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RF magnetron sputtering of LaS thin films on InP substrates

机译:在INP基板上的LAS薄膜的RF磁控溅射

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Recently, we have proposed that rare-earth sulfides on various III-V semiconductor surfaces [1, 2] are attractive materials to reach Negative Electron Affinity (NEA) [3] at various III-V semiconductor surfaces [1, 2]. These compounds are chemically more stable than the cesiated surfaces [4] used hitherto in such applications. Of particular interest is the fact that the work function (WF) of rare-earth sulfides at room temperature, when extrapolated from high-temperature measurements, is quite mall (between 1 and 1.5 eV). It is therefore expected that these materials can be used to reach NEA when deposited on p-type doped semiconductors. For instance, LaS has a lattice constant (5.854 A) very close to the lattice constant of InP (5.8688 A). Since the room temperature WF of LaS (1.14 eV) is below the band gap of InP (1.35 eV), NEA can therefore be realized at InP/LaS interface using heavily p-type doped semiconductor substrate [1, 2]. Two other important features of the fcc cubic form of LaS are its fairly large melting temperature (about 2200 °C) and its metallic character (its electrical resistivity has been measured as low as 25 μΩ cm [5]).
机译:最近,我们提出了各种III-V半导体表面[1,2]的稀土硫化物是在各种III-V半导体表面的负电子亲和力(NEA)[3]的吸引物质[1,2]。这些化合物比在这种应用中使用的迄今为止使用的伴随表面更稳定。特别令人兴趣的是,当从高温测量外推开时,室温下的稀土硫化物的功函数(WF)是非常商场(在1到1.5 eV之间)。因此,预期这些材料可用于在沉积在p型掺杂半导体上时达到NEA。例如,LAS具有晶格常数(5.854A),非常接近INP的晶格常数(5.8688A)。由于LAS(1.14eV)的室温下方,低于INP(1.35eV)的带隙,因此可以在INP / LAS界面中使用大型p型掺杂半导体衬底[1,2]来实现NEA。 FCC立方形式的LAS的其他两个重要特征是其相当大的熔化温度(约2200℃),其金属特性(其电阻率已经低至25μΩcm[5])。

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