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A Mesoscopic Hysteresis Model Based on the Unconstrained Minimization of the Gibbs Free Energy

机译:基于吉布斯自由能无约束最小化的介观磁滞模型

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Mesoscopic hysteresis models are based on a simplified description of the micromagnetic theory in order to simulate magnetization processes on the magnetic domain space scale. Hence, these models are situated between the micromagnetic and macroscopic models. In the presented mesoscopic description, the local magnetization is assumed to be aligned with either the cubic anisotropy axes or with the applied field. In this framework, the magnetization dynamics result from a constrained minimization of the Gibbs free energy. The numerical solution of this constrained minimization problem is highly time consuming. This paper presents a remapping of the model variables, which transforms the constrained minimization problem to an unconstrained problem and consequently results in a speed up and stabilization of the numerical scheme. Moreover, a model parameter analysis is carried out to further optimize the computational burden of the presented unconstrained procedure.
机译:介观磁滞模型基于微磁理论的简化描述,以便在磁畴空间尺度上模拟磁化过程。因此,这些模型位于微磁模型和宏观模型之间。在提出的介观描述中,假定局部磁化强度与立方各向异性轴或外加磁场对齐。在此框架中,磁化动力学是由吉布斯自由能的约束最小化产生的。这个受约束的最小化问题的数值解决方案非常耗时。本文提出了模型变量的重新映射,将约束最小化问题转换为无约束问题,从而导致数值方案的加速和稳定。此外,进行模型参数分析以进一步优化所提出的无约束过程的计算负担。

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