Rotational Perturbation Theory for Magnetic Interactions

We develop rotational perturbation theory for magnetic interactions in collinear and noncollinear systems, distinguishing prescribed rotations of exchange fields from constrained rotations of magnetic moments. At the full exchange splitting, we derive Green-function expressions for prescribedfield energy curvatures directly from perturbation theory, without invoking the local force theorem; constrained-moment curvatures additionally require the stationary magnetic response and are related to the inverse static susceptibility. We examine noncollinear pair interactions and planar and conical spin spirals, and derive the long-wavelength ferromagnetic spin-wave stiffness and, assuming adiabatic sublattice precession, the antiferromagnetic spin-wave velocity. Orbital-nonlocal magnetic potentials and correlated electronic response reveal further requirements for connecting rotational curvatures to collective magnetic behavior. As a practical extension, we project the complete transverse pair Hessian onto an effective scalar Heisenberg exchange and quantify the unreconstructed curvature. Biquadratic and three-spin examples illustrate why locally extracted exchange coefficients need not represent transferable bilinear interactions.

Authors

Publication Details

Journal
arXiv (Cornell University)
Published
2026-10-27
DOI
https://doi.org/10.48550/arxiv.2610.36424
Primary Topic
Magnetic properties of thin films
Type
preprint
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
preprint

Rotational Perturbation Theory for Magnetic Interactions

Vladimir Antropov
arXiv (Cornell University)
Magnetic properties of thin films
preprint

Rotational Perturbation Theory for Magnetic Interactions

Vladimir Antropov
preprint en

Abstract

We develop rotational perturbation theory for magnetic interactions in collinear and noncollinear systems, distinguishing prescribed rotations of exchange fields from constrained rotations of magnetic moments. At the full exchange splitting, we derive Green-function expressions for prescribedfield energy curvatures directly from perturbation theory, without invoking the local force theorem; constrained-moment curvatures additionally require the stationary magnetic response and are related to the inverse static susceptibility. We examine noncollinear pair interactions and planar and conical spin spirals, and derive the long-wavelength ferromagnetic spin-wave stiffness and, assuming adiabatic sublattice precession, the antiferromagnetic spin-wave velocity. Orbital-nonlocal magnetic potentials and correlated electronic response reveal further requirements for connecting rotational curvatures to collective magnetic behavior. As a practical extension, we project the complete transverse pair Hessian onto an effective scalar Heisenberg exchange and quantify the unreconstructed curvature. Biquadratic and three-spin examples illustrate why locally extracted exchange coefficients need not represent transferable bilinear interactions.

arXiv (Cornell University)
Magnetic properties of thin films
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Laika access coming soon