Spin dynamics via a time-dependent adiabatic GW method with spin-dependent interactions
ORAL
Abstract
We present a methodology for GW plus Bethe-Salpeter Equation (GW-BSE) calculations with the included effects of spin-dependent interactions. Using the spin-dependent Hedin equations [1], we are able to include the relativistic spin-spin and spin-orbit interactions of the Pauli-Breit Hamiltonian alongside the bare Coulomb interaction in calculating the dielectric matrix, self-energies, and BSE kernel matrix elements. With spin-dependent interactions included in the BSE kernel, we simulate spin dynamics after laser excitation within a time-dependent adiabatic GW (TD-aGW) method based on the real-time propagation of the interacting density matrix [2]. We discuss an application to the all-optical magnetization reversal by circularly polarized pulses in monolayer CrI3. In this phenomenon, the light pulse populates a bright exciton state with a large orbital moment, which couples to the lattice spins through spin-orbit coupling. Further applications in magnetic systems will be discussed.
[1] Aryasetiawan, F., & Biermann, S. (2009). J. Phys. Condens. Matter, 21(6), 064232.
[2] Chan, Y. H., Qiu, D. Y., da Jornada, F. H., & Louie, S. G. (2021). Proc. Natl. Acad. Sci. U.S.A., 118(25), e1906938118.
[1] Aryasetiawan, F., & Biermann, S. (2009). J. Phys. Condens. Matter, 21(6), 064232.
[2] Chan, Y. H., Qiu, D. Y., da Jornada, F. H., & Louie, S. G. (2021). Proc. Natl. Acad. Sci. U.S.A., 118(25), e1906938118.
*This work was supported by the National Science Foundation and the U.S. Department of Energy.
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Presenters
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Jack McArthur
- University of California, Berkeley