Dong-Li Gao,
Yi Wang*,
Ping Zhang,
Li-Min Fu,
Xi-Cheng Ai and
Jian-Ping Zhang
Department of Chemistry, Renmin University of China, Beijing, 100872, P. R. China. E-mail: gaoyangdongli@sina.com; ywang@ruc.edu.cn; zhangp1988spl@163.com; lmfu@chem.ruc.edu.cn; xcai@chem.ruc.edu.cn; jpzhang@chem.ruc.edu.cn; Tel: +86-10-62516560
First published on 29th September 2015
We carried out a time-resolved charge extraction (TRCE) study on the charge recombination dynamics of open-circuit dye-sensitized solar cells (DSSCs) by examining the temporal evolution of electron density with varying the concentration of the electrolyte component tert-butylpyridine (TBP). The charge recombination dynamics extracted from TRCE results exhibit distinctly different temporal behavior depending on the photovoltage or electron density. We proposed a theoretical model of electron density dependent charge recombination, which unifies the transport- and transfer-limited charge recombination mechanisms. This model, as rationalized by transient photovoltage (TPV) kinetics, can account well for the TRCE results. The relevance between electron transport and charge transfer in the recombination process was unraveled, and the electron density dependent pathway of charge recombination was elucidated.
However, during the charge transport in photoanode, considerable electrons may be consumed via charge recombination. Consequently, the competition between the charge transport and recombination plays a crucial role in determining the overall PCE of DSSCs. Because of the rapid regeneration of oxidized dyes by electrolyte (such as the iodide), charge recombination between oxidized dye molecules and electrons in photoanode is often negligible, and the neutralization between the electrons in TiO2 and the acceptors in electrolyte (e.g. the triiodide) is regarded as the dominant pathway of charge recombination.13–16 Charge recombination may take place at the mesoporous TiO2/electrolyte and/or FTO/electrolyte interfaces, depending on the components of electrolyte, configuration of photoanode, and the illumination condition. For the DSSCs constituted by TiO2-based photoanode and I−/I3−-based electrolyte, the TiO2/electrolyte interface is suggested to be the primary recombination site, as revealed by means of intensity modulated photovoltage spectroscopy (IMVS) and electrochemical impedance spectroscopy (EIS).17–19 Particularly, by testing the voltage-dependent charge transfer resistance, Lagemaat et al. give a strong evidence about the substantial role of charge recombination at TiO2/electrolyte interface in DSSCs.20 In this case, the process of charge recombination involves two aspects, i.e. the transport of electrons in photoanode to reach a recombination site and the transfer of electrons from TiO2 to electrolyte at recombination sites. Hereinafter, in order to distinguish these two processes, they will be termed as “electron transport” and “charge transfer” respectively. Previously, charge transfer was often treated as the rate determining step of recombination, based on which the dynamics of charge recombination was described by the model of transfer-limited recombination.21 Though the reaction mechanism of charge transfer is still in debate to date, by invoking this model, the proportional relation between recombination rate constant (kR) and the square of electron density (n2) was successfully interpreted.18,22–24 It should be noted that transfer-limited recombination was established by assuming charge recombination and electron transport are two independent processes, that's to say the influence of electron transport on charge recombination is negligible. Unfortunately, the subsequent studies revealed this hypothesis seems to be unreasonable. By means of transient photocurrent (TPC) and transient photovoltage (TPV), Kopidakis et al. found the dynamics of both electron transport and charge recombination varied simultaneously with the changing of Li+ concentration in electrolyte.13 What's more, the time constants of transport (τt) and of recombination (τn) showed nearly identical dependence upon electron density.25,26 These experiments indicated that charge recombination is strongly coupled with electron transport in photoanode, conflicting with the transfer limited recombination model. Based on this point, an alternative model i.e. the transport-limited recombination model was introduced, in which the rate of recombination is considered to be predominantly determined by electron transport in photoanode rather than