2018
DOI: 10.1007/s11664-018-6183-z
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A Hydrothermal Route to the Synthesis of CaTiO3 Nanocuboids Using P25 as the Titanium Source

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Cited by 68 publications
(21 citation statements)
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“…Nevertheless, most of the famous semiconductor photocatalysts (e.g. TiO 2 , ZnO, SrTiO 3 , CaTiO 3 , Bi 2 WO 6 , Bi 4 Ti 3 O 12 [6][7][8][9][10][11] ) possess a large bandgap E g > 3.0 eV and can only absorb ultraviolet (UV) light occupying only 4% of the incoming solar energy. Furthermore, the photogenerated electrons and holes in these semiconductor photocatalysts are easily recombined in pairs, thus limiting their photocatalytic activity.…”
Section: Introductionmentioning
confidence: 99%
“…Nevertheless, most of the famous semiconductor photocatalysts (e.g. TiO 2 , ZnO, SrTiO 3 , CaTiO 3 , Bi 2 WO 6 , Bi 4 Ti 3 O 12 [6][7][8][9][10][11] ) possess a large bandgap E g > 3.0 eV and can only absorb ultraviolet (UV) light occupying only 4% of the incoming solar energy. Furthermore, the photogenerated electrons and holes in these semiconductor photocatalysts are easily recombined in pairs, thus limiting their photocatalytic activity.…”
Section: Introductionmentioning
confidence: 99%
“…The existence of other oxidation states can be excluded since no additional binding energy peaks are detected on the Bi 4f and Ti 2p XPS spectra. On the O 1s XPS spectrum (Figure 8d), the binding energy at 529.7 eV is attributed to the crystal lattice oxygen of Bi 4 Ti 3 O 12 , whereas the binding energy at 531.5 eV could arise from chemisorbed oxygen species [58,59]. The C 1s XPS spectrum (Figure 8e) presents two peaks at 284.8 and 287.7 eV.…”
Section: Resultsmentioning
confidence: 99%
“…The C 1s XPS spectrum (Figure 8e) presents two peaks at 284.8 and 287.7 eV. The peak at 284.8 eV arises from the C–C sp 2 -hybridized carbon of CQDs and adventitious carbon that is used to calibrate the binding energy scale [59,60]. The peak at 287.7 eV is attributed to the presence of C–O–C or C=O [60].…”
Section: Resultsmentioning
confidence: 99%
“…4c. The absorption edge can be determined from the peak wavelength in the derivative spectra [53]. It can be seen that the light absorption edge of bare Ag 3 PO 4 is located at ~ 527 nm, corresponding to the bandgap energy ( E g ) of ~ 2.35 eV.…”
Section: Resultsmentioning
confidence: 99%