未来单光声子和红外光子探测器的TES功率噪声表征

C. Fink, S. Watkins, T. Aramaki, P. Brink, S. Ganjam, B. Hines, M. Huber, N. Kurinsky, N. Kurinsky, R. Mahapatra, N. Mirabolfathi, W. Page, R. Partridge, M. Platt, M. Pyle, B. Sadoulet, B. Serfass, S. Zuber
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引用次数: 18

摘要

在本文中,我们介绍了临界温度为40 mK的$100~\mu\mathrm{m}\times 400~\mu\mathrm{m} \times 40~\mathrm{nm}$钨(W)过渡边缘传感器(TES)的性能。该器件的测量噪声等效功率(NEP)为$1.5\times 10^{-18}\ \mathrm{W}/\sqrt{\mathrm{Hz}}$,带宽为$2.6$ kHz,表明狄拉克δ能量沉积的分辨率为$40\pm 5~\mathrm{meV}$ (rms)。该装置所展示的性能是开发用于低质量暗物质搜索的$\mathcal{O}(100)~\mathrm{meV}$阈值非热声子探测器的关键一步。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Characterizing TES power noise for future single optical-phonon and infrared-photon detectors
In this letter, we present the performance of a $100~\mu\mathrm{m}\times 400~\mu\mathrm{m} \times 40~\mathrm{nm}$ tungsten (W) Transition-Edge Sensor (TES) with a critical temperature of 40 mK. This device has a measured noise equivalent power (NEP) of $1.5\times 10^{-18}\ \mathrm{W}/\sqrt{\mathrm{Hz}}$, in a bandwidth of $2.6$ kHz, indicating a resolution for Dirac delta energy depositions of $40\pm 5~\mathrm{meV}$ (rms). The performance demonstrated by this device is a critical step towards developing a $\mathcal{O}(100)~\mathrm{meV}$ threshold athermal phonon detectors for low-mass dark matter searches.
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