We present sensitivities for both heavy-mediator ($F_{\rm DM}=1$) and light-mediator ($F_{\rm DM}\propto 1/q^{2}$) benchmarks, quantify dominant systematics (threshold, phonon quality factor $Q$, and bulk defect densities), and outline a staged program toward kg$\cdot$yr exposures that begins to test models approaching the solar CE$ν$NS background.
