April 22 - 26, 2024
Seattle, Washington
May 7 - 9, 2024 (Virtual)

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2024 MRS Spring Meeting
SF01.09.02

Growth and Characterization of High Entropy Perovskite (La0.2Nd0.2Gd0.2Sm0.2Y0.2)MnO3 Thin Films on Cubic and Orthorhombic Substrates

When and Where

Apr 25, 2024
9:00am - 9:15am
Terrace Suite 1, Level 4, Summit

Presenter(s)

Co-Author(s)

Maximilian Mihm1,Aladin Ullrich1,David Stein1,Christian Holzmann1,Helmut Karl1,Manfred Albrecht1

Institute of Physics, University of Augsburg1

Abstract

Maximilian Mihm1,Aladin Ullrich1,David Stein1,Christian Holzmann1,Helmut Karl1,Manfred Albrecht1

Institute of Physics, University of Augsburg1
With the discovery of high entropy oxides in 2015 many different oxides have been synthesized using the high entropy strategy [1]. Since 2018 many different high entropy perovskites have been synthesized, some of them contain five elements on the A- or the B-site [2]. Some high entropy perovskites were synthesized with ten different elements, five on the A-site and five on the B-site [2]. Most of them were produced as polycrystalline powders, only a few oft them have been grown as thin film [2-5]. In the recent research, the focus has shifted to high entropy manganites-perovskites, because of their interesting magnetic properties, where the Mn-O-Mn exchange dominates the magnetic properties and the rare earth ion radii influences the strength of the exchange [3,4]. One high entropy manganite-perovskite is (La<sub>0.2</sub>Nd<sub>0.2</sub>Gd<sub>0.2</sub>Sm<sub>0.2</sub>Y<sub>0.2</sub>)MnO<sub>3 </sub>which was previously produced as a powder [2].<br/>We have grown thin films of (La<sub>0.2</sub>Nd<sub>0.2</sub>Gd<sub>0.2</sub>Sm<sub>0.2</sub>Y<sub>0.2</sub>)MnO<sub>3</sub> via pulsed laser deposition on three different substrates, one with a cubic structure SrTiO<sub>3 </sub>(001) and two with an orthorhombic structure, NdGaO<sub>3 </sub>(001), and YAlO<sub>3 </sub>(001). All films were subsequently annealed. X-ray diffraction data confirmed epitaxial growth of (La<sub>0.2</sub>Nd<sub>0.2</sub>Gd<sub>0.2</sub>Sm<sub>0.2</sub>Y<sub>0.2</sub>)MnO<sub>3 </sub>on all substrates. Wide-range reciprocal space mapping and electron-backscattered diffraction revealed, that (La<sub>0.2</sub>Nd<sub>0.2</sub>Gd<sub>0.2</sub>Sm<sub>0.2</sub>Y<sub>0.2</sub>)MnO<sub>3</sub> has three different crystal orientations on SrTiO<sub>3</sub> and two on NdGaO<sub>3</sub> and YAlO<sub>3</sub>. On SrTiO<sub>3</sub> (La<sub>0.2</sub>Nd<sub>0.2</sub>Gd<sub>0.2</sub>Sm<sub>0.2</sub>Y<sub>0.2</sub>)MnO<sub>3 </sub>grows in two different directions (001) and (110). The (001) orientated crystals are rotated by 45° with respect to the substrate, while the (110) crystals are aligned either to the substrate lattice or are also rotated by 45°. On NdGaO<sub>3</sub> we observed only (001) orientated crystals, but with two different in-plane orientations, either (001) or (110). On YAlO<sub>3</sub> two crystal orientations were observed (110) and (001), both are aligned to the substrate lattice. High-resolution transmission electron microscopy confirmed the perovskite structure and the epitaxial growth. All surfaces showed a grainy structure which was observed by atomic force microscopy. Zero-field-cooled and field-cooled measurements revealed a magnetic transition temperature around 38 K for (La<sub>0.2</sub>Nd<sub>0.2</sub>Gd<sub>0.2</sub>Sm<sub>0.2</sub>Y<sub>0.2</sub>)MnO<sub>3</sub> grown on SrTiO<sub>3</sub>, which is lower compared to most of the parent compounds. This is in good agreement with the magnetic measurements on corresponding powder. Below 25 K the rare earth elements couple antiferromagnetic to the manganese, which is indicated by a decrease of the magnetization in the field-cooled curve. All samples showed a small coercive field and a small remanent magnetization, which indicates a soft magnetic behaviour.<br/>[1] C. M. Rost, E. Sachet, T. Borman, A. Moballegh, E. C. Dickey, D. Hou, J. L. Jones, S. Curtarolo, and J.-P. Maria, Nature Communications <b>6</b>, 8485 (2015).<br/>[2] A. Sarkar, R. Djenadic, D. Wang, C. Hein, R. Kautenburger, O. Clemens, and H. Hahn, Journal of the European Ceramic Society <b>38</b>, 2318 (2018).<br/>[3] R. Das, S. Pal, S. Bhattacharya, S. Chowdhury, S. K. K., M. Vasundhara, A. Gayen, and M. M. Seikh, Physical Review Materials <b>7</b>, 024411 (2023).<br/>[4] A. Sarkar, R. Djenadic, D. Wang, C. Hein, R. Kautenburger, O. Clemens, and H. Hahn, Journal of the European Ceramic Society <b>38</b>, 2318 (2018).<br/>[5] A. R. Mazza, E. Skoropata, J. Lapano, J. Zhang, Y. Sharma, B. L. Musico, V. Keppens, Z. Gai, M. J. Brahlek, A. Moreo, D. A. Gilbert, E. Dagotto, and T. Z. Ward, Physical Review B <b>104</b>, 094204 (2021).

Keywords

magnetic properties | perovskites | thin film

Symposium Organizers

Ben Breitung, Karlsruhe Institute of Technology
Alannah Hallas, The University of British Columbia
Scott McCormack, University of California, Davis
T. Zac Ward, Oak Ridge National Laboratory

Session Chairs

Alan Farhan
T. Zac Ward

In this Session