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Arjan Ferdinand van Loo

Publications and source records attributed to Arjan Ferdinand van Loo.

3 recordsLinked to original sources

Search for Axion Dark Matter around \texorpdfstring{$15.6\,μ\text{eV}$}{15.6 microeV} with a Broadly Tunable High-Temperature Superconducting Cavity

We report an axion dark matter search in the mass range of $15.30\text{--}15.85\,μ\text{eV}$ using a broadly tunable high-temperature superconducting (HTS) haloscope. By soldering substrate-stripped rare-earth barium copper oxide (REBCO) films onto a copper shell, we achieved a quality factor 3--4 times higher than in copper cavities across its tuning band in an 8\text{-T} magnetic field. We set robust Frequentist 90\%~confidence-level exclusion limits on the axion--photon coupling down to 1.3 times the KSVZ coupling, while a complementary Bayesian analysis achieves KSVZ-level sensitivity.

hep-ex↗

Broadband Kinetic-Inductance Parametric Amplifiers with Impedance Engineering

Broadband quantum-limited parametric amplifiers (PAs) are essential components in quantum information science and technology. Impedance-engineered resonator-based PAs and traveling-wave PAs are the primary approaches to overcome the gain-bandwidth constraint. While the former PAs are simpler to fabricate, the target characteristic impedance Z_\text{NR} of the nonlinear resonator has been restricted to be below 10 Ω, requiring large capacitance. Moreover, these PAs have only been implemented with aluminum-based Josephson junctions (JJs), hindering their operation at high temperatures or strong magnetic fields. To address these issues, we propose a three-stage impedance-transformer scheme, showcased with a 20-nm-thick, 250-nm-wide high-kinetic-inductance niobium-titanium-nitride (NbTiN) film. Our scheme enables Z_\text{NR} up to several tens of ohms--a tenfold improvement over conventional designs, achieved through an additional quarter-wavelength transmission line with the characteristic impedance of 180 Ω. Our kinetic-inductance impedance-engineered parametric amplifiers (KIMPA), featuring a 330-fF shunt capacitor, demonstrate a phase-preserving amplification with a 450-MHz bandwidth at 17-dB gain, and an added noise ranging from 0.5-1.3 quanta near the center frequency of 8.4 GHz. Due to the high critical current of the NbTiN nanowire, the KIMPA also achieves a saturation power of up to -68\pm3 dBm, approximately 30-dB higher than that of JJ-based PAs. This scheme also opens new possibilities for other three-wave-mixing building blocks.

quant-ph↗

Near-Quantum-Noise Axion Dark Matter Search at CAPP around 9.5 $μ$eV

We report the results of an axion dark matter search over an axion mass range of 9.39-9.51 $μ$eV. A flux-driven Josephson parametric amplifier (JPA) was added to the cryogenic receiver chain. A system noise temperature of as low as 200 mK was achieved, which is the lowest recorded noise among published axion cavity experiments with phase-insensitive JPA operation. In addition, we developed a two-stage scanning method which boosted the scan speed by 26%. As a result, a range of two-photon coupling in a plausible model for the QCD axion was excluded with an order of magnitude higher in sensitivity than existing limits.

hep-ex↗