Open Access Article
Anna A.
Wilson
a,
Thomas P.
Shalvey
b,
Andreas
Kafizas
ac,
Asim
Mumtaz
bd and
James R.
Durrant
*ae
aDepartment of Chemistry, Centre for Processable Electronics, Imperial College London, London, W12 0BZ, UK. E-mail: j.durrant@imperial.ac.uk
bStephenson Institute for Renewable Energy, Department of Physics, University of Liverpool, Liverpool, L69 7ZF, UK
cLondon Centre for Nanotechnology, Imperial College London, SW7 2AZ, UK
dSchool of Physics, Engineering & Technology, University of York, Heslington, York, YO10 5DD, UK
eSPECIFIC IKC, College of Engineering, Swansea University, Swansea, SA2 7AX, UK
First published on 6th September 2023
Charge carrier dynamics studies of SrTiO3 under applied bias offer the opportunity to gain unique insights into what underpins its state-of-the-art photocatalytic water splitting activity. Herein, time resolved spectroscopic measurements are employed, to investigate the impact of applied bias on the transient and steady state charge carrier dynamics of SrTiO3 across μs–s timescales, and simultaneously measure charge extraction kinetics. A high density of Ti3+ defect states in SrTiO3 photoanodes are identified and associated with prevalent electron trapping into deep states, which is in competition with electron extraction and limits the photocurrent. Despite the high density of trapped electrons, an intrinsically long lifetime for photogenerated holes in SrTiO3 photoanodes is observed using transient absorption spectroscopy, even in the absence of applied bias. This is important for overcoming the slow kinetics and hole accumulation associated with the water oxidation reaction, and for enabling good performance in photocatalytic systems where bias cannot be applied.
In contrast to the state-of-the-art performance of SrTiO3-based photocatalysts achieving up to near-unity quantum efficiencies,6,7,9 the performance of SrTiO3 photoanodes employed in PEC water splitting are modest compared to alternative metal oxide materials. As such, research into the use of SrTiO3 for water splitting has largely been focused on the use of particles for photocatalytic applications.6,7,10–12 Following the optimisation of Nb doping to improve the conductivity and photocurrent densities of SrTiO3, photocurrents of ∼0.1 mA cm−2 have been reported.13,14 These photocurrent are significantly lower than the photocurrents of 2.6–6.75 mA cm−2 achieved by photoanodes based on TiO2, BiVO4, WO3 or α-Fe2O3.15–21 Most previous work on SrTiO3 photoanodes has focused on enhancing the achievable current densities, such as by doping. However, as demonstrated recently by Chen et al.,22 studying the charge carrier dynamics of SrTiO3 photoanodes offers valuable opportunities to investigate the impact of applied bias on the charge carrier kinetics and interfacial charge carrier processes of this material, even in the absence of high photocurrent densities. Thus, such studies can provide functional insights that would be challenging to obtain through the study of isolated particulate photocatalysts.
As is the case for many metal oxide materials, under ambient conditions SrTiO3 is non-stoichiometric, with oxygen vacancies (VO) resulting in its n-type character. In SrTiO3, the formation of Ti3+ defect states is reported to coincide with VO generation, in order to maintain charge neutrality.11,23 The impacts of VO and associated defect states in metal oxides are extensive, with implications on charge trapping, recombination, transport and the resulting water splitting performance.24–26 In order to understand the impact of these defect states, kinetic studies are often required to determine whether they enhance or are of detriment to charge separation and lifetimes.
In this work, SrTiO3 photoanodes are characterised and investigated with and without applied bias, with the aim of improving our understanding of their underlying charge carrier dynamics and photophysical properties, rather than their photoanode performance. Transient absorption spectroscopy (TAS) on μs–s timescales is employed to measure the decay kinetics across the visible to NIR, in addition to the effects of bias induced band bending on charge separation and lifetimes. The application of bias to the TAS measurements enables spectral assignments to be made that do not rely on the reactivity of photogenerated charges towards chemical scavengers.27,28 Furthermore, the charge extraction kinetics following laser excitation are determined by transient photocurrent (TPC) measurements. The combination of these characterisation techniques reveals the competition between deep electron trapping and electron extraction, which consequently limits the photocurrent densities achieved. However, even in the presence of prevalent deep electron trapping, long lived hole species are observed that are not dependent on an anodic bias, which is favourable for the use of SrTiO3 in particulate photocatalysts.
