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Angstrom-scale distance dependence of antenna-enhanced vibrational signals

机译:天线增强的振动信号的埃尺度距离依赖性

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摘要

The resonantly enhanced near-field of micrometer-sized gold antennas has been probed with Angstrom-scale resolution. In situ surface-enhanced infrared spectroscopic vibrational signals of carbon monoxide (CO) layers cold-condensed on the antennas in ultrahigh-vacuum conditions are compared to the signals of CO layers with corresponding thicknesses on a flat gold surface. Vibrational signals of CO as well as the shift of the plasmonic resonance frequency were used to analyze the distance dependence of the near-field. The signal enhancement induced by the antennas not only decays monotonically from the surface but, in contrast to classical near-field models, shows a maximum between 10 and 15 ? and decays also toward the surface of the antenna. This effect is attributed to the spill-out of the electron wave function, as expected from quantum mechanical calculations.
机译:微米级金天线的共振增强近场已经用埃尺度分辨率进行了探测。将在超高真空条件下冷冷凝在天线上的一氧化碳(CO)层的原位表面增强红外光谱振动信号与平坦金表面上具有相应厚度的CO层的信号进行比较。使用CO的振动信号以及等离子体共振频率的偏移来分析近场的距离依赖性。天线引起的信号增强不仅从表面单调衰减,而且与经典的近场模型相比,最大值在10至15?之间。并朝天线表面衰减。如量子力学计算所预期的,该效应归因于电子波函数的溢出。

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