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Identification of surface adsorbates by scanning tunneling microscope light emission spectra

机译:通过扫描隧穿显微镜光发射光谱识别表面吸附物

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In order to demonstrate that surface adsorbates can be identified by STM light emission spectra, we have measured the STM light emission spectra of various combinations of adsorbates and substrates. We presented the spectra of Cu(110)-0 and Ni(110)-H. The adsorbate specific spectra have been found for both systems. When the tip is located over the O atom adsorbed on the Cu(110) surface, the three additional components due to the electronic transitions localized at the O site is superposed on the STM light emission spectra. Thus we can identify the O atom from the spectra. In the case of Ni(110)-H system, the vibrational energy of the H atom is determined from the spectra. Consequently, we can identify the H atom from the spectra. As mentioned in the introduction, surface vibrational energies are specific to each adsorbate. Hence classical surface vibrational spectroscopic methods such as EELS and infrared absorption spectroscopy are conveniently used for identification of surface adsorbates under macroscopic spatial resolution. The result for Ni(110)-H demonstrates that the vibrational energies of surface adsorbates can be determined by measuring the STM light emission spectra with the benefit of atomic spatial resolution. In this manner the STM light emission spectroscopy is a very unique and valuable tool for identification of surface adsorbates with atomic spatial resolution.
机译:为了证明表面吸附物可以通过STM发光光谱识别,我们测量了吸附物和基板的各种组合的STM发射光谱。我们介绍了Cu(110)-0和Ni(110)-H的光谱。已经找到了对两个系统的吸附物特异性光谱。当尖端位于吸附在Cu(110)表面上的O原子上时,由于O位点的电子转换引起的三个附加部件叠加在STM光发射光谱上。因此,我们可以从光谱识别O原子。在Ni(110)-H系统的情况下,从光谱确定H原子的振动能量。因此,我们可以从光谱识别H原子。如引言所提到的,表面振动能对于每种吸附物特异。因此,典型的表面振动光谱方法如鳗鱼和红外吸收光谱,方便地用于鉴定宏观空间分辨率下的表面吸附物。 Ni(110)-h的结果表明,通过用原子空间分辨率的益处测量STM发光光谱,可以确定表面吸附物的振动能量。以这种方式,STM发光光谱是一种非常独特而有价值的工具,用于识别具有原子空间分辨率的表面吸附物。

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