Noise analysis and optical response of microwave kinetic inductance detectors with an optical stack

Paul Nicaise, Jie Hu, Christine Chaumont, Piercarlo Bonifacio, Michel Piat, Hervé Geoffray, Faouzi Boussaha
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Abstract

We report on the experimental investigation of optical coupling for superconducting microresonators known as microwave kinetic inductance detectors (MKIDs) in the visible and near-infrared bands. MKIDs are photon-counting, time and energy-resolving detectors that still suffer from a poor quantum efficiency. To improve this efficiency, we propose to add a superconducting reflective layer below the absorbing part of the detector separated by a transparent Al2O3 layer with a quarter-wavelength thickness optimized around a single wavelength λ = 405 nm. We have first fabricated samples patterned from stoichiometric TiN ( Tc4 K), one with the full optical stack, one without for reference and one with a partial optical stack in order to characterize the noise influence of each layer individually. We observe that the full optical stack geometry has the most impact on the resonator’s noise and quality factors. A second design was fabricated to characterize the optical response to short pulses of the optical stack and we show from both the frequential noise and optical response that a strong signature of TLS is still present in the optical stack sample. We have finally obtained single-photon response with the optical stack using a more sensitive tri-layer TiN/Ti/TiN absorber ( Tc1.3 K) for which a maximum energy resolving power of R=E/ΔE 1.3 was achieved using 405 nm laser pulses at 225 mK. The quality factors of both the reference and optical stack samples are similar but the frequency noise is still a tenfold higher for the optical stack sample which degrades the energy-resolving power of the detector.
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带光学叠层的微波动感探测器的噪声分析和光学响应
我们报告了对被称为微波动感探测器(MKID)的超导微谐振器在可见光和近红外波段的光耦合实验研究。MKID 是一种光子计数、时间和能量分辨探测器,但量子效率较低。为了提高这一效率,我们建议在探测器吸收部分的下方添加一个超导反射层,该层由透明的氧化铝层隔开,其厚度为四分之一波长,围绕单一波长 λ = 405 纳米进行了优化。我们首先制作了由化学钛(Tc∼4 K)图案化的样品,其中一个带有完整的光学叠层,一个不带光学叠层供参考,另一个带有部分光学叠层,以分别表征每一层对噪声的影响。我们观察到,全光学叠层几何形状对谐振器的噪声和品质因数影响最大。我们还制作了第二种设计,以表征光学叠层对短脉冲的光学响应。我们从频率噪声和光学响应中发现,光学叠层样品中仍然存在强烈的 TLS 特征。最后,我们利用灵敏度更高的三层 TiN/Ti/TiN 吸收体(Tc∼1.3 K)获得了光学叠层的单光子响应,在 225 mK 温度下使用 405 nm 激光脉冲可获得 R=E/ΔE∼1.3 的最大能量分辨力。参考样品和光学堆栈样品的质量因子相似,但光学堆栈样品的频率噪声仍然高出十倍,从而降低了探测器的能量分辨能力。
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