An efficient first-principles approach to calculate x-ray magnetic circular dichroism (XMCD) and x-ray natural circular dichroism (XNCD) is developed and applied in the near-edge region at the K and L-1 edges in solids. Computation of circular dichroism requires precise calculations of x-ray absorption spectra (XAS) for circularly polarized light. For the derivation of the XAS cross section, we used a relativistic description of the photon-electron interaction that results in an additional term in the cross section that couples the electric dipole operator with an operator sigma . (is an element of x r) that we call the spin position operator. The numerical method relies on pseudopotentials, on the gauge including projected augmented-wave method, and on a collinear spin relativistic description of the electronic structure. We apply the method to calculations of K-edge XMCD spectra of ferromagnetic iron, cobalt, and nickel and of I L-1-edge XNCD spectra of alpha-LiIO3, a compound with broken inversion symmetry. For XMCD spectra we find that, even if the electric dipole term is the dominant one, the electric quadrupole term is not negligible (8% in amplitude in the case of iron). The term coupling the electric dipole operator with the spin-position operator is significant (28% in amplitude in the case of iron). We obtain a sum rule relating this term to the spin magnetic moment of the p states. In alpha-LiIO3 we recover the expected angular dependence of the XNCD spectra.

X-ray magnetic and natural circular dichroism from first principles: Calculation of K- and L-1-edge spectra / Bouldi, N.; Vollmers, N. J.; Delpy-Laplanche, C. G.; Joly, Y.; Juhin, A.; Sainctavit, Ph.; Brouder, Ch.; Calandra, M.; Paulatto, L.; Mauri, F.; Gerstmann, U.. - In: PHYSICAL REVIEW. B. - ISSN 2469-9950. - 96:8(2017). [10.1103/PhysRevB.96.085123]

X-ray magnetic and natural circular dichroism from first principles: Calculation of K- and L-1-edge spectra

Mauri, F.;
2017

Abstract

An efficient first-principles approach to calculate x-ray magnetic circular dichroism (XMCD) and x-ray natural circular dichroism (XNCD) is developed and applied in the near-edge region at the K and L-1 edges in solids. Computation of circular dichroism requires precise calculations of x-ray absorption spectra (XAS) for circularly polarized light. For the derivation of the XAS cross section, we used a relativistic description of the photon-electron interaction that results in an additional term in the cross section that couples the electric dipole operator with an operator sigma . (is an element of x r) that we call the spin position operator. The numerical method relies on pseudopotentials, on the gauge including projected augmented-wave method, and on a collinear spin relativistic description of the electronic structure. We apply the method to calculations of K-edge XMCD spectra of ferromagnetic iron, cobalt, and nickel and of I L-1-edge XNCD spectra of alpha-LiIO3, a compound with broken inversion symmetry. For XMCD spectra we find that, even if the electric dipole term is the dominant one, the electric quadrupole term is not negligible (8% in amplitude in the case of iron). The term coupling the electric dipole operator with the spin-position operator is significant (28% in amplitude in the case of iron). We obtain a sum rule relating this term to the spin magnetic moment of the p states. In alpha-LiIO3 we recover the expected angular dependence of the XNCD spectra.
2017
Multiple-scattering theory; 3D transition-metals; Foldy-Wouthuysen; transformation; atomic screening constants; absorpion fine-structures; augmented wave method; sum-rules; orbital-magnetization; electronic structure; edge absorption
01 Pubblicazione su rivista::01a Articolo in rivista
X-ray magnetic and natural circular dichroism from first principles: Calculation of K- and L-1-edge spectra / Bouldi, N.; Vollmers, N. J.; Delpy-Laplanche, C. G.; Joly, Y.; Juhin, A.; Sainctavit, Ph.; Brouder, Ch.; Calandra, M.; Paulatto, L.; Mauri, F.; Gerstmann, U.. - In: PHYSICAL REVIEW. B. - ISSN 2469-9950. - 96:8(2017). [10.1103/PhysRevB.96.085123]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1067932
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