Investigations of optical aberration on quantum diamond microscopy toward high spatial resolution and sensitivity.

IF 1.3 4区 工程技术 Q3 INSTRUMENTS & INSTRUMENTATION
Shunsuke Nishimura, Moeta Tsukamoto, Kento Sasaki, Kensuke Kobayashi
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Abstract

Quantum diamond microscopy (QDM), which employs nitrogen-vacancy (NV) center ensembles, is a promising approach to quantitatively imaging magnetic fields with both high resolution that approaches the diffraction limit and a wide field of view. The commonly adopted setups of QDM capture the photoluminescence through transparent diamonds, which inevitably entail aberrations-optical errors that degrade the optical resolution and contrast of the obtainable image. In this study, we delve into the impact of optical aberrations, focusing on their dependence on diamond thickness. We first introduce a rigorous model [B. Richards et al., Proc. R. Soc. London, Ser. A 253, 358-379 (1959) and J. Braat et al., J. Opt. Soc. Am. A 20, 2281-2292 (2003)] of diffraction that incorporates aberrations, producing the NV center optical image. We confirm that this model accurately reproduces the confocal images of single NV centers obtained at various depths in diamonds. Extending this model to a wide-field microscope, we find that the model also accurately reproduces the USAF 1951 resolution test chart obtained through diamonds of various thicknesses. Based on these investigations, we quantitatively assess the consequent resolution constraints and propose thinning the diamond as a viable solution. We present a robust method to quantitatively ascertain resolution in optical systems influenced by aberrations caused by ray transmission through diamonds. For instance, for a typical microscope with an objective lens of NA = 0.7, the diffraction limit is achievable through diamonds that are 30 μm thick, and a resolution of 1 μm is obtained through diamonds that are 100 μm thick. Those results open up avenues for enhanced performance in QDM.

面向高空间分辨率和高灵敏度的量子金刚石显微镜光学像差研究。
量子金刚石显微镜(QDM)采用氮空位(NV)中心系集,是一种有前途的磁场定量成像方法,具有接近衍射极限的高分辨率和宽视场。通常采用的QDM设置通过透明钻石捕获光致发光,这不可避免地会产生像差-光学误差,从而降低可获得图像的光学分辨率和对比度。在这项研究中,我们深入研究了光学像差的影响,重点是它们对金刚石厚度的依赖。我们首先引入一个严格的模型[B]。Richards et al., Proc. R. Soc。伦敦,爵士。A 253, 358-379(1959)和J. Braat等。点。[20,2281 -2292(2003)]包含像差的衍射,产生NV中心光学图像。我们证实,该模型准确地再现了在钻石中不同深度获得的单个NV中心的共聚焦图像。将该模型扩展到宽视场显微镜下,我们发现该模型也准确地再现了通过不同厚度的金刚石获得的USAF 1951分辨率测试图。基于这些研究,我们定量地评估了随之而来的分辨率限制,并提出将金刚石变薄作为一种可行的解决方案。我们提出了一种可靠的方法来定量确定光学系统的分辨率,这些光学系统受射线通过钻石传输引起的像差的影响。例如,对于典型的物镜NA = 0.7的显微镜,通过30 μm厚的金刚石可以达到衍射极限,通过100 μm厚的金刚石可以获得1 μm的分辨率。这些结果为提高QDM的性能开辟了道路。
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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来源期刊
Review of Scientific Instruments
Review of Scientific Instruments 工程技术-物理:应用
CiteScore
3.00
自引率
12.50%
发文量
758
审稿时长
2.6 months
期刊介绍: Review of Scientific Instruments, is committed to the publication of advances in scientific instruments, apparatuses, and techniques. RSI seeks to meet the needs of engineers and scientists in physics, chemistry, and the life sciences.
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