Strain effect on magnetic-exchange-induced phonon splitting in NiO films

NiO thin films with various strains were grown on SrTiO3 (STO) and MgO substrates using a pulsed laser deposition technique. The films were characterized using an x-ray diffraction, atomic force microscopy, and infrared reflectance spectroscopy. The films grown on STO (001) substrate show a compress...

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Veröffentlicht in:Journal of physics. Condensed matter 2020-09, Vol.32 (40), p.405607
Hauptverfasser: Kashir, Alireza, Goian, Veronica, Yoon, Daseob, Cho, Byeong-Gwan, Jeong, Yoon Hee, Lee, Gil-Ho, Kamba, Stanislav
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Sprache:eng
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Zusammenfassung:NiO thin films with various strains were grown on SrTiO3 (STO) and MgO substrates using a pulsed laser deposition technique. The films were characterized using an x-ray diffraction, atomic force microscopy, and infrared reflectance spectroscopy. The films grown on STO (001) substrate show a compressive in-plane strain which increases as the film thickness is reduced resulting in an increase of the NiO phonon frequency. On the other hand, a tensile strain was detected in the NiO film grown on MgO (001) substrate which induces a softening of the phonon frequency. Overall, the variation of in-plane strain from −0.36% (compressive) to 0.48% (tensile) yields the decrease of the phonon frequency from 409.6 cm−1 to 377.5 cm−1 which occurs due to the ∼1% change of interatomic distances. The magnetic exchange-driven phonon splitting Δω in three different samples, with relaxed (i.e. zero) strain, 0.36% compressive strain and 0.48% tensile strain, was measured as a function of temperature. The Δω increases on cooling in NiO relaxed film as in the previously published work on a bulk crystal. The splitting increases on cooling also in 0.48% tensile strained film, but Δω is systematically 3-4 cm−1 smaller than in relaxed film. Since the phonon splitting is proportional to the non-dominant magnetic exchange interaction J1, the reduction of phonon splitting in tensile-strained film was explained by a diminishing of J1 with lattice expansion. Increase of Δω on cooling can be also explained by rising of J1 with reduced temperature.
ISSN:0953-8984
1361-648X
DOI:10.1088/1361-648X/ab9f08