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1. The ground state optical absorption was measured with a UV-vis spectrometer (Shimadzu UV-2600). The surface chemical composition and valence band structure was measured by X-ray photoelectron spectroscopy (XPS), using a Thermo K-Alpha spectrometer with a monochromated Al Kα radiation source.
| VRHE = VAg/AgCl + 0.0591pH + V0Ag/AgCl | (1) |
Transient photocurrent (TPC) measurements were undertaken using the same experimental set-up as for TAS measurements under applied bias, but with a change in the time base recorded by the oscilloscope. Following laser excitation with the laser pulse, the photogenerated TPC was obtained by measuring the voltage change with the oscilloscope from 10 μs to 0.1 s, triggered by the laser pulse induced trigger signal measured by the photodiode. In this measurement, data from the DAQ is not required.
![]() | (2) |
| A = εh+ × c × l | (3) |
![]() | (4) |
The charge carrier dynamics of the SrTiO3 films were first investigated in the absence of applied bias and under inert N2 conditions. The transient absorption spectrum at 10 μs is comprised of two features: a feature in the visible (<600 nm) that grows in amplitude with decreasing wavelengths and a broad feature in the early-NIR (Fig. 2a). Such features in the visible and early-NIR regions are in good agreement with the spectroscopic features reported in the literature on μs timescales for SrTiO3 particulate photocatalysts, and vary in relative intensity depending on the fabrication route and defects present.36,37 The decay kinetics exhibit a clear dependence on probe wavelength, with a distinct change in decay kinetics observed at probe wavelengths below and above 600 nm (Fig. 2b). Interestingly, the lifetimes observed below 600 nm are much longer than those typically observed in metal oxides in the absence of bias or chemical scavengers.27,28,38
The impact of applied bias on the decay kinetics was investigated, to enable spectral assignments of the two spectral features with distinct decay kinetics, as well as to determine the role of applied bias in modulating band bending and the resulting charge carrier dynamics. With increasingly anodic bias, electron extraction is increased (as observed as an increase in photocurrent, Fig. S5†) and is therefore expected to increase the yield of long lived holes. At 500 nm, the decay kinetics become slower and the optical signals increase in amplitude with increasingly anodic bias (Fig. 3a). Thus, 500 nm and the corresponding spectral region probed below 600 nm is assigned primarily to hole species. In contrast, at 800 nm the decay kinetics accelerate and optical signals decrease in amplitude with increasingly anodic bias (Fig. 3b). Therefore, 800 nm and the corresponding early-NIR feature is assigned primarily to electron species. This distinction between photoinduced absorption in the visible and NIR spectral regions being preferentially dominated by respectively hole and electron absorption is typical of SrTiO3 and other metal oxides.36,37,39–42 Although this bias dependence of the decay kinetics was sufficient to make spectral assignments, the bias dependence was much less dramatic than that observed in other metal oxides.27,28,38 This is consistent with the low photocurrent densities and suggests that factors other than bias induced band bending are responsible for the long hole lifetimes. The distinct kinetics observed for holes and electrons suggests that the decays observed do not simply correspond to the recombination of the two probed species. Instead, an additional decay pathway that reduces electron lifetimes must be present. As such, our observation of faster electron decays compared to hole decays, even at modest anodic biases where no photocurrent is observed, indicates two competing processing for electron decay on the timescales studied: electron relaxation/trapping within the SrTiO3 and, under strong anodic bias, electron extraction to the external circuit. The immobile nature of trapped charges may also contribute to the small degree of bias dependence, as explored further in the discussion.
