首页> 外文期刊>Journal of Alloys and Compounds: An Interdisciplinary Journal of Materials Science and Solid-state Chemistry and Physics >An interplay among the Mg2+ ion coordination, structural order, oxygen vacancies and magnetism of MgO thin films
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An interplay among the Mg2+ ion coordination, structural order, oxygen vacancies and magnetism of MgO thin films

机译:MgO薄膜的Mg2 +离子协调,结构阶,氧空位和磁性之间的相互作用

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The magnetic properties of MgO thin films were discussed as an interplay among the oxygen vacancies, Mg2+ ion coordination and structural order deposited using radio frequency (RF) sputtering method by varying substrate temperature and deposition power followed by in-situ annealing. Rutherford back-scattering spectrometry (RBS) and high resolution transmission electron microscopic (HRTEM) performed for these films showed decrease of film thickness with increase of substrate temperature. Films are thicker for higher sputtering powers at corresponding substrate temperatures. Spectral features in Mg K-edge near edge X-ray absorption fine structure (NEXAFS) spectra are characteristics of MgO for both sputtering powers at substrate temperature of room temperature (RT) and 350 degrees C. O K-edge NEXAFS spectra exhibited onset of oxygen vacancies as inferred from pre-edge region. Magnetization versus applied magnetic field curves for these films showed onset of d(0) ferromagnetism. This behavior ceased with increase of substrate temperature, however, become dominant with increase of sputtering power. Magnetic behavior was dominant for the films which had slightly distorted Mg2+ ion co-ordination. The existence of oxygen vacancies was not observed to be consistent with magnetization. Thus, this study envisaged the role of Mg2+ ion coordination, long range structural order and oxygen vacancies in order to determine magnetism in these systems. (C) 2019 Elsevier B.V. All rights reserved.
机译:通过改变基板温度和沉积功率,在原位退火之后,讨论了MgO薄膜的氧空位,Mg2 +离子配位和结构阶的相互作用作为使用射射频率(RF)溅射方法的相互作用。对这些薄膜进行的Rutherford背散射光谱(RBS)和高分辨率透射电子显微镜(HRTEM)显示膜厚度随衬底温度的增加而降低。在相应的基板温度下,薄膜对更高的溅射功率较厚。边缘X射线吸收细结构(NEXAFS)光谱附近的Mg k侧的光谱特征是用于室温(RT)的底物温度的溅射功率的MgO的特性(RT)和350℃。O K-Edge NexaFS光谱表现出爆发从预先边缘区域推断出氧气空位。对于这些薄膜的磁化与施加的磁场曲线显示出D(0)铁磁性的发作。然而,随着溅射动力的增加,这种行为随着衬底温度的增加而变得显着。对于略微扭曲Mg2 +离子协调的薄膜,磁性行为占主导地位。未观察到氧空位的存在与磁化相一致。因此,本研究设想了MG2 +离子协调,长距离结构顺序和氧空位的作用,以便确定这些系统中的磁性。 (c)2019 Elsevier B.v.保留所有权利。

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