Dynamics of Agglomeration of Magnetite Nanoparticles under Magnetic Field Studied by Monitoring Magnetic Weight

RAN Pub Date : 2016-04-01 DOI:10.11159/ICNEI16.102
D. Jin, Hackjin Kim
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Abstract

Extended Abstract One of many important applications of magnetic nanoparticles is the separation of complex mixture by magnetic field [1]. Magnetic nanoparticles aggregate with impurities of the mixture under magnetic field in the separation process. We have built a simple experimental setup for monitoring the temporal change of magnetic weight with a conventional electronic balance in order to study the agglomeration dynamics of magnetite nanoparticles by magnetic field [2]. The magnetic field is applied in the direction parallel to the gravitational force in our setup. Magnetite nanoparticles are prepared by reacting FeCl2 and FeCl3 in aqueous ammonia solution [3]. When the ferrofluid sample is placed under the field, the magnetic weight of the sample jumps instantaneously by Neel and Brown relaxation, and then increases slowly over a few days as the nanoparticles agglomerate. The slow increase of the magnetic weight shows the stretched exponential behaviour, M(t) = M() + [M(0) – M()] exp[-(t/)  ] where 0 <  < 1. The stretched exponential function results from the distribution of energy barrier involved in the dynamics, which can be calculated by the inverse Laplace transformation of the stretched exponential function if the Arrhenius pre-exponent factor of the rate constant is given [4]. Typical agglomeration of magnetite nanoparticles by magnetic field gives the energy barrier distribution function with the peak energy of ~36 kJ mol -1 and the width of ~8 kJ mol -1 [5]. In addition to the overall stretched exponential change, the magnetic weight of ferrofluid shows thermal fluctuation, which is explained well with the Boltzmann factor. The energy difference of < 10 kJ mol -1 , estimated from the temperature dependence of the dynamics, that is, the Boltzmann factor corresponds to the energy difference between the agglomerated states. Again, this energy difference is not a single value but shows some distribution.
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磁重监测研究磁铁矿纳米颗粒在磁场作用下的团聚动力学
磁性纳米颗粒的许多重要应用之一是利用磁场分离复杂混合物[1]。在分离过程中,磁性纳米颗粒与混合物中的杂质在磁场作用下聚集。为了研究磁铁矿纳米颗粒在磁场作用下的团聚动力学,我们建立了一个简单的实验装置,用传统的电子天平监测磁重的时间变化[2]。在我们的设置中,磁场作用的方向与重力平行。通过FeCl2和FeCl3在氨水溶液中反应制备磁铁矿纳米颗粒[3]。当铁磁流体样品被放置在磁场下时,样品的磁性重量通过尼尔和布朗弛豫瞬间跳跃,然后随着纳米颗粒的聚集而在几天内缓慢增加。磁重的缓慢增加表现为拉伸指数行为,M(t) = M()+ [M(0) - M()]exp[-(t/)],其中0 << 1。拉伸指数函数是动力学中涉及的能量势垒分布的结果,如果给定速率常数的Arrhenius指数前因子[4],则可以通过拉伸指数函数的拉普拉斯逆变换来计算。典型的磁铁矿纳米颗粒在磁场作用下的团聚得到能量势垒分布函数,其峰值能量为~36 kJ mol -1,宽度为~8 kJ mol -1[5]。除了整体的拉伸指数变化外,铁磁流体的磁重还表现出热波动,这可以用玻尔兹曼因子很好地解释。从动力学的温度依赖性估计出的能量差< 10 kJ mol -1,即玻尔兹曼因子对应于凝聚态之间的能量差。同样,这个能量差不是一个单一的值,而是有一定的分布。
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