1. Characterizing TES power noise for future single optical-phonon and infrared-photon detectors
- Author
-
W. A. Page, R. Mahapatra, R. Partridge, B. Serfass, B. A. Hines, P. L. Brink, S. Zuber, C. W. Fink, Bernard Sadoulet, S. Ganjam, Noah Kurinsky, Martin E. Huber, Tsuguo Aramaki, Matt Pyle, S. L. Watkins, N. Mirabolfathi, and M. Platt
- Subjects
Physics - Instrumentation and Detectors ,Infrared ,Phonon ,Dark matter ,FOS: Physical sciences ,General Physics and Astronomy ,Dirac delta function ,02 engineering and technology ,01 natural sciences ,symbols.namesake ,Power noise ,0103 physical sciences ,Noise-equivalent power ,010302 applied physics ,Physics ,business.industry ,Bandwidth (signal processing) ,Detector ,Instrumentation and Detectors (physics.ins-det) ,021001 nanoscience & nanotechnology ,lcsh:QC1-999 ,symbols ,Optoelectronics ,0210 nano-technology ,business ,lcsh:Physics - Abstract
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., Comment: 5 pages, 6 figures. Accepted for publication at AIP Advances
- Published
- 2020