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Enhanced Néel-Type Skyrmion Stability in Polar VOSe<sub>2</sub>O<sub>5</sub> through Tunable Magnetic Anisotropy under Pressure

ORAL

Abstract

Polar VOSe2O5, with P4cc space group (C4V symmetry), was recently identified as hosting a rare Néel-type skyrmion phase within a very narrow range of temperature and magnetic field. Motivated by this discovery, we investigated the effect of pressure on its magnetic properties, focusing on improving the stability of the skyrmion phase. At ambient pressure, two magnetic transitions were observed at TC1 ~ 7.4 K and TC2 ~ 4.0 K. Notably, the contrasting behavior of these transitions under applied magnetic fields—TC1 increases while TC2 is suppressed—reflects the magnetic anisotropy in VOSe2O5. Neutron diffraction refinements reveal a three-up-one-down spin configuration, with alignment switching from the c-axis at 6.0 K to the b-axis at 1.8 K, further demonstrating the anisotropic nature. Pressure-dependent AC susceptibility measurements show TC1 increasing by 0.043(3) K/kbar and TC2 decreasing by -0.052(4) K/bar, indicating pressure-tunable anisotropy. The field-temperature (H-T) phase diagrams confirm the significant stabilization of the Néel-type skyrmion phase under 14.21 kbar of pressure, with its area expanding approximately threefold. These findings underscore the role of pressure in promoting Néel-type skyrmion stability through modulation of magnetic anisotropy, offering valuable insights into controllable topological phases for spintronics and related technological applications.

Presenters

  • Ting-Wei Kuo

    University of Houston, Texas Center for Superconductivity

Authors

  • Ting-Wei Kuo

    University of Houston, Texas Center for Superconductivity

  • Liangzi Deng

    University of Houston

  • Ching-Wu Chu

    TCSUH and Department of Physics, University of Houston; Lawrence Berkeley National Laboratory; Hong Kong University of Science and Technology, University of Houston

  • Melissa J Gooch

    University of Houston

  • Hung-Duen Yang

    National Sun Yat-sen University

  • Hung-Cheng Wu

    Department of Physics, National Sun Yat-sen University