Assembly and alignment of thin mirrors using ultrafast laser generated strain toward future x-ray telescope optics

Brody D. McElwain, Tyler Wilson, I. J. Arnold, Brandon D. Chalifoux
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Abstract

High-resolution and large-effective-area x-ray telescopes are critical tools for observing the high-energy universe, but the existing quasi-kinematic and over-constrained mounts for aligning mirrors trade off accuracy and strength. We propose a method to fabricate spacers and bond them between thin mirrors, then adjust mirror alignment by focusing ultrafast laser pulses into these spacers. We built a simple mirror stack assembly composed of two flat mirrors bonded to two spacers and wrote laser-induced modifications into these spacers. We interferometrically measured the air gap between the two mirrors after each set of laser-induced modifications. The resulting deformation in the spacers and measured tilt between flat mirrors shows that realignment can be controlled using the ultrafast laser, however there is uncertainty introduced by imperfect mirror stack assemblies. Future work will aim to achieve predictable laser-induced strain. The presented assembly procedure and laser-strain generation process serves as a potential solution to the optomechanically-limited design of current-generation x-ray telescopes.
利用超快激光产生的应变组装和对准薄反射镜,面向未来的x射线望远镜光学
高分辨率和大有效面积的x射线望远镜是观测高能宇宙的关键工具,但现有的准运动学和过度约束的对准镜支架在精度和强度方面存在折衷。我们提出了一种制造间隔片的方法,并将它们粘合在薄反射镜之间,然后通过将超快激光脉冲聚焦到这些间隔片上来调节反射镜的对准。我们建立了一个简单的反射镜堆栈组件,由两个平面反射镜连接到两个间隔片,并在这些间隔片中写入激光诱导修改。在每组激光诱导修饰后,我们用干涉测量法测量了两个反射镜之间的气隙。由此产生的间隔片变形和测量到的平面镜之间的倾斜表明,使用超快激光可以控制重新对准,但是由于镜面堆叠组件不完美而引入了不确定性。未来的工作将致力于实现可预测的激光诱导应变。所提出的装配程序和激光应变生成工艺为解决当前一代x射线望远镜光力学受限的设计提供了一种潜在的解决方案。
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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