Increased Curie temperature and enhanced perpendicular magneto anisotropy of Cr<sub>2</sub>Ge<sub>2</sub>Te<sub>6</sub>/NiO heterostructure
ORAL
Abstract
Van der Waals (vdW) materials with ferromagnetic properties down to few layers such as CrI3 and Cr2Ge2Te6 have recently attracted a lot of attention due to their potential in spintronic applications. However, the Curie temperature (TC) of these vdW has remained relatively low. Here, we report increased TC and enhanced perpendicular magnetic anisotropy in Cr2Ge2Te6 (CGT) flakes interfaced with antiferromagnetic insulator NiO for a wide range of CGT thicknesses (5-200 nm).
Measurements of the same flake by polar magneto optic Kerr effect (MOKE) microscopy before and after coating NiO reveal a hysteresis loop with a square shape and larger coercive field for the CGT/NiO heterostructure. Furthermore, the maximum TC observed for CGT/NiO reached ~120K, almost double the TC of CGT alone (~60K). These observations suggest that interfacing van der Waals ferromagnets with other materials could provide a venue to engineer their magnetic properties. [1]
[1] H. Idzuchi, A. E. Llacsahuanga Allcca, X. C. Pan, K. Tanigaki and Y. P. Chen (2019), Increased Curie temperature and enhanced perpendicular magneto anisotropy of Cr2Ge2Te6/NiO heterostructure. Manuscript submitted for publication.
Measurements of the same flake by polar magneto optic Kerr effect (MOKE) microscopy before and after coating NiO reveal a hysteresis loop with a square shape and larger coercive field for the CGT/NiO heterostructure. Furthermore, the maximum TC observed for CGT/NiO reached ~120K, almost double the TC of CGT alone (~60K). These observations suggest that interfacing van der Waals ferromagnets with other materials could provide a venue to engineer their magnetic properties. [1]
[1] H. Idzuchi, A. E. Llacsahuanga Allcca, X. C. Pan, K. Tanigaki and Y. P. Chen (2019), Increased Curie temperature and enhanced perpendicular magneto anisotropy of Cr2Ge2Te6/NiO heterostructure. Manuscript submitted for publication.
*We acknowledge partial support of the work by NSF, Sumimoto Foundation, WPI-AIMR, and JSPS.
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Presenters
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Andres Llacsahuanga Allcca
- Physics and Astronomy, Purdue University