Implication of ferroelectric during the growth of superlattices and heterostructures
ORAL
Abstract
In ferroelectric superlattices the materials are often under considerable epitaxial strain, raising their ferroelectric transition temperature to be comparable to the growth temperature. This has important consequences for the growth of superlattices and their eventual properties. For example, the as-grown polarization domain structure in PbTiO$_{\mathrm{3}}$/BaTiO$_{\mathrm{3}}$ (PTO/BTO) superlattices is markedly different depending on if the overall structure's transition temperature lies below, above, or oscillates around the growth temperature. More surprisingly, we found that the ferroelectric polarization of a growing structure has a strong effect on the characteristics of films grown on it. We have studied this effect by focusing on the properties of BTO thin films grown on very thin layers of PTO using a combination of XRD, vertical and lateral PFM and electrical characterization. It reveals that the ferroelectricity of PTO can induce lateral polarization domain structures in BTO grown on it. Further insight into these effects is obtained by XRD performed in-situ during the growth process at the NSLS-II ISR beamline. The results show the ferroelectricity of PTO layers can effects BTO films' growth mode and help them stay in strained ferroelectric state.
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Authors
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Rui Liu
Department of Physics and Astronomy, Stony Brook University
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Alec Sun
Department of Physics and Astronomy, Stony Brook University
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Charles Pan
Department of Physics and Astronomy, Stony Brook University
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Kaize Cheng
Department of Physics and Astronomy, Stony Brook University
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Eli Doyle
Department of Physics and Astronomy, Stony Brook University
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Hsiang-Chun Hsing
Department of Physics and Astronomy, Stony Brook University
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Anna Gura
Department of Physics and Astronomy, Stony Brook University
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Giulia Bertino
Department of Physics and Astronomy, Stony Brook University
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Jin-Wen Lai
Department of Physics and Astronomy, Stony Brook University
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Matthew Dawber
Department of Physics and Astronomy, Stony Brook University