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arxiv: 1308.5616 · v2 · pith:L2LKIQ4Ynew · submitted 2013-08-26 · ❄️ cond-mat.supr-con · cond-mat.mtrl-sci

Raman spectroscopy study of the interface structure in (CaCuO2)n/(SrTiO3)m superlattices

classification ❄️ cond-mat.supr-con cond-mat.mtrl-sci
keywords interfacesuperlatticescacuo2ramansrtio3structureatmospherecm-1
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Raman spectra of CaCuO2/SrTiO3 superlattices show clear spectroscopic marker of two structures formed in CaCuO2 at the interface with SrTiO3. For non-superconducting superlattices, grown in low oxidizing atmosphere, the 425 cm-1 frequency of oxygen vibration in CuO2 planes is the same as for CCO films with infinite layer structure (planar Cu-O coordination). For superconducting superlattices grown in highly oxidizing atmosphere, a 60 cm-1 frequency shift to lower energy occurs. This is ascribed to a change from planar to pyramidal Cu-O coordination because of oxygen incorporation at the interface. Raman spectroscopy proves to be a powerful tool for interface structure investigation.

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