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自旋波的从头算计算:理论方法与应用综述

Ab Initio Calculations of Spin Waves: A Review of Theoretical Approaches and Applications.

作者信息

Neugum Michael, Schindlmayr Arno

机构信息

Department Physik, Universität Paderborn, 33095 Paderborn, Germany.

出版信息

Materials (Basel). 2025 Sep 22;18(18):4431. doi: 10.3390/ma18184431.

DOI:10.3390/ma18184431
PMID:41010273
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC12471309/
Abstract

Spin waves represent an important class of low-energy excitations in magnetic solids, which influence the thermodynamic properties and play a major role in technical applications, such as spintronics or magnetic data storage. Despite the enormous advances of ab initio simulations in materials science, quantitative calculations of spin-wave spectra still pose a significant challenge, because the collective nature of the spin dynamics requires an accurate treatment of the Coulomb interaction between the electrons. As a consequence, simple lattice models like the Heisenberg Hamiltonian are still widespread in practical investigations, but modern techniques like time-dependent density-functional theory or many-body perturbation theory also open a route to material-specific spin-wave calculations from first principles. Although both are in principle exact, actual implementations necessarily employ approximations for electronic exchange and correlation as well as additional numerical simplifications. In this review, we recapitulate the theoretical foundations of ab initio spin-wave calculations and analyze the common approximations that underlie present implementations. In addition, we survey the available results for spin-wave dispersions of various magnetic materials and compare the performance of different computational approaches. In this way, we provide an overview of the present state of the art and identify directions for further developments.

摘要

自旋波是磁性固体中一类重要的低能激发,它影响热力学性质,并在诸如自旋电子学或磁数据存储等技术应用中发挥重要作用。尽管从头算模拟在材料科学领域取得了巨大进展,但自旋波谱的定量计算仍然面临重大挑战,因为自旋动力学的集体性质要求精确处理电子之间的库仑相互作用。因此,像海森堡哈密顿量这样的简单晶格模型在实际研究中仍然广泛使用,但诸如含时密度泛函理论或多体微扰理论等现代技术也为从第一性原理进行特定材料的自旋波计算开辟了一条途径。虽然这两种方法原则上都是精确的,但实际实现必然要对电子交换和关联采用近似以及进行额外的数值简化。在本综述中,我们概述了从头算自旋波计算的理论基础,并分析了当前实现方法所基于的常见近似。此外,我们考察了各种磁性材料自旋波色散的现有结果,并比较了不同计算方法的性能。通过这种方式,我们提供了当前技术水平的概述,并确定了进一步发展的方向。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/6c532df58229/materials-18-04431-g009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/962f92d9bf80/materials-18-04431-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/25c90c162d47/materials-18-04431-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/7afb6f87abb6/materials-18-04431-g003.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/d39e1f7921f8/materials-18-04431-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/f43ac9d2a8f5/materials-18-04431-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/3191e0de398b/materials-18-04431-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/6c532df58229/materials-18-04431-g009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/962f92d9bf80/materials-18-04431-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/25c90c162d47/materials-18-04431-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/7afb6f87abb6/materials-18-04431-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/2b99ca4f52c6/materials-18-04431-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/72f139d70db5/materials-18-04431-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/d39e1f7921f8/materials-18-04431-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c8f5/12471309/f43ac9d2a8f5/materials-18-04431-g007.jpg
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