Experimental astroparticle physicist developing novel quantum-limited detectors for dark matter and neutrino sensing. Directions: (1) COHERENT experiment — first measurement of coherent elastic neutrino-nucleus scattering (CEvNS) and ongoing precision measurements; (2) bubble chamber and scintillating bolometer detectors for WIMP dark matter; (3) development of low-threshold detectors sensitive to sub-GeV dark matter; (4) nuclear recoil sensing at the few-eV threshold. Enrico Fermi Institute member.

Fruth is an experimentalist on LZ, the world-leading liquid-xenon dark matter experiment, and works on the detector-physics end: electron and single-photon backgrounds, calibration, and the characterisation of the anomalous low-energy events that currently limit sensitivity at the bottom of the energy spectrum. The programme is a pure exercise in pushing a detector's noise floor down until it is limited by irreducible physics (the neutrino fog). 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 — dark matter detection and NV-ensemble magnetometry are the same problem in different clothing — an exquisitely quiet detector, a signal below the background, and a systematics budget that determines everything — and the quantum-sensing community is increasingly supplying the readout technology (quantum-limited amplifiers, single-photon counters) that these experiments now need. Early-career PI.

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.

Directs the Wisconsin IceCube Particle Astrophysics Center (WIPAC); works on IceCube and next-generation neutrino telescope instrumentation for high-energy astroparticle physics.

Jamieson's group built the counted single-ion implantation capability that underpins every donor spin qubit made at UNSW and Melbourne: individual P, Sb or Bi ions are implanted into silicon through a nanoscale aperture while on-chip detector electrodes register the electron-hole pairs from each ion stop event, so the number and position of dopants is known rather than assumed. Recent directions extend this to high-atomic-number donors for nuclear-spin qudits, to colour-centre creation in diamond and silicon carbide by counted implantation, and to characterising the damage and charge environment those ions leave behind. The work is fabrication-forward but its scientific content is single-particle detection metrology. 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 — his contribution is upstream: the deterministic creation and validation of the very spin defects whose ensembles are later interrogated by DEER and nanoscale NMR at pT/sqrt(Hz).

Astroparticle physicist and long-time IceCube collaborator, working on high-energy neutrino detection instrumentation and analysis at the South Pole.

Astroparticle physicist searching for sources of ultrahigh-energy cosmic particles with IceCube and developing next-generation astroparticle/neutrino detector instrumentation.

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.

Works on quantum-limited sensing for astroparticle physics. Directions: (1) Pierre Auger Observatory — UHE cosmic ray composition and spectrum via radio and fluorescence detection; (2) liquid argon dark matter detectors; (3) co-PI DARPA QuSeN (2025) — quantum sensing of neutrinos using phonon-coupled SC qubit sensors with Cleland and Chou. KICP member.