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On the Néel Vector Dependence of X-ray Magnetic Circular Dichroism in Altermagnets

Jan Kuneš

TL;DR

This work develops a group-theoretical framework to relate the x-ray Hall vector $\mathbf{h}(\omega)$ to the Néel vector $\mathbf{L}$ in altermagnets under the free valence spin (FVS) approximation. The authors show that $\mathbf{h}(\omega)$ depends linearly on $\mathbf{L}$ through symmetry-determined spectral functions, yielding the general form $\mathbf{h}(\omega)=\tfrac{1}{2}\big(\boldsymbol{\Omega}(\omega)-\mathbf{g}\boldsymbol{\Omega}(\omega)\mathbf{g}^T\big)\hat{\mathbf{L}}$, where $\boldsymbol{\Omega}$ encodes site- and edge-specific invariants and $\mathbf{g}$ maps between magnetic sublattices. Applying this to rutile and NiAs structures shows that XMCD can be allowed or forbidden purely by symmetry in FVS, with rutile yielding a single spectral function linking $\mathbf{h}$ to $\mathbf{L}$ (and enabling in-plane domain imaging), while NiAs generally suppresses XMCD unless symmetry is lowered by core-valence exchange or valence SOC. Across representative altermagnets, including MnTe and CrSb, the framework clarifies when core-valence effects are essential to observe XMCD and provides a compact, symmetry-based route to interpret XMCD data as a probe of Néel-vector orientation and domain structure.

Abstract

Dependence of x-ray magnetic circular dichroism on the experimental geometry is described by a frequency-dependent Hall vector. Using group theory, we derive a general relationship between the Hall vector and the orientation of the Néel vector $\bL$ in altermagnets within the free valence spin (FVS) approximation, where the spin-orbit coupling of the valence electrons and their exchange interaction with the core electrons are neglected. For a given spin point group, the full $\bL$-dependence of the Hall vector can be expressed in terms of several irreducible spectral functions. This derivation generalizes earlier results for the special cases of MnTe and MnF$_2$. Depending on the system symmetry, XMCD in the FVS approximation may be present, emerge only when the neglected terms are included, or be completely forbidden.

On the Néel Vector Dependence of X-ray Magnetic Circular Dichroism in Altermagnets

TL;DR

This work develops a group-theoretical framework to relate the x-ray Hall vector to the Néel vector in altermagnets under the free valence spin (FVS) approximation. The authors show that depends linearly on through symmetry-determined spectral functions, yielding the general form , where encodes site- and edge-specific invariants and maps between magnetic sublattices. Applying this to rutile and NiAs structures shows that XMCD can be allowed or forbidden purely by symmetry in FVS, with rutile yielding a single spectral function linking to (and enabling in-plane domain imaging), while NiAs generally suppresses XMCD unless symmetry is lowered by core-valence exchange or valence SOC. Across representative altermagnets, including MnTe and CrSb, the framework clarifies when core-valence effects are essential to observe XMCD and provides a compact, symmetry-based route to interpret XMCD data as a probe of Néel-vector orientation and domain structure.

Abstract

Dependence of x-ray magnetic circular dichroism on the experimental geometry is described by a frequency-dependent Hall vector. Using group theory, we derive a general relationship between the Hall vector and the orientation of the Néel vector in altermagnets within the free valence spin (FVS) approximation, where the spin-orbit coupling of the valence electrons and their exchange interaction with the core electrons are neglected. For a given spin point group, the full -dependence of the Hall vector can be expressed in terms of several irreducible spectral functions. This derivation generalizes earlier results for the special cases of MnTe and MnF. Depending on the system symmetry, XMCD in the FVS approximation may be present, emerge only when the neglected terms are included, or be completely forbidden.

Paper Structure

This paper contains 3 sections, 8 equations, 1 table.