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29–31 May 2024
Wilson Hall
America/Chicago timezone

Low Tc Hafnium Kinetic Inductance Device for Dark Matter Search

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

2nd Floor Crossover

Wiilson Hall

Description

Closely related but contrary to Qubits, dark matter detectors are built to be ultra-sensitive to phonons created from impacts in the substrate. TESs have been successfully implemented as phonon sensors on gram-scale detectors. Kinetic inductance devices (KIDs) are naturally suitable for multiplexing readout, which can scale detectors to kilogram scale.
At LBL we focus on low Tc Hafnium KIDs R&D for phonon sensing. 250mK Tc resonators with internal quality factors exceeding 10^5 have been demonstrated. Low Tc not only yields more quasiparticles per unit energy, but also enables quasiparticle trapping from aluminum phonon absorbers. This technique will lead to sub-eV energy threshold kilogram scale dark matter detectors.

Primary authors

Aritoki Suzuki (Lawrence Berkeley National Laboratory) Xinran Li (Lawrence Berkeley national laboratory) Maurice Garcia-Sciveres (LBNL)

Presentation materials

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