Proximity-Induced Magnetic Phases in CrI3 Monolayers Coupled to WTe2

Eötvös Loránd University
Centre For Energy Research

Zoltán Tajkov









The Team



- László Oroszlány, Zoltán Tajkov, János Koltai, Dániel Pozsár, Andor Kormányos, András Balogh, Tamás Véber, Marcell Sipos
- Jaime Ferrer, Amador Garcia Fuente, Gabriel Martinez-Carracedo, Aurelio Hierro Rodriguez, Balázs Nagyfalusi, Rosa Eulalia González Ferreras
- Felix Büttner, Kai Litzius, Steffen Wittrock
- Efren Navarro-Moratalla, Marta Galbiati, Jose Joaquin Perez Grau
- László Szunyogh, László Udvardi, Bendegúz Nyári, Anjali Jyothi Bhasu



























Heisenberg model and DFT perturbation theory

DFT through
RKKR
&

Liechtenstein, Katsnelson , Antropov, Gubanov
J. Magn. Magn. Mater. 67 65 (1987)
Oroszlány, Ferrer, Deák, Udvardi, Szunyogh
Phys. Rev. B 99, 224412 (2019)
What is \(\delta \hat{V}_i\) ?
1) We need to rotate the magnetic moment!

2) We need to identify the magnetic entity!
Could be:
- Single atom
- Cluster of atoms
- Certain orbitals inside an atom
Relativistic magnetic model parameters
Udvardi, Szunyogh, Palotás, Weinberger
Phys. Rev. B 68, 104436 (2003)
Martínez-Carracedo, Oroszlány, García-Fuente, Nyári, Udvardi, Szunyogh, Ferrer
Phys. Rev. B 108, 214418 (2023)
Istropic
exchange
Symmetric traceless exchange
Dzyaloshinskii - Moriya vector
On-site
anisotropy

Grogu
State of GROGU
Udvardi, Szunyogh, Palotás, Weinberger
Phys. Rev. B 68, 104436 (2003)
Martínez-Carracedo, Oroszlány, García-Fuente, Nyári, Udvardi, Szunyogh, Ferrer
Phys. Rev. B 108, 214418 (2023)

Grogu
- Full SIESTA support
- GPU support
- Relativstic parameters
- Flexible API to set up more complicated systems with complex magnetic entities
- Command line interface to extract and visualize the magnetic parameters
- Multiple output formats for atomistic spin dynamics softwares
Coming soon:
- Wannier90 support
- OpenMX support
- Higher order interaction


Showcase: CrI3 monolayer
Cr
I
- Semiconductor
- Experimental \( T_C \) is around 45 K
- Superexchange
- Hubbard-U, U=3eV needed!




Showcase: CrI3 monolayer


d=1.62 \( \AA \)
Unit cell length: 7.13 \( \AA \)
Exchange parameters [meV]:
Calculated \( T_C \) is around 23 K
VAMPIRE 7





-1.14
-0.93
-0.02
0.15

D. Wang, Journal of Physical Chemistry C 125, 18467, 2021
Showcase: CrI3 monolayer + WTe2


Exchange parameters [meV]:
Cr
I

W
Te

d \( = 1.64 \AA \)
Unit cell length: 7.13 \( \AA \)
d\(_\mathrm{vdW} = 4.28 \AA\)
Small, > 0.15% strain
-1.14
-1.16
-0.93
-1.03
-0.02
-0.05
0.15
0.38
Pure CrI3
With WTe2
Showcase: CrI3 monolayer + WTe2





Exchange parameters [meV]:
-1.14
-1.16
-0.93
-1.03
-0.02
-0.05
0.15
0.38
- Tc for pure CrI3: 23 K Pure CrI3
- Tc for CrI3+WTe2: 32 K With WTe2
VAMPIRE 7

40% increase
Pure CrI3
With WTe2
Showcase: CrI3 monolayer + WTe2





Modest external electric field boosts Tc up to 33%
VAMPIRE 7



Relativistic magnetic interactions
- https://github.com/danielpozsar/grogu
- Single DFT calculation
- Pair creation is extremely cheap
- parallel BZ integral with MPI or CUDA
- Generalised Heisenberg model

UNDER 1 Hour on 8 GPUs



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