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Interface roughness driven magnetic anisotropy and Dzyaloshinskii- Moriya interaction in thin films with broken structural inversion symmetry.

机译:界面粗糙度驱动的薄膜的各向异性和Dzyaloshinskii-Moriya相互作用具有破坏的结构反转对称性。

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An interface between 3d transition metal and 5d(4d) heavy metal (HM) is a host of intriguing spin-related effects desirable for spin-orbitronic applications [1]. Chiral interaction between two 3d spins due to a strong spin-orbit coupling (SOC) in an underlying atomic layer of heavy metal is associated with the Dzyaloshinskii-Moriya interaction (DMI) [2]. The and interfacial DMI (iDMI) value is extremely sensitive to the ferromagnetic layer thickness tFM, where the non-linear dependence of iDMI on tFM implies the degradation of interfaces at small tFM [3]. Recently, Wells et al. [4] has demonstrated the effect of interface quality, reflecting both roughness and intermixing of interfaces, on iDMI in symmetrical Pt/Co/Pt trilayers. There is a radically different situation in the inversion symmetry broken systems, where the ideal (which is difficult to achieve in polycrystalline films) or having identical quality of top and bottom interfaces of a ferromagnetic layer are the main source of the enhanced iDMI [5], [6]. One can suppose that if in such systems the quality parameter, defined as the difference between quality of top and bottom interfaces of the magnetic layer, tends to zero, iDMI will be strong. The case of the coherent roughnesses of top and bottom interfaces corresponds to this assumption, which arises from the sensitivity of iDMI to the magnetic layer thickness variation. We report on results of the investigation of the magnetic anisotropy and interfacial DMI in the magnetic layer sandwiched between two 5d HM (Pt and Ta) (Series 1 - Pt(2)/CoFeSiB(1.5)/Ta(5)) or one 5d HM (Pt) from the bottom and 4d HM (Ru) from the top (Series - 2 Pt(2)/CoFeSiB(1.5)/Ru(3)/Ta(5)), where the layer's thickness is indicated in nm. The two series of samples were deposited by magnetron sputtering on the top of the Pd surface with artificially introduced interface roughness: The substrates with Pd seed layer of different thickness ranging from 0 to 56 ML (or from 0 to 12.6 nm were epitaxially grown on the atomically smooth Si(111)/Cu surface. Roughness of the Pd surface in dependence on the thickness was measured by and AFM. The surface is represented by well-ordered atomic terraces of Si, covered by Cu seed layer with the Pd islands grown on top of it. The island growth leads to the significant increase of the mean-square roughness (Rq) as well as the amplitude of roughnesses of the Pd surface. But the period of roughnesses remains constant within the value distribution: p = 70 10 nm. In order to analyze the interface quality (roughness, intermixing, thickness variation) we used the X-ray reflectivity (XRR) measurement technique. The study was performed on a SmartLab (RIGAKU) X-ray diffractometer at CuK radiation wavelength (1.54Å). The simulations of XRR spectra were performed with GlobalFit software. The main