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Distribution functions of magnetic nanoparticles determined by a numerical inversion method

机译:用数值反演方法确定磁性纳米粒子的分布函数

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In the present study, we applied a regularized inversion method to extract the particle size, magnetic moment and relaxation-time distribution of magnetic nanoparticles from small-angle x-ray scattering (SAXS), DC magnetization (DCM) and AC susceptibility (ACS) measurements. For the measurements the particles were colloidally dispersed in water. At first approximation the particles could be assumed to be spherically shaped and homogeneously magnetized single-domain particles. As model functions for the inversion, we used the particle form factor of a sphere (SAXS), the Langevin function (DCM) and the Debye model (ACS). The extracted distributions exhibited features/peaks that could be distinctly attributed to the individually dispersed and non-interacting nanoparticles. Further analysis of these peaks enabled, in combination with a prior characterization of the particle ensemble by electron microscopy and dynamic light scattering, a detailed structural and magnetic characterization of the particles. Additionally, all three extracted distributions featured peaks, which indicated deviations of the scattering (SAXS), magnetization (DCM) or relaxation (ACS) behavior from the one expected for individually dispersed, homogeneously magnetized nanoparticles. These deviations could be mainly attributed to partial agglomeration (SAXS, DCM, ACS), uncorrelated surface spins (DCM) and/or intra-well relaxation processes (ACS). The main advantage of the numerical inversion method is that no ad hoc assumptions regarding the line shape of the extracted distribution functions are required, which enabled the detection of these contributions. We highlighted this by comparing the results with the results obtained by standard model fits, where the functional form of the distributions was a priori assumed to be log-normal shaped.
机译:在本研究中,我们应用正则化反演方法从小角度X射线散射(SAXS),直流磁化(DCM)和交流磁化率(ACS)提取磁性纳米粒子的粒径,磁矩和弛豫时间分布测量。为了进行测量,将颗粒胶体分散在水中。最初近似时,可以假定这些粒子是球形且均匀磁化的单畴粒子。作为反演的模型函数,我们使用了球体的粒子形状因子(SAXS),朗格文函数(DCM)和德拜模型(ACS)。提取的分布表现出可以明显归因于单独分散且不相互作用的纳米颗粒的特征/峰。对这些峰的进一步分析与通过电子显微镜和动态光散射对粒子整体的先验表征相结合,可以对粒子进行详细的结构和磁学表征。此外,所有三个提取的分布均具有峰,这表明散射(SAXS),磁化(DCM)或弛豫(ACS)行为与单独分散的,均匀磁化的纳米颗粒所预期的行为之间存在偏差。这些偏差可能主要归因于部分团聚(SAXS,DCM,ACS),不相关的表面自旋(DCM)和/或井内弛豫过程(ACS)。数值反演方法的主要优点是,不需要关于提取的分布函数的线形的特殊假设,从而可以检测这些贡献。我们通过将结果与通过标准模型拟合获得的结果进行比较来突出显示这一点,其中先验分布的功能形式被假定为对数正态形状。

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