2014
DOI: 10.1016/j.ceramint.2013.12.118
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Photochemical synthesis of AZrO3−X thin films (A=Ba, Ca and Sr) and their characterization

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Cited by 24 publications
(13 citation statements)
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“…Thus, the new peak at 527.45 eV should be assigned to the O1s peak of Ca-O-Zr hetero-linkages, which would attribute to the base structure of CaZrO 3 . The results also well agree with some other works[35][36][37][38][39][40][41][42]. In addition, the XPS spectra of Ca2p and Zr3d also support the Ca-O-Zr hetero-linkage formation: Ca2p 1/2 shifted from 344.92 to 344.31 eV and that ofCa2p 3/2 from 348.55 to 348.03 eV, together with Zr3d 3/2 shifting from 182.26 to 181.81 eV and that of Zr3d 5/2 from 179.92 to 179.47 eV.…”
supporting
confidence: 93%
See 1 more Smart Citation
“…Thus, the new peak at 527.45 eV should be assigned to the O1s peak of Ca-O-Zr hetero-linkages, which would attribute to the base structure of CaZrO 3 . The results also well agree with some other works[35][36][37][38][39][40][41][42]. In addition, the XPS spectra of Ca2p and Zr3d also support the Ca-O-Zr hetero-linkage formation: Ca2p 1/2 shifted from 344.92 to 344.31 eV and that ofCa2p 3/2 from 348.55 to 348.03 eV, together with Zr3d 3/2 shifting from 182.26 to 181.81 eV and that of Zr3d 5/2 from 179.92 to 179.47 eV.…”
supporting
confidence: 93%
“…Furthermore, some groups also reported that they succeeded in preparing CaZrO 3 at high temperatures over 800 o C [37][38][39][40][41]. (Figure 7a).…”
Section: Catalytic Activity Of Zromentioning
confidence: 99%
“…On the other hand, the spin-orbit distance (3d5/2 -3d3/2 splitting) for CaZrO3 species is around 2,4 eV [33] . The comparison of XPS spectra for initial and final Ca-doped sample shows an increase of binding energy from 182,5 to 183.0 eV as well as an increase in 3d5/2 -3d3/2 splitting from 2,2 to 2,5 eV.…”
Section: Resultsmentioning
confidence: 95%
“…Additionally, the chemical analysis performed using XPS measurements indicates the presence of a Cu2O/CuO oxides mixture in the anodized surfaces [37,54]. The high resolution Cu2p spectrum (see Figure 2a) shows important contributions at a binding of 932.2 and 933.9 eV; these signals are attributed to Cu + Cu2O, CuO and [49], for the case of the Cu-Auger signal, the Cu + CuO and Cu2O contributions are identified at binding energy of 567.0 and 569.3 eV, respectively (see Figure 2b). Additionally, high resolution O1s spectrum (see Figure 2c) evidences the presence of both CuO and Cu2O oxides as well as hydrated species in the sample, which are in agreement with the above showed Raman results.…”
Section: Resultsmentioning
confidence: 98%
“…Raman experiments were performed ex situ (in air) using a Horiba LabRAM HR spectrometer (Sunnyvale, CA, USA), employing a He/Ne laser (632.8 nm wavelength). Using an XPS-Auger Perkin Elmer Model PHI 1257 spectrometer (Waltham, MA, USA) was employed to determine the chemical composition of samples, by means of HRXPS and using the method described previously [48][49][50]. For AFM measurements, a Nanonics Multi View MV1000 was employed using n-type silicon cantilevers (tip radius ≈ 20 nm; f = 39.4 kHz; Q = 1576) for the intermittent mode.…”
Section: Methodsmentioning
confidence: 99%