![]() | ||
| Fig. 3 SrTiO3 photoanode TAS decays in 0.1 M NaOH under applied bias, using a 355 nm laser at an excitation intensity of 400 μJ cm−2 and 0.8 Hz repetition rate. Probed at (a) 500 nm, and (b) 800 nm. | ||
The charge extraction kinetics from TPC measurements, undertaken in parallel with the TAS experiments, show reasonably fast kinetics, with a peak charge extraction at 0.1 ms (Fig. 4a). These kinetics are similar to those observed in BiVO4 photoanodes, and significantly faster than in WO3.26,38 These charge extraction kinetics are also consistent with the timescales at which the TAS electron signal exhibits accelerated decays with increasingly anodic applied bias (Fig. 3b) (i.e.: only a marginal fractional change in the TAS electron signal is observed at 10 μs with anodic bias, but there is increasing signal loss at longer time delays). This confirms that the faster electron decays at strong anodic bias can be assigned to increased electron extraction.
Using the cumulative charge extracted (Fig. 4b) and the earlier spectral assignment of holes, the hole extinction coefficient (εh+) can be calculated using a method previously reported in our group and explained in the Experimental section.29–31 Briefly, this method uses the Beer–Lambert law and the relationship between the hole absorbance (measured in TAS at 500 nm, Fig. 4c) and the surface hole density (calculated from the cumulative charge extracted, Fig. 4b) at a range of excitation intensities, to extract the εh+. The TAS and TPC measurements used to extract the hole absorbance and surface hole density are undertaken under a sufficiently anodic applied bias (1.3 VRHE), whereby the absence of photocurrent spikes in Fig. S5 and S6a† suggests back electron–hole recombination has been turned off. Both the hole absorbance and surface hole density increase with increasing excitation intensities, until they begin to plateau at 630 μJ cm−2. It is notable that the decay dynamics of this TAS hole signal are independent of laser intensity, indicating that the decays do not result from bimolecular recombination, which is consistent with our conclusion above regarding the decay kinetics not simply being the result of recombination of the probed species. Instead, the decays are attributed to a monomolecular process, as we discuss further below. A linear correlation between the hole absorbance and surface hole density is obtained (Fig. 4d). The εh+ is subsequently extracted from the gradient of the linear fit using the Beer–Lambert law, to yield a εh+ of 2200 ± 100 M−1 cm−1. Since this is the first calculation of the εh+ in SrTiO3 to our knowledge, it cannot be compared to previously reported values for SrTiO3. However, it is reasonable when compared to the εh+ reported for dense anatase TiO2, of 2000–2930 M−1 cm−1,30,43 which has similar optoelectronic properties to SrTiO3, such as valence and conduction bands that correspond to the density of states from O 2p and Ti 3d orbitals respectively.44 It is noted that despite the reasonable εh+ value and associated error, the linear fit does not completely extrapolate to zero, suggesting that there is a small electron contribution to the 500 nm absorbance.
