Effects of pressure on the electronic and magnetic properties of bulk NiI2

  • Jesse Kapeghian
  • , Danila Amoroso
  • , Connor A. Occhialini
  • , Luiz G.P. Martins
  • , Qian Song
  • , Jesse S. Smith
  • , Joshua J. Sanchez
  • , Jing Kong
  • , Riccardo Comin
  • , Paolo Barone
  • , Bertrand Dupé
  • , Matthieu J. Verstraete
  • , Antia S. Botana

Research output: Contribution to journalArticleAcademicpeer-review

Abstract

Transition metal dihalides have recently garnered interest in the context of two-dimensional van der Waals magnets as their underlying geometrically frustrated triangular lattice leads to interesting competing exchange interactions. In particular, NiI2 is a magnetic semiconductor that has been long known for its exotic helimagnetism in the bulk. Recent experiments have shown that the helimagnetic state survives down to the monolayer limit with a layer-dependent magnetic transition temperature that suggests a relevant role of the interlayer coupling. Here, we explore the effects of hydrostatic pressure as a means to enhance this interlayer exchange and ultimately tune the electronic and magnetic response of NiI2. We study first the evolution of the structural parameters as a function of external pressure using first-principles calculations combined with x-ray diffraction measurements. We then examine the evolution of the electronic structure and magnetic exchange interactions via first-principles calculations and Monte Carlo simulations. We find that the leading interlayer coupling is an antiferromagnetic second-nearest-neighbor interaction that increases monotonically with pressure. The ratio between isotropic third- and first-nearest-neighbor intralayer exchanges, which controls the magnetic frustration and determines the magnetic propagation vector q of the helimagnetic ground state, is also enhanced by pressure. As a consequence, our Monte Carlo simulations show a monotonic increase in the magnetic transition temperature, indicating that pressure is an effective means to tune the magnetic response of NiI2.

Original languageEnglish
Article number014403
JournalPhysical Review B
Volume109
Issue number1
DOIs
Publication statusPublished - 3 Jan 2024

Bibliographical note

Publisher Copyright:
© 2024 American Physical Society.

Funding

We thank S. Picozzi for useful discussions during the early stages of this work. J.K. acknowledges support from NSF Grant No. DMR 2206987. A.S.B. was supported by the Alfred P. Sloan Foundation FG-2022-19086. We thank the ASU Research Computing Center for high-performance computing resources. D.A., B.D., and M.J.V. acknowledge the SWIPE project funded by FNRS Belgium Grant No. PINT-MULTIR.8013.20. M.J.V. acknowledges ARC project DREAMS (G.A. 21/25-11) funded by Federation Wallonie Bruxelles and ULiege. P.B. acknowledges financial support from the Italian MIUR through Project No. PRIN 2017Z8TS5B. C.A.O., L.G.P.M., Q.S., and R.C. acknowledge support from the US Department of Energy, BES under Award No. DE-SC0019126 (materials synthesis and characterization and x-ray diffraction measurements).

FundersFunder number
National Science FoundationDMR 2206987
U.S. Department of Energy
Alfred P. Sloan FoundationFG-2022-19086
Basic Energy SciencesDE-SC0019126
Automotive Research Center
Fonds De La Recherche Scientifique - FNRSPINT-MULTIR.8013.20
Fédération Wallonie-Bruxelles
Ministero dell’Istruzione, dell’Università e della RicercaPRIN 2017Z8TS5B

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