trend is the increase of the interface roughness for all layers with the rising tPd. Noteworthy, the initial Rq for CoFeSiB is higher than for rest layers. It can relate to the amorphous nature of the magnetic layer. With increase of tPd up to 10.2 nm roughness of CoFeSiB layer approaches to Rq of the underneath Pd and Pt layers, which corresponds to the roughness coherency. The experimental data revealed that Ta capping layer smooths the surface roughness. We observed the correlation between the interface quality factor and iDMI for both series. The direct measurement of DMI was performed by Brillouin light scattering (BLS) spectroscopy based on DMI-driven asymmetric dispersion shift of long-wavelength thermal spin waves in the Damon-Eshbach surface mode. At the small Pd roughness the magnitude of has maximum that means the highest incoherency between top and bottom interfaces of CoFeSiB layer leading to the relatively small iDMI. The flowing tendency of with rising tPd reflects the growing coherence of interface roughnesses causing in significant increase of iDMI about twice for series 1 and 2. We demonstrate the direct dependence between the quality of CoFeSiB interfaces, the iDMI value and magnetic anisotropy. The coherent roughnesses of top and bottom interfaces can enhance the iDMI value up to 2.5 times with the maximum obtained value Deff = -0.9 mJ m2 or surface DMI is Ds = -1.05 pJ/m), which is largest known iDMI for CoFeB-based systems. For samples with high iDMI we observed the isolated skyrmions (or skyrmion bubbles) formation with the size about 200-300 nm.
机译:3d过渡金属和5d(4d)重金属(HM)之间的界面是自旋或双电子应用所需要的许多有趣的自旋相关效应[1]。由于重金属下面的原子层中的强自旋轨道耦合(SOC),两个3d自旋之间的手性相互作用与Dzyaloshinskii-Moriya相互作用(DMI)相关[2]。界面DMI(iDMI)值对铁磁层厚度t极为敏感 FM ,其中iDMI对t的非线性依赖性 FM 暗示在小t时接口的性能下降 FM [3]。最近,Wells等人。 [4]已经证明了界面质量对对称Pt / Co / Pt三层iDMI的影响,反映了界面的粗糙度和混合。反对称对称破碎系统存在截然不同的情况,其中理想的(在多晶膜中很难实现)或铁磁层的顶部和底部界面质量相同是增强iDMI的主要来源[5]。 ,[6]。可以假设,如果在这样的系统中,定义为磁性层顶部和底部界面质量之间的差异的质量参数趋于零,则iDMI将很强。顶部和底部界面的相干粗糙度的情况与该假设相对应,这是由于iDMI对磁性层厚度变化的敏感性所致。我们报告了夹在两个5d HM(Pt和Ta)(系列1-Pt(2)/ CoFeSiB(1.5)/ Ta(5))或一个5d之间的磁性层中的磁各向异性和界面DMI的调查结果从底部开始的HM(Pt),从顶部开始的4d HM(Ru)(系列-2 Pt(2)/ CoFeSiB(1.5)/ Ru(3)/ Ta(5)),其中层的厚度以nm表示。通过磁控溅射将这两个系列的样品沉积在具有人工引入的界面粗糙度的Pd表面顶部上:在Pd表面上外延生长具有厚度范围为0到56 ML(或0到12.6 nm)的Pd种子层的基板。原子光滑的Si(111)/ Cu表面,Pd表面的粗糙度随厚度的变化通过AFM和AFM进行测量,该表面以有序的Si原子台阶表示,被Si晶种层覆盖,并在Pd岛上生长了Pd岛。岛的增长导致均方根粗糙度(R q )以及Pd表面的粗糙度幅度。但是粗糙度周期在值分布内保持恒定:p = 70 10 nm。为了分析界面质量(粗糙度,混合度,厚度变化),我们使用了X射线反射率(XRR)测量技术。该研究是在SmartLab(RIGAKU)X射线衍射仪上以CuK辐射波长(1.54Å)进行的。 XRR光谱的模拟是使用GlobalFit软件进行的。主要趋势是,随着t的增加,所有层的界面粗糙度都会增加 Pd 。值得注意的是,初始R q CoFeSiB的含量高于其余层。它可能与磁性层的非晶性有关。随着t的增加 Pd CoFeSiB层的粗糙度可达R的10.2 nm q 下层Pd和Pt层的厚度,对应于粗糙度相干性。实验数据表明,Ta覆盖层可平滑表面粗糙度。我们观察到两个系列的接口质量因子和iDMI之间的相关性。 DMI的直接测量是通过布里渊光散射(BLS)光谱法进行的,该光谱基于DMI驱动的Damon-Eshbach表面模式下长波长热自旋波的不对称色散位移。在较小的Pd粗糙度下,的幅值最大,这意味着CoFeSiB层的顶部和底部界面之间的最高不相干性导致了相对较小的iDMI。 t上升的流动趋势 Pd 反映了界面粗糙度不断增长的连贯性,导致系列1和2的iDMI显着增加了大约两倍。我们证明了CoFeSiB界面质量之间的直接相关性,iDMI值和磁各向异性。顶部和底部界面的相干粗糙度可将iDMI值提高至2.5倍,最大获得值D eff = -0.9兆焦耳米 2 或表面DMI为Ds = -1.05 pJ / m),这是基于CoFeB的系统中最大的已知iDMI。对于具有高iDMI的样品,我们观察到形成了约200-300 nm大小的孤立的天空蛋白(或天空蛋白气泡)。

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