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Physics > Instrumentation and Detectors

arXiv:2207.05534 (physics)
[Submitted on 12 Jul 2022 (v1), last revised 13 Feb 2023 (this version, v2)]

Title:Resolving Power of Visible to Near-Infrared Hybrid $β$-Ta/NbTiN Kinetic Inductance Detectors

Authors:Kevin Kouwenhoven, Daniel Fan, Enrico Biancalani, Steven A.H. de Rooij, Tawab Karim, Carlas S. Smith, Vignesh Murugesan, David J. Thoen, Jochem J.A. Baselmans, Pieter J. de Visser
View a PDF of the paper titled Resolving Power of Visible to Near-Infrared Hybrid $\beta$-Ta/NbTiN Kinetic Inductance Detectors, by Kevin Kouwenhoven and 9 other authors
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Abstract:Kinetic Inductance Detectors (KIDs) are superconducting energy-resolving detectors, sensitive to single photons from the near-infrared to ultraviolet. We study a hybrid KID design consisting of a beta phase tantalum ($\beta$-Ta) inductor and a NbTiN interdigitated capacitor (IDC). The devices show an average intrinsic quality factor $Q_i$ of 4.3$\times10^5$ $\pm$ 1.3 $\times10^5$. To increase the power captured by the light sensitive inductor, we 3D-print an array of 150$\times$150 $\mu$m resin micro lenses on the backside of the sapphire substrate. The shape deviation between design and printed lenses is smaller than 1$\mu$m, and the alignment accuracy of this process is $\delta_x = +5.8 \pm 0.5$ $\mu$m and $\delta_y = +8.3 \pm 3.3$ $\mu$m. We measure a resolving power for 1545-402 nm that is limited to 4.9 by saturation in the KID's phase response. We can model the saturation in the phase response with the evolution of the number of quasiparticles generated by a photon event. An alternative coordinate system that has a linear response raises the resolving power to 5.9 at 402 nm. We verify the measured resolving power with a two-line measurement using a laser source and a monochromator. We discuss several improvements that can be made to the devices on a route towards KID arrays with high resolving powers.
Comments: 13 pages, 11 Figures, Journal Paper
Subjects: Instrumentation and Detectors (physics.ins-det); Instrumentation and Methods for Astrophysics (astro-ph.IM); Superconductivity (cond-mat.supr-con)
Cite as: arXiv:2207.05534 [physics.ins-det]
  (or arXiv:2207.05534v2 [physics.ins-det] for this version)
  https://doi.org/10.48550/arXiv.2207.05534
arXiv-issued DOI via DataCite
Journal reference: Phys. Rev. Appl. 19 (2023) 034007
Related DOI: https://doi.org/10.1103/PhysRevApplied.19.034007
DOI(s) linking to related resources

Submission history

From: Kevin Kouwenhoven [view email]
[v1] Tue, 12 Jul 2022 13:52:02 UTC (30,969 KB)
[v2] Mon, 13 Feb 2023 15:50:43 UTC (31,357 KB)
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