Bohn F, Corrêa M A, Carara M, Papanikolaou S, Durin G, Sommer R L
Departamento de Física Teórica e Experimental, Universidade Federal do Rio Grande do Norte, 59078-970 Natal, RN, Brazil.
Departamento de Física, Universidade Federal de Santa Maria, 97105-900 Santa Maria, RS, Brazil.
Phys Rev E Stat Nonlin Soft Matter Phys. 2014 Sep;90(3):032821. doi: 10.1103/PhysRevE.90.032821. Epub 2014 Sep 29.
We investigate the statistical properties of the Barkhausen noise in amorphous ferromagnetic films with thicknesses in the range between 100 and 1000 nm. From Barkhausen noise time series measured with the traditional inductive technique, we perform a wide statistical analysis and establish the scaling exponents τ,α,1/σνz, and ϑ. We also focus on the average shape of the avalanches, which gives further indications on the domain-wall dynamics. Based on experimental results, we group the amorphous films in a single universality class, characterized by scaling exponents τ=1.28±0.02,α=1.52±0.3, and 1/σνz=ϑ=1.83±0.03, values compatible with that obtained for several bulk amorphous magnetic materials. Besides, we verify that the avalanche shape depends on the universality class. By considering the theoretical models for the dynamics of a ferromagnetic domain wall driven by an external magnetic field through a disordered medium found in literature, we interpret the results and identify an experimental evidence that these amorphous films, within this thickness range, present a typical three-dimensional magnetic behavior with predominant short-range elastic interactions governing the domain-wall dynamics. Moreover, we provide experimental support for the validity of a general scaling form for the average avalanche shape for non-mean-field systems.
我们研究了厚度在100至1000纳米范围内的非晶铁磁薄膜中巴克豪森噪声的统计特性。通过传统感应技术测量的巴克豪森噪声时间序列,我们进行了广泛的统计分析,并确定了标度指数τ、α、1/σνz和ϑ。我们还关注雪崩的平均形状,这为畴壁动力学提供了进一步的指示。基于实验结果,我们将非晶薄膜归为单一的普适类,其特征标度指数为τ = 1.28±0.02、α = 1.52±0.3以及1/σνz = ϑ = 1.83±- 03,这些值与几种块状非晶磁性材料所获得的值相符。此外,我们验证了雪崩形状取决于普适类。通过考虑文献中发现的由外部磁场驱动通过无序介质的铁磁畴壁动力学的理论模型,我们解释了结果,并确定了一个实验证据,即在该厚度范围内,这些非晶薄膜呈现出典型的三维磁行为,其中主要的短程弹性相互作用支配着畴壁动力学。此外,我们为非平均场系统的平均雪崩形状的一般标度形式的有效性提供了实验支持。