Stability of biskyrmions in centrosymmetric magnetic films

ORAL

Abstract

In [1], we investigate analytically and numerically the stability of biskyrmions in films of finite thickness, taking into account the nearest-neighbor exchange interaction, perpendicular magnetic anisotropy (PMA), dipole-dipole interaction (DDI), and the discreteness of the atomic lattice. The biskyrmion is characterized by the topological charge Q=2, the spatial scale λ, and another independent length d that can be interpreted as a separation of two Q=1 skyrmions inside a Q=2 topological defect in the background of uniform magnetization. We find that biskyrmions with d of order λ can be stabilized by the magnetic field within a certain range of the ratio of PMA to DDI in a film having a sufficient number of atomic layers Nz. The shape of biskyrmions has been obtained by the numerical minimization of the energy of interacting spins in a 1000×1000×Nz atomic lattice. It is close to the exact solution of the Belavin-Polyakov model when d is below the width of the ferromagnetic domain wall. We compute the magnetic moment of a biskyrmion and discuss ways of creating biskyrmions in experiment.

[1]D. Capic, D. Garanin and E.M. Chudnovsky, Stability of biskyrmions in centrosymmetric magnetic films, Phys. Rev. B 100, 014432 (2019).

*Grant No. OSR2016-CRG5-2977 from KAUST

Presenters

  • Daniel Capic

    • CUNY-Lehman Coll

Authors

  • Daniel Capic

    • CUNY-Lehman Coll
  • Dmitry Garanin

    • CUNY-Lehman Coll
    • Physics, Herbert H. Lehman College
  • Eugene M Chudnovsky

    • Physics Department, Lehman College and Graduate School
    • CUNY-Lehman Coll
    • Physics, Herbert H. Lehman College