Near-Quantum-Noise Axion Dark Matter Search at CAPP around 9.5 eV
arXiv:2207.13597 · doi:10.1103/PhysRevLett.130.091602
Abstract
We report the results of an axion dark matter search over an axion mass range of 9.39-9.51 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.
arXiv comment6 pages, 4 figures
References in corpus (21)
- Planck 2015 results. XIII. Cosmological parameters
- New CAST Limit on the Axion-Photon Interaction
- A SQUID-based microwave cavity search for dark-matter axions
- A Search for Invisible Axion Dark Matter with the Axion Dark Matter Experiment
- Extended Search for the Invisible Axion with the Axion Dark Matter Experiment
- A quantum-enhanced search for dark matter axions
- First results from a microwave cavity axion search at 24 micro-eV
- Results from phase 1 of the HAYSTAC microwave cavity axion experiment
- Search for "Invisible" Axion Dark Matter in the eV Mass Range
- An Improved RF Cavity Search for Halo Axions
- Axion Dark Matter Search around 6.7 eV
- Results from a High-Sensitivity Search for Cosmic Axions
- First Results from Axion Haloscope at CAPP around 10.7 eV
- Piezoelectrically Tuned Multimode Cavity Search for Axion Dark Matter
- Search for invisible axion dark matter with a multiple-cell haloscope
- The HAYSTAC Axion Search Analysis Procedure
- Squeezing with a flux-driven Josephson parametric amplifier
- Experimental Constraints on the Axion Dark Matter Halo Density
- Axion-photon Couplings in Invisible Axion Models
- New solar axion search in CAST with He filling
- Flux-driven Josephson parametric amplifiers: Hysteretic flux response and nondegenerate gain measurements
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- Parameter optimization of Josephson parametric amplifiers using a heuristic search algorithm for axion haloscope search
- Axions at the meV Crossroads: Theory, Cosmology, Astrophysics, and Experiments
- Cavity, lumped-circuit, and spin-based detection of axion dark matter: differences and similarities
- Resonant enhancement of axion dark matter decay
- Extended Haloscope Search and Exclusion of a Candidate Signal near 1.036 GHz
- Physics beyond the Standard Model with the DSA-2000