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    Interfacial reconstruction effects in insulating double perovskite Nd2NiMnO6/SrTiO3 and Nd2NiMnO6/NdGaO3 thin films

    Nandana Bhattacharya1,*, Ranjan Kumar Patel1,†, Siddharth Kumar1,†, Prithwijit Mandal1, Jyotirmay Maity1, Christoph Klewe2, Zhan Zhang3, Hua Zhou3,‡, and Srimanta Middey1,§

    • *Contact author: nandanab@iisc.ac.in
    • †Currently at Department of Electrical and Computer Engineering, Rutgers University, Piscataway, NJ 08854, USA.
    • ‡Contact author: hzhou@anl.gov
    • §Contact author: smiddey@iisc.ac.in

    Phys. Rev. B 111, 235438 – Published 20 June, 2025

    DOI: https://doi.org/10.1103/1qzc-j65h

    Abstract

    Ferromagnetic insulating (FMI) double perovskite oxides (DPOs) A2BB′O6 with near-room-temperature Curie temperatures are promising candidates for ambient-temperature spintronics applications. To realize their potential, epitaxial stabilization of DPO films and understanding the effect of multiple broken symmetries across the film/substrate interface are crucial. This study investigates ultrathin films of the FMI Nd2NiMnO6 grown on SrTiO3 (STO) and NdGaO3 (NGO) substrates. By comparing growth on these substrates, we examine the influence of polarity and structural symmetry mismatches, which are absent in the NGO system. The interface exhibits immeasurable resistance in both cases. Using synchrotron x-ray diffraction, we show that films have three octahedral rotational domains because of the structural symmetry mismatch with the STO substrate. Furthermore, our coherent Bragg rod analysis of specular x-ray diffraction reveals a significant modification of the out-of-plane lattice parameter within a few unit cells at the film/substrate interface and the surface. This arises from polarity compensation and surface symmetry breaking, respectively. These structural alterations influence the Mn orbital symmetry, a dependence that we further confirm through x-ray linear dichroism measurements. Since the ferromagnetism in insulating DPOs is mediated by orbital-dependent superexchange interactions [Phys. Rev. Lett. 100, 186402 (2008)], our study provides a framework for understanding the evolution of magnetism in ultrathin geometry.

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