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'Big Bang' tomography as a new route to atomic-resolution electron tomography

机译:“大爆炸”层析成像是原子分辨率电子层析成像的新途径

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摘要

Until now it has not been possible to image at atomic resolution using classical electron tomographic methods, except when the target is a perfectly crystalline nano-object imaged along a few zone axes. The main reasons are that mechanical tilting in an electron microscope with sub-angstrom precision over a very large angular range is difficult, that many real-life objects such as dielectric layers in microelectronic devices impose geometrical constraints and that many radiation-sensitive objects such as proteins limit the total electron dose. Hence, there is a need for a new tomographic scheme that is able to deduce three-dimensional information from only one or a few projections. Here we present an electron tomographic method that can be used to determine, from only one viewing direction and with sub-angstrom precision, both the position of individual atoms in the plane of observation and their vertical position. The concept is based on the fact that an experimentally reconstructed exit wave consists of the superposition of the spherical waves that have been scattered by the individual atoms of the object. Furthermore, the phase of a Fourier component of a spherical wave increases with the distance of propagation at a known 'phase speed'. If we assume that an atom is a point-like object, the relationship between the phase and the phase speed of each Fourier component is linear, and the distance between the atom and the plane of observation can therefore be determined by linear fitting. This picture has similarities with Big Bang cosmology, in which the Universe expands from a point-like origin such that the distance of any galaxy from the origin is linearly proportional to the speed at which it moves away from the origin (Hubble expansion). The proof of concept of the method has been demonstrated experimentally for graphene with a two-layer structure and it will work optimally for similar layered materials, such as boron nitride and molybdenum disulphide.%最先进的电子显微镜能够轻而易举以亚原子分rn辨率解析结构,但要获得具有相似分辨率的三rn维图像却是一个更大的挑战。在这项研究中,rnDirk Van Dyck和Fu-Rong Chen描述了一个原rn始图像重建方法,它仅仅从一次投射便能在平rn面上以及在垂直方向上提取到关于所有原子去rn向的信息。该概念是基于这样的假设:每个原rn子作为一个“点源”(point source)来行动,散rn射出向探测器传播的球面波,在探测器上它们rn与来自其他原子的球面波相互干涉。所观测到rn的“出来的波”(exit wave)包含样品中所有原rn子的信息,可以用适当的算法进行调用。该方rn法对一个两层的石墨烯样品进行了实验演示。rn本文作者指出,他们的重建方法与宇宙学家用rn来构建“哈勃图”(Hubble plot)的方法相似,rn所以将其称之为“大爆炸断层扫描”(Big Bang rntomography)。
机译:到目前为止,除非目标是沿几个区域轴成像的完全结晶的纳米物体,否则无法使用经典的电子断层扫描方法以原子分辨率成像。主要原因是,很难在很大的角度范围内以亚埃级精度在电子显微镜中进行机械倾斜,许多现实生活中的物体(例如微电子设备中的介电层)受到几何约束,并且许多辐射敏感物体(例如蛋白质限制了总电子剂量。因此,需要一种新的断层摄影方案,该方案能够仅从一个或几个投影推导三维信息。在这里,我们介绍一种电子断层扫描方法,该方法可以仅从一个观察方向以亚埃的精度确定单个原子在观察平面中的位置及其垂直位置。该概念基于以下事实:实验重建的出射波由已被物体各个原子散射的球面波的叠加组成。此外,球形波的傅立叶分量的相位随着传播距离的增加而以已知的“相速度”增加。如果我们假设原子是点状对象,则每个傅立叶分量的相位和相速度之间的关系是线性的,因此原子与观察平面之间的距离可以通过线性拟合确定。这张图片与Big Bang宇宙学相似,在宇宙中宇宙从点状原点扩展,因此任何星系到原点的距离都与它离开原点的速度成线性比例(哈勃扩展)。该方法的概念证明已通过实验证明了具有两层结构的石墨烯,并且将最适合于类似层状的材料,例如氮化硼和二硫化钼。%最先进的电子显微镜能够轻而易举以亚原子分rn在此研究中,rn Dirk Van Dyck和Fu-Rong Chen描述了一个原先的图像重建方法,它该概念是基于这样的假设:每个原rn子作为一个“点源”(点源)来行动,散rn射出向探测器传播的球面波,在探测器上其rn与来自其他原子的球面波相互干扰。子方的信息,可以用适当的算法进行调用。该方rn法对一个两层的石墨烯样品进行了实验演示。 (哈勃图)的方法相似,rn所以将其称为“大爆炸断层扫描”。

著录项

  • 来源
    《Nature》 |2012年第7402期|p.243-246d3|共5页
  • 作者

    Dirk Van Dyck; Fu-Rong Chen;

  • 作者单位

    University of Antwerp, Groenenborgerlaan 171, B2020 Antwerp, Belgium;

    National Tsing Hua University, Number 101, Section 2, Kuang-Fu Road, Hsin Chu, Taiwan 300, China;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);美国《化学文摘》(CA);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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