charge transfer at TiO2/electrolyte interface.27 Obviously, the relevance between electron transport and charge recombination is well interpreted by this model; however there are still some imperfections while the most notable one is the over-simplification of treating the probable recombination pathways. As described by transport-limited recombination model, both of electron transport and charge transfer can only take place in conduction band, that's to say, the conduction band of TiO2 was the only recombination channel. Nevertheless, based on the theoretical simulation of open-circuit voltage decay (OCVD) kinetics in DSSCs, Bisquert et al. found that both of conduction band and surface states of TiO2 can act as recombination sites depending on the scale of electron density.28 In addition, these authors proposed a novel model claiming that charge recombination takes place dominantly through the surface states and conduction band, respectively, at low and high electron density.28 Very recently, some groups successively reported the observation of nonlinear recombination in DSSCs, implying the involvement of surface states in charge recombination.29,30 Besides, this model is also used to interpret the particular dependence of open-circuit voltage (VOC) on illumination intensity in DSSC, but more specific kinetics or dynamics studies are needed to confirm its reasonability, as the authors claimed, because the model invokes too many adjustable parameters for numerical fittings.31 On intuition, anyhow, the latest model mentioned above is unambiguous, since it can quantitatively interpret the result of OCVD on the base of Fermi–Dirac statistics. However, the rationalization of Fermi–Dirac statistics in OCVD measurement was then queried. Boschloo and Hagfeldt utilized numerous techniques, such as TPV, time-resolved charge extraction (TRCE), IMVS and OCVD, to study recombination dynamics of the same DSSC sample.32 Surprisingly, the results of TPV, TRCE and IMVS exhibited high agreements; while the OCVD result significantly deviates from the results of aforementioned measurements. The inaccuracy of OCVD was assigned to the utilization of the Fermi–Dirac statistics, in practically at low electron density.32 This interpretation is very possible, because Fermi–Dirac statistics is only appropriate for electrons in thermal equilibrium and this requirement was meet under the perturbation conditions (such as the experimental condition of TPV and IMVS).33,34 On the other hand, the OCVD measurement is often utilized to investigate the recombination dynamics with the decay of voltage from a high value to zero. In this case, the studied system especially at low electron density breaks the thermal equilibrium and dissatisfies the precondition of Fermi–Dirac statistics. In fact, the results indicated by OCVD at low electron density i.e. electron lifetime depended on voltage in reciprocal of the Gaussian,28 to our best knowledge, has never been observed by other means. Bisquert et al. have used Marcus theory to describe the kinetics of electron transfer both from conduction band and from surface trap states to electrolyte acceptors, but they neglected the truth that electrons in surface trap states are much more localized than those in conduction band, which may lead to a substantially lower charge transfer coefficient. As a result, the landscape of charge recombination via conduction band would be significantly different from that via surface states (vide infra).
In the present work, we directly explored the temporal evolution of electron density in DSSCs at open circuit, by means of TRCE, without invoking Fermi–Dirac statistics. In this case, we could study the recombination dynamics and avoid introducing errors from the improper adoption of Fermi–Dirac statistics. On the base of TRCE results, the mathematic expression of recombination rate constant as a function of electron density was derived. In addition, a physical model focusing on the description of charge recombination mechanisms in working DSSCs was put forth, which was experimentally verified by the results of TPV measurement. At last, the influence of electrolyte components on recombination dynamics was quantitatively analyzed.
(1) Electrolyte of cell-1: LiI (0.05 M), I2 (0.03 M), tert-butylpyridine (TBP, 0.5 M), guandinethiocyanate (GuNCS, 0.1 M) and 1-butyl-3-methylimidazolium iodide (BMII, 1 M) in an acetonitrile–valeronitrile binary solvent (5
:
1, v/v).
(2) Electrolyte of cell-2: same to cell-1, but reducing the TBP to 0.01 M.
