Heterodyne Broadband Detection of Axion Dark Matter
arXiv:2007.15656 · doi:10.1103/PhysRevD.104.L111701
Abstract
We propose a new broadband search strategy for ultralight axion dark matter that interacts with electromagnetism. An oscillating axion field induces transitions between two quasi-degenerate resonant modes of a superconducting cavity. In two broadband runs optimized for high and low masses, this setup can probe unexplored parameter space for axion-like particles covering fifteen orders of magnitude in mass, including astrophysically long-ranged fuzzy dark matter.
10+14 pages, 3 figures
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Cited by in corpus (19)
- Detecting High-Frequency Gravitational Waves with Microwave Cavities
- The Cosmic Axion Background
- Hunt for Light Primordial Black Hole Dark Matter with Ultra-High-Frequency Gravitational Waves
- The Interplay between the Dark Matter Axion and Primordial Black Holes
- Friendship in the Axiverse: Late-time direct and astrophysical signatures of early-time nonlinear axion dynamics
- Axion minivoids and implications for direct detection
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- Searching for Low-Mass Axions using Resonant Upconversion
- Nonperturbative structure in coupled axion sectors and implications for direct detection
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- Early dark energy by dark Higgs, and axion-induced non-thermal trapping
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- Sensitivity of Resonant Axion Haloscopes to Quantum Electromagnetodynamics
- Axion Haloscope Array With Symmetry
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- Constraints on Axions from Cosmic Distance Measurements
- ALP Dark Matter from Kinetic Fragmentation: Opening up the Parameter Window
- Axion Searches with Two Superconducting Radio-frequency Cavities
- Storage Rings and Gravitational Waves: Summary and Outlook