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POLOCALC: A Novel Method to Measure the Absolute Polarization Orientation of the Cosmic Microwave Background

机译:POLOCALC:一种测量宇宙微波背景绝对极化方向的新方法

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We describe a novel method to measure the absolute orientation of the polarization plane of the Cosmic Microwave Background (CMB) photons with arcsecond accuracy, enabling unprecedented measurements for cosmology and fundamental physics. Existing and planned CMB polarization instruments looking for primordial B-mode signals need an independent, experimental method for systematics control on the absolute polarization orientation. The lack of such a method limits the accuracy of the detection of inflationary gravitational waves, the constraining power on the neutrino sector through measurements of gravitational lensing of the CMB, the possibility of detecting Cosmic Birefringence (CB), and the ability to measure primordial magnetic fields. Sky signals used for calibration and direct measurements of the detector orientation cannot provide an accuracy better than 1°. Self-calibration methods provide better accuracy, but may be affected by foreground signals and rely heavily on model assumptions, losing constr...
机译:我们描述了一种新颖的方法,以弧秒精度测量宇宙微波背景(CMB)光子偏振面的绝对方向,从而为宇宙学和基础物理学提供了前所未有的测量方法。寻找原始B模式信号的现有和计划中的CMB极化仪器需要一种独立的实验方法来对绝对极化方向进行系统控制。缺乏这种方法限制了膨胀引力波检测的准确性,通过测量CMB的引力透镜对中微子扇区的约束能力,检测宇宙双折射(CB)的可能性以及测量原始磁场的能力领域。用于校准和直接测量探测器方位的天空信号不能提供优于1°的精度。自校准方法可提供更好的准确性,但可能会受到前景信号的影响,并且严重依赖于模型假设,因此会失去约束。

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