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.
DI CASTRO, D., Caramazza, S., Innocenti, D., Balestrino, G., Marini, C., Dore, P., et al. (2013). Raman spectroscopy study of the interface structure in (CaCuO2)n/(SrTiO3)m superlattices. APPLIED PHYSICS LETTERS, 103(19) [10.1063/1.4828358].
Raman spectroscopy study of the interface structure in (CaCuO2)n/(SrTiO3)m superlattices
DI CASTRO, DANIELE;BALESTRINO, GIUSEPPE;
2013-11-01
Abstract
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.File | Dimensione | Formato | |
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