The steady-state kinetics of hole accumulation and decay were measured by PIAS using a quasi-steady state 8 second LED light pulse under strong anodic bias. The PIAS signals increase with increasing excitation intensities (Fig. 5), which is attributed to increased charge generation and resulting steady-state charge densities. Upon light-off, the hole signals decay with t50% decay times of ∼0.5 s (Fig. 5, inset). These hole decays, which most likely have contributions from recombination and water oxidation, are termed τdec herein. Following this initial decay there is a residual signal that remains and decays very slowly, likely due to a population of trapped hole species that do not contribute to photoelectrochemical activity.45–47 The kinetics of hole consumption were further investigated by a rate law analysis, where the hole flux to the surface (equated to the photocurrent extracted) is correlated to the steady-state surface hole density.29–31,48–50 To achieve this, the steady-state photocurrent (Fig. S6a†) is measured simultaneously with the steady-state hole absorbance in PIAS (Fig. 5). The hole absorbance signal is converted to a surface hole density, using the calculated hole extinction coefficient of 2200 M−1 cm−1 (Fig. 4d). Under these conditions a second order reaction is measured (Fig. S6b†), in agreement with a recent study by Chen et al.,22 and previously reported orders between one and three for other metal oxide photoanodes.29–31 A second order reaction indicates that the rate limiting step of water oxidation, on SrTiO3 photoanodes under these operating conditions, involves the accumulation of two hole species (or oxidising equivalents). However, due to the low photocurrent densities observed herein, we are cautious of strongly assigning hole consumption to water oxidation alone. The reaction time constant can also be calculated from the ratio between the hole flux to the surface and the surface hole density (Fig. S7†). The hole decay times indicated by this time constant only take into account the reaction of surface holes that have avoided electron–hole recombination and are termed τsurf. The τsurf values calculated are in the range of 1–5 s, which indicates a slower hole decay time than that obtained from the PIAS decays (0.15–0.5 s). This is consistent with τsurf being indicative of water oxidation kinetics alone, whilst τdec results from the sum of both water oxidation and hole recombination/trapping pathways, which will be explored further in the discussion.
Using TAS on μs–s timescales, distinctly different decay kinetics of electrons and holes are observed, with slower decay kinetics attributed to the hole species probed below ∼600 nm. This is indicative of an additional decay pathway being present that extends hole lifetimes. Interestingly, wavelength dependent decay kinetics and long lifetimes in the absence of applied bias have also been observed in BaTiO3,51 which shares the cubic perovskite structure of SrTiO3. Even though the bias dependence of the TAS kinetics was sufficiently clear to enable confident spectral assignments and calculation of the εh+, the extent of changes in TAS signals with bias dependence was small compared to what is commonly observed in other metal oxide photoanodes.27,28,30,52 The small degree of bias dependence in SrTiO3 and considerable charge carrier lifetimes, even in the absence of bias, implies that the intrinsic properties of SrTiO3 enable the generation of remarkably long lived holes. This is an especially important feature in photocatalytic applications of SrTiO3 particles, where a bias cannot be applied to drive the necessary charge separation and lifetime gains for the slow interfacial water splitting reactions.
The chemical doping density from Ti3+ donor states, that are associated with electron occupied oxygen vacancies and approximated using the Ti3+ concentration measured by XPS, is high at ∼1020 cm−3. The high Ti3+ chemical doping density is indicative of a high electron occupancy of the Ti3+ defect states, suggesting that they are sufficiently deep to have much of their distribution below the EF level. The deeply trapped electrons in these states are likely to be immobile and unable to be extracted to contribute to the photocurrent. Thus, the prevalent trapping of electrons into deep VO states, prior to the timescales of the TAS measurement, may explain the low photocurrents measured herein, despite the relatively fast electron carrier extraction rate (peaking at 0.1 ms) and intrinsic charge separation properties in SrTiO3 observed. With this in mind, the improved photocatalytic performance of Al3+ doped SrTiO3,8 likely results from the suppression of these deep trap states. The large Ti3+ chemical doping density is approaching that of WO3 (∼1020–1022 cm−3),53,54 which is widely recognised for its high doping density from VO, that result in W5+ states when occupied by an electron.41 In WO3, a slow charge extraction rate (peaking at 1 ms)38 coincides with the high density of VO, due to the slow trapping–detrapping electron transport that proceeds via the shallow trap states.25 In SrTiO3, the electron trapping may limit the size of the photocurrent but it does not result in a slow extraction rate, possibly due to the immobile nature of the deeply trapped electrons limiting their influence on the charge extraction kinetics.55 The immobile nature of these trapped charges also aids explanation of the small degree of bias dependence of the decay kinetics.
