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Correlating Electronic Structure and Photoluminescence in CrSBr: Insights from XAS, RIXS, and XEOL

ORAL

Abstract

Magnetic van der Waals (vdW) materials have attracted significant attention over the last decade. Owing to their quasi-2D behavior, the possibility to control the number of layers and to construct vertical heterostructures, these systems offer vast possibilities to explore new physics and design advanced spintronic devices. In this context, Cr-based vdW magnets display a great potential thanks to their optical and magnetic characteristics.

We focus here on the vdW antiferromagnet CrSBr. Its stability in air, together with its unique magnetoelectric coupling properties, makes this system one of the most promising materials for future optoelectronic applications. Indeed, it hosts at least two optically active excitons strongly coupled to the magnetic state of the system. They are at the origin of a strong photoluminescence (PL), which is tunable in energy and shape by: strain, number of layers, and by driving the system from an anti-ferromagnetic to a ferromagnetic phase upon the application of a relatively weak magnetic field of about 0.35 T.

To gain deeper insight into the mechanisms governing the observed PL and to relate it with the electronic structure of CrSBr, we correlate X-ray Absorption Spectroscopy (XAS), Resonant Inelastic X-ray Scattering (RIXS), and X-ray Excited Optical Luminescence (XEOL), acquired in one single experiment and therefore in same experimental conditions. Our measurements reveal significant linear dichroism, along with signatures of characteristic Cr3+ d-d transitions, which we attempt to model using crystal field calculations. To further explore the relationship between magnetic properties and PL behavior, we also present the evolution of both RIXS and PL under an applied magnetic field. This study highlights the benefits of combining excitation and recombination spectroscopy techniques.

Publication: Planned paper : Investigation of magneto-optical van der Waals magnet via correlative spectroscopic techniques<br>To be submitted to PRB within the next few weeks.

Presenters

  • Victor Porée

    Synchrotron SOLEIL, Synchrotron SOLEIL, L'Orme des Merisiers, Saint-Aubin, BP 48, F-91192 Gif-sur-Yvette, France

Authors

  • Victor Porée

    Synchrotron SOLEIL, Synchrotron SOLEIL, L'Orme des Merisiers, Saint-Aubin, BP 48, F-91192 Gif-sur-Yvette, France

  • Alberto Zobelli

    Laboratoire de Physique des Solides, Universit e Paris-Saclay, CNRS UMR 8502, F-91405, Orsay, France, Laboratoire de Physique des Solides, Université Paris-Saclay, CNRS UMR 8502, F-91405, Orsay, France

  • Amit Pawbake

    LNCMI-EMFL. CNRS, Univ. Grenoble Alpes, Univ. Toulouse, Laboratoire National des Champs Magnétiques Intenses, CNRS-UGA-UPS-INSA-EMFL, 38042, Grenoble, France

  • Jakub Regner

    Department of Inorganic Chemistry, University of Chemistry and Technology Prague, Technicka 5, 166 28 Prague 6, Czech Republic

  • Zdenek Sofer

    University of Chemistry and Technology Prague, Department of Inorganic Chemistry, University of Chemistry and Technology Prague

  • Clement Faugeras

    LNCMI-EMFL. CNRS, Univ. Grenoble Alpes, Univ. Toulouse, Laboratoire National des Champs Magnétiques Intenses, CNRS-UGA-UPS-INSA-EMFL, 38042, Grenoble, France, LNCMI, CNRS

  • Alessandro Nicolaou

    Synchrotron SOLEIL, L'Orme des Merisiers, Saint-Aubin, BP 48, F-91192 Gif-sur-Yvette, France