Galbiati co-leads the DarkSide/Global Argon Dark Matter Collaboration program (DarkSide-20k and successors), developing ultra-radiopure underground argon and cryogenic noble-liquid time-projection chambers for direct WIMP dark-matter detection, building on his earlier work on the Borexino solar-neutrino scintillator experiment. Included as a borderline quantum-sensing entry on the strength of the ultra-low-background, single-quantum (photon/ionization) detection technology his group has developed, which is now being adapted for other applications such as total-body PET imaging.
Experimental astroparticle physicist searching for dark matter with noble liquid detectors. Directions: (1) DarkSide-20k — liquid argon TPC at INFN Gran Sasso targeting WIMP dark matter with 20-tonne active volume; (2) development of cryogenic SiPM photon detection for LAr detectors; (3) low-background detector techniques and radon mitigation; (4) argon purification and light yield optimization. Argonne joint appointment.
Gratta's group works at the interface of atomic and particle physics, developing cold-atom interferometric gravimeters and gradiometers for tests of gravity alongside searches for neutrinoless double-beta decay using liquid-xenon TPCs (EXO-200/nEXO), spanning quantum sensing hardware and rare-event particle detection.
Hobson co-leads the Ultracold Strontium Laboratory within the AION atom-interferometer collaboration, developing squeezed strontium atomic ensembles and quantum-non-demolition measurement techniques to beat the standard quantum limit in long-baseline atom-interferometric searches for dark matter and gravitational waves, alongside a parallel programme on ultra-precise, shock-resistant optical clocks. Actively recruiting postdocs as the group builds out its cold-atom laboratories.
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.
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.
Best known as a collider (ATLAS) physicist, Miller also leads the BREAD collaboration's broadband dish-antenna search for axion dark matter, converting axions to photons inside a solenoid magnet and reading them out with a THz receiver and Fourier-transform spectrometer to cover mass ranges inaccessible to narrowband cavity haloscopes. This is a fundamentally different quantum-sensing strategy than solid-state NV-ensemble magnetometers/thermometers, which reach pT/sqrt(Hz)-class sensitivity via DEER, NMR, and T1-relaxometry protocols on spin ensembles; Miller's approach instead pushes broadband photon-counting sensitivity for fundamental-physics searches. Actively recruiting postdocs for BREAD instrumentation and analysis.
O'Hare is a dark-matter phenomenologist whose work sits unusually close to instrumentation: he is the principal theorist of the 'neutrino fog' that limits direct-detection experiments, of directional dark matter detection (using the daily modulation of the WIMP wind to distinguish signal from background), and of the axion and ultralight dark-matter searches that increasingly rely on quantum sensors — haloscopes, comagnetometers, NMR-based searches and atomic magnetometers. He writes the sensitivity projections that tell experimentalists which quantum sensor to build. Positioned against the established body of NV-ensemble quantum sensing work — DEER, nanoscale NMR and T1 relaxometry protocols operating at pT/sqrt(Hz) field sensitivity — the axion/ALP search programme he works on consumes spin-ensemble magnetometry directly: CASPEr-class experiments are, in effect, precision NMR magnetometers operating far below pT/sqrt(Hz), and his phenomenology sets the sensitivity targets they aim at. Theory PI with strong experimental engagement.
Oberlack leads Mainz's contribution to the XENON/XENONnT dual-phase liquid-xenon dark-matter programme at Gran Sasso, covering detector instrumentation, ultra-low-background material screening, light and charge readout, and the associated rare-event analysis; the same detectors also probe neutrinoless double beta decay and coherent neutrino scattering. Relative to the established NV-ensemble quantum-sensing playbook (DEER, nanoscale NMR, T1 relaxometry at pT/sqrt(Hz) ensemble sensitivity), this is an astro-particle pivot: the shared discipline is single-quantum detection at absurd background rejection, and the group is a natural landing spot for a quantum-sensing postdoc interested in low-background readout electronics or in the growing overlap between quantum sensors and dark-matter searches.
Pop's group builds superconducting quantum circuits from high-kinetic-inductance materials, above all granular aluminium, and uses them as detectors. The distinctive capability is single-microwave-photon detection and QND photon counting with superinductor-based devices -- an extremely low dark-count, quantum-limited receiver in the GHz band -- plus fluxonium-type qubits, quantum-limited and travelling-wave parametric amplification, and studies of quasiparticle and noise mechanisms that set coherence limits. The direct sensing payoff is dark-matter search: a photon counter that beats the standard quantum limit lets a haloscope integrate far faster than an amplifier-based readout. Relative to the established NV-ensemble quantum-sensing playbook (DEER, nanoscale NMR, T1 relaxometry at pT/sqrt(Hz) ensemble sensitivity), this is the microwave/superconducting counterpart to an NV ensemble -- same objective (detect an absurdly weak field), different physical platform and roughly opposite temperature regime. A recent addition to Stuttgart's 1st Institute of Physics, so the lab is being built out now, which usually means unusual latitude for a postdoc.