首页> 美国卫生研究院文献>Scientific Reports >Spin-glass-like freezing of inner and outer surface layers in hollow γ-Fe2O3 nanoparticles
【2h】

Spin-glass-like freezing of inner and outer surface layers in hollow γ-Fe2O3 nanoparticles

机译:空心γ-Fe2O3纳米粒子内外表面层的自旋玻璃状冻结

代理获取
本网站仅为用户提供外文OA文献查询和代理获取服务,本网站没有原文。下单后我们将采用程序或人工为您竭诚获取高质量的原文,但由于OA文献来源多样且变更频繁,仍可能出现获取不到、文献不完整或与标题不符等情况,如果获取不到我们将提供退款服务。请知悉。

摘要

Disorder among surface spins is a dominant factor in the magnetic response of magnetic nanoparticle systems. In this work, we examine time-dependent magnetization in high-quality, monodisperse hollow maghemite nanoparticles (NPs) with a 14.8 ± 0.5 nm outer diameter and enhanced surface-to-volume ratio. The nanoparticle ensemble exhibits spin-glass-like signatures in dc magnetic aging and memory protocols and ac magnetic susceptibility. The dynamics of the system slow near 50 K, and become frozen on experimental time scales below 20 K. Remanence curves indicate the development of magnetic irreversibility concurrent with the freezing of the spin dynamics. A strong exchange-bias effect and its training behavior point to highly frustrated surface spins that rearrange much more slowly than interior spins. Monte Carlo simulations of a hollow particle corroborate strongly disordered surface layers with complex energy landscapes that underlie both glass-like dynamics and magnetic irreversibility. Calculated hysteresis loops reveal that magnetic behavior is not identical at the inner and outer surfaces, with spins at the outer surface layer of the 15 nm hollow particles exhibiting a higher degree of frustration. Our combined experimental and simulated results shed light on the origin of spin-glass-like phenomena and the important role played by the surface spins in magnetic hollow nanostructures.
机译:表面自旋之间的无序是磁性纳米粒子系统的磁响应中的主要因素。在这项工作中,我们研究了高质量的单分散空心磁赤铁矿纳米颗粒(NPs)中随时间变化的磁化强度,该纳米颗粒的外径为14.8±0.5 nm,表面积与体积比得到增强。纳米粒子集合体在直流磁老化和存储协议以及交流磁化率中表现出类似自旋玻璃的特征。该系统的动力学在接近50 K时变慢,并在低于20 experimentalK的实验时间尺度上冻结。剩磁曲线表明磁不可逆性的发展与自旋动力学的冻结同时发生。强烈的交换偏向效应及其训练行为表明,高度受挫的表面旋转比内部旋转慢得多。空心粒子的蒙特卡洛模拟证实了具有复杂能量分布的严重无序的表面层,这些能量分布是玻璃状动力学和磁性不可逆性的基础。计算出的磁滞回线表明,内,外表面的磁性能不同,在15 nm中空粒子的外表面层的自旋表现出更高的挫败感。我们的组合实验和模拟结果揭示了类自旋玻璃现象的起源以及表面自旋在磁性空心纳米结构中的重要作用。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
代理获取

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号