X-ray magnetic and natural circular dichroism from first principles: Calculation of K- and L1-edge spectra

N. Bouldi, N. J. Vollmers, C. G. Delpy-Laplanche, Y. Joly, A. Juhin, Ph. Sainctavit, Ch. Brouder, M. Calandra, L. Paulatto, F. Mauri, and U. Gerstmann
Phys. Rev. B 96, 085123 – Published 17 August 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 L1 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 σ·(ε×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 L1-edge XNCD spectra of αLiIO3, 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 αLiIO3 we recover the expected angular dependence of the XNCD spectra.

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  • Received 4 April 2017

DOI:https://doi.org/10.1103/PhysRevB.96.085123

©2017 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

N. Bouldi1,2,*, N. J. Vollmers3, C. G. Delpy-Laplanche1, Y. Joly4, A. Juhin1, Ph. Sainctavit1, Ch. Brouder1, M. Calandra1, L. Paulatto1, F. Mauri5, and U. Gerstmann3

  • 1UPMC Université Paris 6, CNRS, UMR 7590, IRD, MNHN, Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, case 115, 4 place Jussieu, 75252 Paris Cedex 5, France
  • 2Synchrotron SOLEIL, L'Orme des Merisiers, Saint-Aubin, Boîte Postale 48, 91192 Gif-sur-Yvette Cedex, France
  • 3Lehrstuhl für Theoretische Physik, Universität Paderborn, Warburger Strasse 100, 33098 Paderborn, Germany
  • 4Institut Néel, CNRS and Université Joseph Fourier, Boîte Postale 166, 38042 Grenoble Cedex 9, France
  • 5Departimento di Fisica, Università di Roma La Sapienza, Piazzale Aldo Moro 5, 00185 Roma, Italy

  • *nadejda.bouldi@impmc.upmc.fr

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Vol. 96, Iss. 8 — 15 August 2017

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