Co/Alq3 双电层磁性随结构和形态的变化:厚度依赖性研究

IF 1.6 4区 物理与天体物理 Q3 PHYSICS, APPLIED Journal of Superconductivity and Novel Magnetism Pub Date : 2024-08-09 DOI:10.1007/s10948-024-06812-8
Manisha Priyadarsini, Sonia Kaushik, Arun Singh Dev, Sharanjeet Singh, Pooja Gupta, Matthias Schwartzkopf, Stephan V. Roth, V. Raghavendra Reddy, Dileep Kumar
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引用次数: 0

摘要

有机自旋电子学(OS)侧重于利用有机材料中的自旋自由度,因其技术层面和未来应用而一直是一个引人入胜的话题。在快速发展的有机自旋电子学领域,面内单轴磁各向异性(UMA)正变得越来越重要。本研究在三(8-羟基喹啉)铝(Alq3)层上沉积了不同厚度的钴(Co)薄膜,以研究磁性和 UMA 的演变。通过改变易磁化轴与外加磁场之间的方位角,利用磁光克尔效应进行了磁性测量和同步畴成像。结果发现,在形成厚度约为 10 纳米的连续 Co 薄膜后,双层膜在薄膜平面上呈现出定义明确的 UMA。在德国同步辐射光源 PETRA-III P03 光束线使用掠入射小角 X 射线散射和广角 X 射线散射测量法研究了所有 Co/Alq3 双层膜的结构和形态特性。综合分析表明,与无机磁性多晶薄膜的 UMA 主要源于应力不同,Co/Alq3 的 UMA 源于 c 轴(Co (002))优先取向引起的磁晶各向异性。Alq3 的表面自由能小于 Co 的表面自由能;因此,Co 的生长从岛的形成开始,并随着厚度的增加而凝聚。观察到的结构取向可归因于将凝聚产生的磁弹性能量最小化,这就是所谓的 "拉链效应"。厚度较低的薄膜(约 5 nm)中没有 UMA,这可以理解为扩散界面导致的各向同性引脚引起的随机短程应力。
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Evolution of Magnetic Properties with Structure and Morphology of Co/Alq3 Bilayer: A Thickness Dependent Study

Organic spintronics (OS), which focuses on utilizing the spin degree of freedom in organic materials, has been a fascinating topic because of its technological aspects and future applications. In-plane uniaxial magnetic anisotropy (UMA) is becoming increasingly important in the rapidly developing field of OS. In this study, Cobalt (Co) films were deposited with varying thicknesses on the Tris (8-hydroxyquinolinato) aluminium (Alq3) layer to investigate the evolution of magnetism and UMA. Magnetic measurements and simultaneous domain imaging have been done using the magneto-optic Kerr effect by varying the azimuthal angle between the easy axis of magnetization and the applied magnetic field. It was discovered that the bilayer exhibits a well-defined UMA in the film plane upon forming a continuous Co film with a thickness of around 10 nm. Structural and morphological properties of all the Co/Alq3 bilayers were studied using grazing-incidence small-angle X-ray scattering and wide-angle X-ray scattering measurements at synchrotron radiation source, P03 beamline PETRA-III, Germany. The combined analysis revealed that in contrast to the inorganic magnetic polycrystalline thin films, where the UMA originates mainly due to the stress, the origin of UMA in Co/Alq3 is attributed to the magnetocrystalline anisotropy caused by c-axis (Co (002)) preferential orientation. The surface free energy of Alq3 is less than that of Co; therefore, the growth of Co starts with island formation, which coalescences with increasing thickness. The observed structure orientation may be attributed to minimizing the magnetoelastic energies due to coalescence known as the zipping effect. The absence of UMA in films with lower thickness film (~5 nm) is understood in terms of random short-range stress caused by isotropic pinning due to the diffused interface.

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来源期刊
Journal of Superconductivity and Novel Magnetism
Journal of Superconductivity and Novel Magnetism 物理-物理:凝聚态物理
CiteScore
3.70
自引率
11.10%
发文量
342
审稿时长
3.5 months
期刊介绍: The Journal of Superconductivity and Novel Magnetism serves as the international forum for the most current research and ideas in these fields. This highly acclaimed journal publishes peer-reviewed original papers, conference proceedings and invited review articles that examine all aspects of the science and technology of superconductivity, including new materials, new mechanisms, basic and technological properties, new phenomena, and small- and large-scale applications. Novel magnetism, which is expanding rapidly, is also featured in the journal. The journal focuses on such areas as spintronics, magnetic semiconductors, properties of magnetic multilayers, magnetoresistive materials and structures, magnetic oxides, etc. Novel superconducting and magnetic materials are complex compounds, and the journal publishes articles related to all aspects their study, such as sample preparation, spectroscopy and transport properties as well as various applications.
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