Technique - (4) Axion dark matter detection (microwave cavity)

Type: Experimental

Description: Haloscope cavities coupled to quantum-limited JPA/SQUID amplifiers for axion-photon conversion.

Department(s)/lab(s): Physics | Chou Group @ UChicago
Summary:

Develops quantum metrology for ultra-weakly-coupled dark sectors and fundamental physics. Directions: (1) axion dark matter detection using entangled probe state preparation and superconducting qubit QND readout (HAYSTAC, ADMX); (2) dark radiation/energy detection with Cooper-pair box quasiparticle sensors; (3) GW detectors based on high-B-field microwave cavities probing early-universe phase transitions; (4) emergent gauge symmetries in quantum spin liquids. Co-PI DARPA QuSeN (quantum sensing of neutrinos, 2025). Devices/Sensors lead, DOE Quantum Science Center.

Department(s)/lab(s): Physics | Knirck Axion Group @ Harvard
Summary:

Knirck builds novel microwave- and mm-wave-frequency detectors (ADMX resonant cavities, MADMAX dielectric haloscopes, and the broadband BREAD/dish-antenna concept) to search for axion dark matter, explicitly leveraging cutting-edge single-photon quantum sensing to push beyond the standard quantum limit. He describes axion searches as sitting directly at the intersection of particle physics, astrophysics, photonics, and quantum sensing, and is building a new experimental group at Harvard.

Department(s)/lab(s): Physics & Astronomy | Quantum Technologies for Fundamental Physics Group (McDonald Group) @ Manchester
Summary:

McDonald leads the Quantum Technologies for Fundamental Physics (QTFP) theme at CQSE Manchester. Research directions: (1) Manchester Axion Novel Cavity eXperiment (MANCX) — building a cavity haloscope to search for QCD axions and axion-like particles coupling to photons via resonant microwave cavity enhancement at Manchester; (2) Astroparticle theory — superradiance from black holes for ultralight dark matter/axion bounds; neutron star probes of new physics; (3) Dark energy / extended gravity — vacuum energy and Casimir-type effects; (4) High-frequency gravitational waves — novel detection concepts. Workshop chair for Manchester's QTFP international workshop (Jan 2026). Interdisciplinary collaboration with quantum engineers, low-temperature physicists, and particle physicists.

Department(s)/lab(s): Physics | Salemi Lab @ UCB
Summary:

Salemi builds millikelvin-scale microwave-cavity and quantum-sensor-read-out haloscopes to search for axion dark matter, relying on near-quantum-limited amplifiers to detect the vanishingly small signals expected from axion-photon conversion in a magnetic field. The lab is actively recruiting postdocs.