Dark Characterization of Ti/Al LEKIDs for the Search of Axions in the $W$-Band

We report the electrical (dark) characterization of lumped-element kinetic inductance detectors (LEKIDs) fabricated from a Titanium/Aluminum bilayer and designed for broadband absorption in the W–band (75-110 GHz). These detectors are prototypes for future Quantum Chromodynamics (QCD) axion search experiments within the Canfranc Axion Detection Experiment (CADEx), which demand sub-<inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$10^{-19}~\text{W}/\sqrt{\text{Hz}}$</tex-math></inline-formula> sensitivities under low optical backgrounds. We combine a Mattis-Bardeen analysis to the temperature dependence of the detector parameters with noise spectroscopy to determine the electrical noise equivalent power (NEP). The minimum measured value for the electrical NEP is <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\sim 3 \times 10^{-19}~\text{W}/\sqrt{\text{Hz}}$</tex-math></inline-formula>. Across the measured temperature range, we find that quasiparticle lifetime deviates from the expected BCS recombination law. Our analysis suggests that non-equilibrium relaxation is governed by spatial inhomogeneities in the superconducting gap and phonon diffusion effects. This work sets the road-map to achieve suitable and ultra-sensitive detectors in the W–band for dark matter axion search experiments.

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Journal
IEEE Transactions on Applied Superconductivity
Published
2026-02-23
DOI
https://doi.org/10.1109/tasc.2026.3664493
Primary Topic
Dark Matter and Cosmic Phenomena
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article
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article

Dark Characterization of Ti/Al LEKIDs for the Search of Axions in the $W$-Band

Víctor Rollano, María Teresa Magaz, David Rodríguez, Alicia Gómez et al.
IEEE Transactions on Applied Superconductivity
Dark Matter and Cosmic Phenomena
article

Dark Characterization of Ti/Al LEKIDs for the Search of Axions in the $W$-Band

Víctor Rollano, María Teresa Magaz, David Rodríguez, Alicia Gómez, Alessandro Monfardini, Daniel Granados, Martino Calvo
article en

Abstract

We report the electrical (dark) characterization of lumped-element kinetic inductance detectors (LEKIDs) fabricated from a Titanium/Aluminum bilayer and designed for broadband absorption in the W–band (75-110 GHz). These detectors are prototypes for future Quantum Chromodynamics (QCD) axion search experiments within the Canfranc Axion Detection Experiment (CADEx), which demand sub-<inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$10^{-19}~\text{W}/\sqrt{\text{Hz}}$</tex-math></inline-formula> sensitivities under low optical backgrounds. We combine a Mattis-Bardeen analysis to the temperature dependence of the detector parameters with noise spectroscopy to determine the electrical noise equivalent power (NEP). The minimum measured value for the electrical NEP is <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"><tex-math notation="LaTeX">$\sim 3 \times 10^{-19}~\text{W}/\sqrt{\text{Hz}}$</tex-math></inline-formula>. Across the measured temperature range, we find that quasiparticle lifetime deviates from the expected BCS recombination law. Our analysis suggests that non-equilibrium relaxation is governed by spatial inhomogeneities in the superconducting gap and phonon diffusion effects. This work sets the road-map to achieve suitable and ultra-sensitive detectors in the W–band for dark matter axion search experiments.

IEEE Transactions on Applied SuperconductivityVol. 36(6)
Madrid Institute for Advanced Studies (ES), Centre National de la Recherche Scientifique (FR), Centro de Astrobiología (ES), Université Grenoble Alpes (FR)
Openalex Percentile: Top 44%
Dark Matter and Cosmic Phenomena
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