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Uniaxial pressure effects in the two-dimensional van der Waals ferromagnet CrI3
Heidelberg Univ, Kirchhoff Inst Phys, INF 227, D-69120 Heidelberg, Germany..
Heidelberg Univ, Kirchhoff Inst Phys, INF 227, D-69120 Heidelberg, Germany..
Heidelberg Univ, Kirchhoff Inst Phys, INF 227, D-69120 Heidelberg, Germany..
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Condensed Matter Physics of Energy Materials. Natl Univ Sci & Technol MISiS, Moscow 119049, Russia..ORCID iD: 0000-0002-1802-5279
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2022 (English)In: Physical Review B, ISSN 2469-9950, E-ISSN 2469-9969, Vol. 105, no 6, article id L060404Article in journal (Refereed) Published
Abstract [en]

Magnetoelastic coupling and uniaxial pressure dependencies of the ferromagnetic ordering temperature in the quasi-two-dimensional layered van der Waals material CrI3 are experimentally studied and quantified by high-resolution dilatometry. Clear anomalies in the thermal expansion coefficients at T-C imply positive (negative) pressure dependencies partial derivative T-C/partial derivative p(i) for pressure applied along (perpendicular to) the c axis. The experimental results are backed up by numerical studies showing that the dominant, intralayer magnetic coupling increases upon compression along the c direction and decreases with negative in-plane strain. In contrast, interlayer exchange is shown to initially increase and subsequently decrease upon the application of both out-of-plane and in-plane compression.

Place, publisher, year, edition, pages
American Physical Society (APS) American Physical Society, 2022. Vol. 105, no 6, article id L060404
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Condensed Matter Physics
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URN: urn:nbn:se:uu:diva-470221DOI: 10.1103/PhysRevB.105.L060404ISI: 000761174600006OAI: oai:DiVA.org:uu-470221DiVA, id: diva2:1646389
Funder
Swedish Research Council, 2018-05393Swedish Research Council, 2019-03569Available from: 2022-03-22 Created: 2022-03-22 Last updated: 2024-01-15Bibliographically approved

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Abdel-Hafiez, MahmoudKvashnin, Yaroslav

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