Spin-flip Determination in CrX<sub>3</sub> (X = Cl, Br, and I) 2D Magnets using High-resolution X-ray Scattering

ORAL

Abstract

Chromium tri-halides CrX3 (X = Cl, Br, and I) exhibit low-temperature, layer-dependent magnetism that can be manipulated by an electric field, which makes them important candidates for spintronics applications. Their magnetic ground states depend keenly on electronic parameters such as spin-orbit coupling (SOC), Hund’s coupling (JH ), p−d covalency, and interorbital Coulomb interactions. Therefore, accurately determining these parameters is paramount for understanding the CrX3 physics. We have used resonant inelastic x-ray scattering (RIXS) spectroscopy facilitated by ligand field multiplet calculations in C3 symmetry to simulate experimental RIXS spectra. Tanabe-Sugano-like energy level diagram calculations facilitated the determination of detailed electronic structure parameters in CrX3. These methods provide the most detailed description of CrX3 magneto-optical and electronic energetic (terms) to date. The determined 10Dq values are in good agreement with the spectrochemical series, the Racah B parameter follows the expected Nephelauxetic effect, and the crystal field distortion parameters Dσ and Dτ are calculated for the first time. Moreover, high-resolution RIXS spectra reveal a clear energy separation between spin-allowed quartet and spin-forbidden doublet states in CrX3, showcasing the potential of this technique in determining materials’ electronic parameters. This study validates the role of SOC in Cr 2p spin-flip excitations. Such precise measurements offer insights into the energy design of spintronic devices that utilize quantum state tuning and the effect of halides in determining spin-flip excitation energies in 2D magnets.

*This research was conducted at RIXS beamline 41A, Taiwan Photon Source, and PEAXIS, BESSY II, Germany. The preliminary measurements were taken at Advanced Light Source (ALS). We thank all the beamline scientists for their valuable support. This work is supported by the Welch Foundation (grant number: E-0001) and the Texas Center for Superconductivity. It is also funded by AFOSR and DOE. Special thanks to the eXn group at the University of Houston, Texas, USA.

Presenters

  • Chamini S Pathiraja

    • University of Houston

Authors

  • Chamini S Pathiraja

    • University of Houston
  • Yi-De Chuang

    • Advanced Light Source
  • Jayajeewana Niranjana Ranhili Pelige

    • University of Houston
  • Deniz Wong

    • Helmholtz-Zentrum Berlin f u¨ r Materialien und Energie
  • Christian Schulz

    • Helmholtz-Zentrum Berlin f u¨ r Materialien und Energie
  • Yu-Cheng Shao

    • National Synchrotron Radiation Research Center
  • Di-Jing Huang

    • Natl Synchrotron Rad Res Ctr
  • Hsiao-Yu Huang

    • Natl Synchrotron Rad Res Ctr
    • National Synchrotron Radiation Research Center, Hsinchu 300092, Taiwan
  • Amol Singh

    • Natl Synchrotron Rad Res Ctr
  • Byron Freelon

    • University of Houston