LEKID-based instruments for cosmic microwave background polarimetry

Glenn Jones
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Abstract

After years of research and development, lumped-element kinetic inductance detectors (LEKIDs) are now competitive with other detector technologies for studying the polarization of the cosmic microwave background (CMB) radiation. One ultimate goal of this effort is the detection of the so-called inflationary B-mode polarization signature, which would yield the most convincing evidence for the theories of inflation and, if detected, would constrain the energy scale of these theories. The B-mode signal is predicted to be extremely small-in the nanokelvin range-requiring excellent sensitivity and exquisite control of systematics.
基于lekid的宇宙微波背景偏振仪
经过多年的研究和发展,集总元动力电感探测器(LEKIDs)在研究宇宙微波背景辐射的极化方面已具有与其他探测器技术相竞争的能力。这项工作的一个最终目标是探测到所谓的暴胀b模偏振特征,这将为暴胀理论提供最令人信服的证据,如果探测到,将限制这些理论的能量尺度。预计b模信号非常小,在纳米开尔文范围内,需要出色的灵敏度和精细的系统控制。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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