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29–31 May 2024
Wilson Hall
America/Chicago timezone

Development of qubit-based light dark matter detector on sapphire substrate

Not scheduled
20m
2nd Floor Crossover (Wiilson Hall)

2nd Floor Crossover

Wiilson Hall

Description

One of the challenges in exploring target materials for dark matter searches is the detection of sub-eV energy excitations from light dark matter interaction with a target material. Dark matter interaction can excite sub-eV optical phonon modes in polar materials like sapphire. Furthermore, the anisotropy of sapphire crystal could provide a signature of daily modulation of the dark matter scattering rate, making it a promising target material. We plan to utilize superconducting qubits on a sapphire substrate to detect the scattering events by taking advantage of the excitation of phonons, which scatter and further down-convert to lower-energy phonons. A good fraction of these phonons are expected to reach the qubit superconductor on the substrate and break Cooper pairs. Such a process can cause qubit decoherence, which can be measured using standard qubit readout protocol. This poster describes our ongoing development of a prototype detector.

Primary author

Kester Anyang (Illinois Institute of Technology)

Presentation materials

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