“…By combining theory and experiment (see Figure ), the Raman feature at 945 cm –1 can be assigned to an interphase Ti–O–Si vibration and the feature at 1085 cm –1 to either an in-phase or out-of-phase Ti–O–Si vibration. As pointed out previously, it is not possible to discriminate between the in-phase and out-of-phase Ti–O–Si modes due to their spectral proximity. Just like the 1085 cm –1 feature, we attribute the 1150 cm –1 feature to a Ti–O–Si mode.…”
Section: Discussionmentioning
confidence: 96%
“…Article vibration. As pointed out previously, 59 it is not possible to discriminate between the in-phase and out-of-phase Ti−O−Si modes due to their spectral proximity. Just like the 1085 cm −1 feature, we attribute the 1150 cm −1 feature to a Ti−O−Si mode.…”
Dispersed
vanadia and titania are of great interest due to their
(photo)catalytic properties. The structure of isolated (highly dispersed)
vanadia and titania has been studied using a combination of deep UV
Raman, UV–vis, and IR spectroscopy. Highly dispersed vanadia
and titania were prepared by incipient wetness impregnation of the
corresponding isopropoxide precursors onto silica SBA-15. Using resonance
Raman spectroscopy, a wide range of vanadium (0.00001–0.7 V/nm2) and titanium (0.001–0.7 Ti/nm2) loadings
can be analyzed. At very low loadings (<0.05 M/nm2)
the structure of both highly dispersed vanadia and titania is characterized
by tetrahedral coordination of the central atom and anchoring to the
support by one or more M–O–S linkages. At higher loadings,
titania partly forms oligomeric surface structures according to UV–vis
results. In the case of highly dispersed vanadia samples (<0.1
V/nm2), Raman spectroscopy reveals distinct differences
in the vanadia surface structures under ambient and dehydrated conditions.
Corresponding UV–vis spectra indicate the formation of isolated
and oligomeric vanadia surface structures. A smaller dependence of
the titania surface structure on the environmental conditions (ambient/dehydrated)
was observed. For the 0.7 M/nm2 samples, the presence of
hydroxylated vanadia and titania structures in the dehydrated state
was verified by IR spectroscopy. The assignment of the vibrational
bands was facilitated by the results of a normal-mode analysis using
models based on polyhedral oligomeric silsesquioxane (POSS). Our study
clearly demonstrates the potential of resonance Raman spectroscopy
using 217.5 nm deep UV excitation to study the surface structure of
transition metal oxide species even in isolated conditions.
“…By combining theory and experiment (see Figure ), the Raman feature at 945 cm –1 can be assigned to an interphase Ti–O–Si vibration and the feature at 1085 cm –1 to either an in-phase or out-of-phase Ti–O–Si vibration. As pointed out previously, it is not possible to discriminate between the in-phase and out-of-phase Ti–O–Si modes due to their spectral proximity. Just like the 1085 cm –1 feature, we attribute the 1150 cm –1 feature to a Ti–O–Si mode.…”
Section: Discussionmentioning
confidence: 96%
“…Article vibration. As pointed out previously, 59 it is not possible to discriminate between the in-phase and out-of-phase Ti−O−Si modes due to their spectral proximity. Just like the 1085 cm −1 feature, we attribute the 1150 cm −1 feature to a Ti−O−Si mode.…”
Dispersed
vanadia and titania are of great interest due to their
(photo)catalytic properties. The structure of isolated (highly dispersed)
vanadia and titania has been studied using a combination of deep UV
Raman, UV–vis, and IR spectroscopy. Highly dispersed vanadia
and titania were prepared by incipient wetness impregnation of the
corresponding isopropoxide precursors onto silica SBA-15. Using resonance
Raman spectroscopy, a wide range of vanadium (0.00001–0.7 V/nm2) and titanium (0.001–0.7 Ti/nm2) loadings
can be analyzed. At very low loadings (<0.05 M/nm2)
the structure of both highly dispersed vanadia and titania is characterized
by tetrahedral coordination of the central atom and anchoring to the
support by one or more M–O–S linkages. At higher loadings,
titania partly forms oligomeric surface structures according to UV–vis
results. In the case of highly dispersed vanadia samples (<0.1
V/nm2), Raman spectroscopy reveals distinct differences
in the vanadia surface structures under ambient and dehydrated conditions.
Corresponding UV–vis spectra indicate the formation of isolated
and oligomeric vanadia surface structures. A smaller dependence of
the titania surface structure on the environmental conditions (ambient/dehydrated)
was observed. For the 0.7 M/nm2 samples, the presence of
hydroxylated vanadia and titania structures in the dehydrated state
was verified by IR spectroscopy. The assignment of the vibrational
bands was facilitated by the results of a normal-mode analysis using
models based on polyhedral oligomeric silsesquioxane (POSS). Our study
clearly demonstrates the potential of resonance Raman spectroscopy
using 217.5 nm deep UV excitation to study the surface structure of
transition metal oxide species even in isolated conditions.
“…The Raman spectra displayed in Figure show high peaks at 443 and 610 cm –1 for E g and A 1g modes of rutile TiO 2 , respectively, thereby confirming that the predominant TiO 2 crystal structure is rutile. Nevertheless, the peak located between 806 and 836 cm –1 is associated with Ti–OH stretching vibrations, which emerged only after PEC measurements in alkaline electrolytes.…”
Section: Resultsmentioning
confidence: 98%
“…The Raman spectra displayed in Figure 3 show high peaks at 443 and 610 cm −1 for E g and A 1g modes of rutile TiO 2 , 25 respectively, thereby confirming that the predominant TiO 2 crystal structure is rutile. Nevertheless, the peak located between 806 and 836 cm −1 is associated with Ti−OH stretching vibrations, 26 which emerged only after PEC measurements in alkaline electrolytes. Figure 4 depicts the photocurrent density of the TiO 2 nanorod at 1.23 V vs RHE under different electrolyte pH with and without a hole scavenger (0.1 M H 2 O 2 ), which was derived from linear sweep voltammetry under chopped light, shown in Figure S3.…”
The redox reaction is related to the pH of the electrolyte
owing
to protonation/deprotonation during photoelectrochemical (PEC) water
splitting. However, the influence of electrolyte pH on water splitting
is not clear, especially the mechanism of the solid–liquid
interface mass transfer and carrier transport process under strong
acid and alkaline conditions. Herein, a comprehensive series of PEC
characterization methods including the linear sweep voltammetry, electrochemical
impedance spectroscopy (EIS), Mott–Schottky, and intensity-modulated
photocurrent/photovoltage spectroscopy (IMPS/IMVS) were deployed to
reveal the effect of pH on the carrier transport at the solid–liquid
interface layer using TiO2 and Sb2Se3 as the photoanode and photocathode, respectively. Our results indicated
that the photocurrent density under alkaline conditions can be as
much as six times greater than that under acidic conditions for Sb2Se3, while for the TiO2 photoanode,
the photocurrent under strong alkaline conditions was approximately
four times greater compared to that under acidic conditions. The relationship
between the photocurrent density and electrolyte pH was investigated
by injecting acidic and alkaline electrolytes through the electrode
surface using a multichannel syringe pump. According to the EIS results,
a rise in the pH reduces the impedance of the electrolyte/electrode
interface and improves the carrier separation efficiency. Interestingly,
the carrier collection efficiency, which is defined by the carrier
lifetime and transport time, was enhanced with a rise in electrolyte
pH. Our work provides a general approach to identify the relationship
between electrolyte pH and carrier dynamics at the electrolyte/electrode
interface by electrolyte regulation using a microchannel reactor.
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