Appearance and disappearance of ferromagnetism in ultra-thin LaMnO on SrTiO substrate: a viewpoint from first-principles
arXiv:1711.11329 · doi:10.1103/PhysRevB.96.235112
Abstract
The intrinsic magnetic state (ferromagnetic or antiferromagnetic) of ultra-thin LaMnO films on the mostly used SrTiO substrate is a long-existing question under debate. Either strain effect or non-stoichiometry was argued to be responsible for the experimental ferromagnetism. In a recent experiment [Science \textbf{349}, 716 (2015)], one more mechanism, namely the self-doping due to polar discontinuity, was argued to be the driving force of ferromagnetism beyond the critical thickness. Here systematic first-principles calculations have been performed to check these mechanisms in ultra-thin LaMnO films as well as superlattices. Starting from the very precise descriptions of both LaMnO and SrTiO, it is found that the compressive strain is the dominant force for the appearance of ferromagnetism, while the open surface with oxygen vacancies leads to the suppression of ferromagnetism. Within LaMnO layers, the charge reconstructions involve many competitive factors and certainly go beyond the intuitive polar catastrophe model established for LaAlO/SrTiO heterostructures. Our study not only explains the long-term puzzle regarding the magnetism of ultra-thin LaMnO films, but also shed light on how to overcome the notorious magnetic dead layer in ultra-thin manganites.
10 pages, 8 figures
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- Light effect on the interface resistance of BaSrTiO/LaMnO heterosctructure