论文标题

测试TES探测器与望远镜环境之间的磁干扰,以未来CMB卫星任务

Testing magnetic interference between TES detectors and the telescope environment for future CMB satellite missions

论文作者

Ghigna, Tommaso, Hoang, Thuong Duc, Hasebe, Takashi, Hoshino, Yurika, Katayama, Nobuhiko, Komatsu, Kunimoto, Lee, Adrian, Matsumura, Tomotake, Sakurai, Yuki, Sugiyama, Shinya, Suzuki, Aritoki, Raum, Christopher, Takaku, Ryota, Westbrook, Benjamin

论文摘要

即将到来的几个CMB实验的两个最常见的组件是大型超导TE(过渡边缘传感器)检测器和极化调节器单元,例如连续旋转的半波板(HWP)。高探测器计数对于提高仪器的原始灵敏度是必要的,但是过去的实验表明,系统效应已成为达到检测原始$ B $ modes所需的灵敏度的主要限制因素之一。因此,近年来极化调节器已变得流行,以减轻几种系统的影响。基于HWP技术的极化调节器需要旋转机制旋转板并调节传入的极化信号。为了最大程度地减少旋转机构的热量耗散,这是一个严格的要求,特别是对于像$ litebird $这样的太空任务,我们可以使用超导磁性轴承来悬浮转子并实现非接触式旋转。该技术的缺点是这些系统产生的相关磁场。在本文中,我们研究了对TES检测器原型的影响,并发现由于施加常数(DC)磁场而没有发现可检测到的$ T_C $变化,以及对变化(AC)磁场的非零TES响应。我们量化了对$ \ sim10^5 $ pa/g的应用的AC磁场的最坏情况的响应,并对拾取机构进行了初步解释。

The two most common components of several upcoming CMB experiments are large arrays of superconductive TES (Transition-Edge Sensor) detectors and polarization modulator units, e.g. continuously-rotating Half-Wave Plates (HWP). A high detector count is necessary to increase the instrument raw sensitivity, however past experiments have shown that systematic effects are becoming one of the main limiting factors to reach the sensitivity required to detect primordial $B$-modes. Therefore, polarization modulators have become popular in recent years to mitigate several systematic effects. Polarization modulators based on HWP technologies require a rotating mechanism to spin the plate and modulate the incoming polarized signal. In order to minimize heat dissipation from the rotating mechanism, which is a stringent requirement particularly for a space mission like $LiteBIRD$, we can employ a superconductive magnetic bearing to levitate the rotor and achieve contactless rotation. A disadvantage of this technique is the associated magnetic fields generated by those systems. In this paper we investigate the effects on a TES detector prototype and find no detectable $T_c$ variations due to an applied constant (DC) magnetic field, and a non-zero TES response to varying (AC) magnetic fields. We quantify a worst-case TES responsivity to the applied AC magnetic field of $\sim10^5$ pA/G, and give a preliminary interpretation of the pick-up mechanism.

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