首页> 外文期刊>Journal of magnetism and magnetic materials >Probing the electronic structure of Ni-Mn-In-Si based Heusler alloys thin films using magneto-optical spectra in martensitic and austenitic phases
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Probing the electronic structure of Ni-Mn-In-Si based Heusler alloys thin films using magneto-optical spectra in martensitic and austenitic phases

机译:利用马氏体和奥氏体相的磁光光谱探测Ni-Mn-In-Si基Heusler合金薄膜的电子结构

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摘要

Thin films of Ni_(52)Mn_(35−) _xIn_(11+) _xSi_2 were fabricated by magnetron sputtering on MgO (0 0 1) single crystal substrates. Magnetization as function of temperature for Ni_(52)Mn_(35)In_(11)Si_2 exhibits features consistent with a magnetostructural transition (MST) from an austenitic phase to a martensitic phase, similar to the bulk material. We observed that the martensitic transformation is externally sensitive to small changes in chemical composition and stoichiometry. It has been found that thin films of Ni_(52)Mn_(34−) _xIn_(11+) _xSi_2 with x = 0 and 1 undergo a temperature-induced MST or remain in a stable austenitic phase, respectively. Comparison of magneto-optical transverse Kerr effect spectra obtained at 0.5-4.0 eV in the 35-300 K temperature interval reveal insignificant differences between the martensitic and austenite phases. We found that the field and temperature dependencies of the transverse Kerr effect are quite different from the magnetization behavior, which is attributed to magnetic inhomogeneity across the films. To elucidate the effects of magnetostructural phase transitions on the electronic properties, we performed density functional calculations of the magneto-optical Kerr effect.
机译:Ni_(52)Mn_(35-)_xIn_(11+)_xSi_2的薄膜是通过磁控溅射在MgO(0 0-1)单晶衬底上制成的。 Ni_(52)Mn_(35)In_(11)Si_2的磁化强度与温度的关系与块状材料相似,具有与从奥氏体相到马氏体相的磁结构转变(MST)相一致的特征。我们观察到,马氏体转变对化学成分和化学计量的微小变化在外部敏感。已发现x = 0和1的Ni_(52)Mn_(34-)_xIn_(11+)_xSi_2薄膜分别经历了温度诱发的MST或保持稳定的奥氏体相。在35-300 K温度范围内以0.5-4.0 eV获得的磁光横向Kerr效应谱的比较显示,马氏体相和奥氏体相之间的差异不明显。我们发现横向克尔效应的场和温度相关性与磁化行为有很大不同,这归因于整个薄膜的磁不均匀性。为了阐明磁结构相变对电子性能的影响,我们对磁光克尔效应进行了密度泛函计算。

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  • 来源
    《Journal of magnetism and magnetic materials》 |2017年第6期|455-460|共6页
  • 作者单位

    Department of Physics, Lomonosov Moscow State University, Moscow, Russian Federation;

    Department of Physics and Astronomy, University of Nebraska-Lincoln, Lincoln, NE, United States;

    Department of Physics, Lomonosov Moscow State University, Moscow, Russian Federation;

    Department of Physics, Southern Illinois University, Carbondale, IL, United States;

    Department of Physics, Southern Illinois University, Carbondale, IL, United States;

    Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA, United States;

    Department of Physics, Southern Illinois University, Carbondale, IL, United States;

    Department of Physics, Lomonosov Moscow State University, Moscow, Russian Federation;

    Department of Physics, Lomonosov Moscow State University, Moscow, Russian Federation;

    Lappeenranta University of Technology, Finland;

    Dpto. de Física de Materiales, Fac. Químicas, UPV/EHU, San Sebastian, Spain,IKERBASQUE, Basque Foundation for Science, Bilbao, Spain;

    Department of Physics, Lomonosov Moscow State University, Moscow, Russian Federation;

    Department of Physics, University of Nebraska at Omaha, Omaha, NE, United States;

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