Interaction between topological defects in Cu2OSeO3: skyrmion lattice annihilation by 3D point defects
ORAL
Abstract
Its phase diagram shows a variety of noncollinear spin states. At low magnetic fields, the ground state is an incommensurate helical spiral with a long period of about 60nm. The magnetic field-temperature phase diagram was similar to those reported for the metallic alloys that show skyrmions. Moreover, the system can become polar when the hexagonal skyrmion lattice is formed in Cu2OSeO3 with a small applied magnetic field [3].
Our previous study [4] with the effective Hamiltonian scheme has reproduced the magnetic field-temperature phase diagram. We use the same approach to reveal the hidden connection between various topological defects (3D point defects and skyrmions) in Cu2OSeO3. We show (i) that Cu2OSeO3 hosts different topological defects with a non-zero local topological charge at different regions of the phase diagram (H, T). (ii) Point defects exerting external pressure on skyrmions, leading to their gradual annihilation as temperature increases. (iii) The annihilation of skyrmions is done by the melting of the lattice into a glassy-like state of spins that connects with the paramagnetic phase [5].
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Publication: [1]. Seki S, Yu X Z, Ishiwata S and Tokura Y (2012) - Observation of Skyrmions in a Multiferroic Material - Science(80),336,198–201
[2] Chacon A, Heinen L, Halder M, Bauer A, Simeth W, Mühlbauer S, Berger H, Garst M, Rosch A and Pfleiderer C (2018) -Observation of two independent skyrmion phases in a chiral magnetic material - Nat. Phys. 14,936–41
[3]. Seki S, Ishiwata S and Tokura Y (2012) - Magnetoelectric nature of skyrmions in a chiral magnetic insulator Cu2OSeO3 - Phys. Rev. B 86, 060403(R)
[4] Sabri H, Kornev I (2023) - Monte Carlo studies of noncollinear magnetic phases in multiferroic Cu2OSeO3 - Phys. Rev. B 107, 0244
[5] Sabri H, Kornev I (2023) - -Skyrmion lattice annihilation by point defects in the multiferroic Cu2OSeO3 (accepted in Phys. Rev. B 09/19/2023)
Presenters
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Houssam SABRI
Department of Physics and Astronomy, University of New Hampshire, Durham, New Hampshire 03824, USA
Authors
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Houssam SABRI
Department of Physics and Astronomy, University of New Hampshire, Durham, New Hampshire 03824, USA
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Igor Kornev
Université Paris-Saclay, CentraleSupélec, CNRS, Laboratoire SPMS UMR 8580, 91190, Gif-sur-Yvette, France.