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首页> 外文期刊>Vacuum: Technology Applications & Ion Physics: The International Journal & Abstracting Service for Vacuum Science & Technology >Reactive DC magnetron sputter deposited Ti-Cu-N nano-composite thin films at nitrogen ambient
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Reactive DC magnetron sputter deposited Ti-Cu-N nano-composite thin films at nitrogen ambient

机译:氮气环境下反应性直流磁控溅射沉积Ti-Cu-N纳米复合薄膜

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摘要

Ti-Cu-N thin films have been grown on Si(111), KBr (potassium bromide), quartz and glass slide substrates using a TiCu (13:87 at. %) single multi-component target by reactive DC magnetron sputtering at nitrogen ambient. This study provides insight into the importance of nitrogen pressure on the characteristic of Ti-Cu-N thin films. Crystalline phases of these films are identified by X-ray diffraction (XRD) technique. The titanium atoms were inserted into the Cu_3N unit cell. The results from XRD show that the observed phases are nano-crystallite cubic anti-Rhenium oxide (anti-ReO _3) structure of Ti doped Cu_3N (Ti:Cu_3N) and nano-crystallite face centre cubic (fcc) structure of Cu. Formation of copper vacancies in Cu_3N cell substituted by titanium atoms and subsequent excess of interstitial nitrogen (N-rich) result in lattice constant expansion and optical energy gap widening. Surface morphology of the films studied by scanning electron microscope (SEM) indicates agglomeration of grains. Ti:Cu atomic ratio of Ti-Cu-N films, determined by energy dispersive X-ray (EDX) spectroscopy, is less than that of the original TiCu single multi-component target and nearly independent of nitrogen pressure. Optical study is performed by Vis-near IR transmittance spectroscopy. Film thickness, refractive index and extinction coefficient are extracted from the measured transmittance using a reverse engineering method. Absorption coefficient indicates that the nitrided films are direct semiconductor. The films electrically show quasi-metallic behavior. The effect of sputtering pressure on deposition rate is investigated. Compared with the Ti free Cu_3N film, the Ti:Cu_3N films possesses fine thermal stability in vacuum.
机译:Ti-Cu-N薄膜已通过在氮气下进行反应性直流磁控溅射,使用TiCu(13:87 at。%)单一多组分靶材在Si(111),KBr(溴化钾),石英和玻璃载玻片上生长。周围。这项研究提供了对氮气压力对Ti-Cu-N薄膜特性的重要性的认识。这些膜的结晶相通过X射线衍射(XRD)技术鉴定。将钛原子插入到Cu_3N晶胞中。 XRD的结果表明,所观察到的相为掺Ti的Cu_3N(Ti:Cu_3N)的纳米微晶立方抗氧化((Anti:ReO _3)结构和Cu的纳米微晶面心立方(fcc)结构。 Cu_3N单元中被钛原子取代的铜空位的形成以及随后过量的间隙氮(富N)导致晶格常数扩展和光能隙变宽。通过扫描电子显微镜(SEM)研究的膜的表面形态表明晶粒的团聚。通过能量色散X射线(EDX)光谱法测定的Ti-Cu-N薄膜的Ti:Cu原子比小于原始TiCu单一多组分靶的原子比,并且几乎与氮气压力无关。光学研究是通过可见近红外透射光谱进行的。使用逆向工程方法从测得的透射率中提取膜厚度,折射率和消光系数。吸收系数表明氮化膜是直接半导体。这些膜在电气上显示出准金属行为。研究了溅射压力对沉积速率的影响。与不含Ti的Cu_3N薄膜相比,Ti:Cu_3N薄膜在真空中具有良好的热稳定性。

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