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Surface electronic structure of α-Mo_2C(0001)

机译:α-Mo_2C(0001)的表面电子结构

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The electronic structure of α-Mo_2C(0001) has been investigated by angle-resolved photoemission spectroscopy utilizing synchrotron radiation. A sharp peak is observed at 3.3 eV in normal-emission spectra. Since the peak shows no dispersion as a function of photon energy and is sensitively attenuated by oxygen adsorption, the initial state of the peak is attributed to a surface state. Resonant photo-emission study shows that the state includes substantial contribution of 4d orbitals of the Mo atoms in the second layer. The emissions with constant kinetic energies of 22 and 31 eV above the Fermi level (E_F) are found in normal-emission spectra, and these emissions are interpreted as originating from the Mo N_1N_(23)V and N_(23)W Auger transitions, respectively.
机译:α-Mo_2C(0001)的电子结构已通过利用同步加速器辐射的角度分辨光发射光谱进行了研究。在正常发射光谱中,在3.3 eV处观察到一个尖峰。由于该峰没有显示出作为光子能量的函数的色散,并且被氧吸附灵敏地衰减,因此该峰的初始状态归因于表面状态。共振光发射研究表明,该态包括第二层中Mo原子的4d轨道的大量贡献。在正常发射光谱中发现具有高于费米能级(E_F)的22和31 eV恒定动能的发射,这些发射被解释为源自Mo N_1N_(23)V和N_(23)W Auger跃迁,分别。

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