The τdec extracted from the PIAS decays (∼0.5 s) is shorter than the τsurf calculated using the comparison of the accumulated hole density vs. the photocurrent density (1–5 s). The τsurf only takes into account the reaction of surface holes with the electrolyte (i.e. water oxidation), whereas the PIAS decay times, τdec, are determined by the sum of recombination and water oxidation kinetics. Thus, the faster τdec times measured by PIAS suggests that even under strongly anodic bias, there is significant competition between water oxidation and an additional decay pathway for long lived holes. This additional decay pathway is attributed to electron–hole recombination mediated by the prevalent electron trapping into deep Ti3+ states, and is consistent with the excitation density independent hole decays measured in Fig. 4c. With this in mind the τsurf could be accelerated by material modifications, for example by adding a co-catalyst that promotes the water oxidation reaction, as has been reported previously.56,57 Cuk and co-workers previously reported the formation of intermediate Ti–O˙ surface radical species on SrTiO3, and suggested that holes were trapped as these surface radical sites on ps timescales.58 It is likely that the long lived holes we observe herein correspond to such Ti–O˙ radicals, with our data indicating that spatial separation from Ti3+ states enables their long lifetimes and a significant fraction of these to remain for 0.5 s after photogeneration. As discussed above, our PIAS data indicate that water oxidation by these SrTiO3 surface radicals proceeds on the 1–5 s timescale, slightly slower than the typical timescales of water oxidation on other metal oxides such as TiO2 at low surface hole densities.30 These slower kinetics may in part be related to the relatively low densities of surface holes accumulating on our electrodes due to competing recombination/trapping pathways.
It is striking that despite the high defect densities we identified in these SrTiO3 photoanodes, we also observed remarkably long lived holes (possibly as surface Ti–O˙ radicals), even in the absence of anodic bias. In particular, it is noteworthy that the high density (∼1020 cm−3) of Ti3+ states do not result in rapid hole recombination. This may be associated with the unusually high dielectric constant of SrTiO3 compared to other oxides (∼300 for SrTiO3,59–62 compared to 13–45 for anatase TiO2,63 32–86 for BiVO4,64–66 and 18–26 for α-Fe2O3 (ref. 67 and 68)), which can be expected to reduce the Coulomb attraction of electrons and holes. It is also possible that band bending resulting from surface dipoles between facets of differing energy may aid the spatial separation of these holes from Ti3+ states.69,70 An energy offset between facets with different surface dipoles was previously proposed as the reason for facet selective photodeposition of co-catalysts on the near-unity SrTiO3 photocatalyst materials.6 In either case, the ability of SrTiO3 to sustain these long hole lifetimes is likely to be a key factor behind the success of this material in photocatalyst particles for unassisted water splitting.6,7,9
The charge carrier dynamics of our SrTiO3 photoanodes obtained herein, using TAS on μs–s timescales, PIAS and TPC measurements, are summarised in Fig. 6. As observed in the TAS data in Fig. 3b, electron trapping occurs on the <0.1 ms timescale, most likely resulting from the formation of localised Ti3+ states associated with the deep VO states. As a result of this deep trapping, a significant population of the electrons are relatively immobile, and therefore cannot be efficiently extracted. This electron trapping appears to be in kinetic competition with electron extraction to the external circuit on the ∼0.1 ms timescale. This electron trapping, and bulk recombination losses from the high density of Ti3+ states, appear to be the primary origins of the low photocurrent densities observed for these photoanodes. As a result of prevalent charge trapping and recombination in the SrTiO3 herein, even under anodic bias, the hole densities that accumulate in SrTiO3 on long (ms–s) timescales are low. Surface holes (Ti–O˙ radicals) oxidise water on seconds timescales, in competition with faster (0.15–0.5 s) recombination losses, most likely associated with back electron–hole recombination with Ti3+ states. The ability of SrTiO3 to maintain long hole lifetimes regardless of the applied bias is remarkable and aids explanation of why SrTiO3 is well suited to particulate photocatalytic applications despite its low photocurrents.
Footnote |
| † Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d3se00886j |
| This journal is © The Royal Society of Chemistry 2023 |