At low electron density, most of electrons in photoanode populate in deep trap states and recombine with the acceptors in electrolyte predominately through the surface states (Scheme 1). The rate of recombination strongly depends on charge transfer kinetics at TiO2/electrolyte interface coinciding with the description of transfer limited recombination mechanism. Based on Marcus theory of single electron transfer, the rate constant of charge transfer is written by:
![]() | (1) |
![]() | (2) |
At low electron density, as verified by numerous works, charge transfer is significantly slower than electron transport.38–40 On the other hand, the mechanism of electron transport in photoanode is generally described by multiple-trapping model or hopping model. In the former, conduction band of TiO2 is regarded as the only transport pathway and electrons in trap states should be thermally released to conduction band prior to their effective motion;41 whereas, the hopping model assumes that electron transport occurs by jumping among trap states.42 At low electron density, the multiple-trapping model may be void, because EFn is far below the conduction band and electrons in trap states are difficult to be excited into conduction band. Hence, hopping among trap states is suggested to be the dominant pathway of electron transport at low electron density. Considering the electrons trapped by surface states are intensely localized which results in slow electron transfer from TiO2 to electrolyte,43 it's reasonable to expect that the distribution of electrons at surface trap states will get equilibrium by rapid hopping preceding charge recombination. As thus, charge transfer dominantly takes place through the surface states with E = Eox, i.e. the fastest recombination channel (eqn (2)), because electrons at other energy levels will quickly hop to the surface states with E = Eox to sustain the electron equilibrium before they are consumed by electrolyte, as shown in Scheme 1. If so, the rate constant of recombination at low electron density turns to be a constant,
![]() | (3) |
By contrary, the scenario of recombination at high electron density is quite different. Under this circumstance (see Scheme 1), EFn approaches to conduction band and multiple-trapping of electrons becomes significant, as a result, conduction band displaces the surface states as the dominant transport pathway,28 because the electrons are much more delocalized in conduction band than those in surface trap states, electron transfer from TiO2 to electrolyte via conduction band is also much faster than that via surface trap states.43 What's more, the rate of charge transfer via conduction band is even faster than electron transport, which leads the electron transport but not charge transfer to be the rate-determining step of recombination, following the description of transport-limited recombination mechanism. Based on multiple-trap theory and the continuity equation, the rate constant of transport-limited recombination can be derived as below,44
![]() | (4) |
On the strength of the derived kR–n relations (eqn (3) and (4)), the evolution of electron density can be obtained. In general, the expression of recombination rate is written as:
![]() | (5) |
At low electron density, recombination rate is limited by charge transfer via surface trap states, and the kR–n relation is written by eqn (3). Combining eqn (3) with eqn (5), one can obtain the temporal evolution of electron density as:
![]() | (6) |
In the same way, at high electron density where the recombination turns to be limited by electron transport, the evolution of electron density is obtained by inserting eqn (4) into eqn (5):
![]() | (7) |
Eqn (6) and (7) indicate that electron density depends on time in exponential and power form, respectively, at low and high electron density.
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| Fig. 1 Current density–voltage (J–V) characteristics of cell-1 (black circle) and cell-2 (red circle). The solid curves are fitting results based on standard diode equation (see text for details). | ||
In order to study the dynamics of charge recombination in the target samples, we investigate the temporal evolution of charge amount (Q)/electron density (n) under open-circuit by means of TRCE following the previous report,22 as depicted in Fig. 2. For each DSSC sample, the decay of n includes a fast component at high electron density (i.e. short delay time) followed by a slow one at low electron density (i.e. long delay time), based on the proposed model (Scheme 1), which are respectively fitted by the transport- (eqn (7)) and transfer-limited (eqn (6)) recombination mechanism.
On the base of temporal evolution of electron density, the dependence of recombination rate constant (kR) on electron density was quantitatively derived by invoking eqn (5). As illustrated in Fig. 3, kR is a constant at low electron density while increases significantly with n at high electron density (Fig. 3(a)). Particularly, in the case of high electron density, kR–n relation could be described by a power function as shown by Fig. 3(b), where the linearity under log–log coordinate was clearly seen. Meanwhile, it's worth noting that the value of kR in cell-2 is obviously larger than that in cell-1, as discussed above, resulting from the variation of TBP concentration in electrolyte. Interestingly, at high electron density, one can see the slopes of kR–n plots under log–log coordinate are nearly same. This issue will be interpreted by taking into account the effect of trap states distribution on recombination dynamics (vide infra).
To get further insight into the charge recombination dynamics, we performed TPV measurement for the two cells, from which the relation between electron lifetime (τn) and voltage could be obtained. In addition, based on the reciprocal relationship between kR and τn, kR–Vph plots could be easily derived which were plotted in Fig. 4. Either in the case of cell-1 or cell-2, as seen from Fig. 4(a) and (b), kR is constant at low voltage (<0.4 V) while increases remarkably at high voltage (>0.4 V). More importantly, in the region of Vph > 0.4 V, kR exhibits exponential dependence upon Vph (Fig. 4(c) and (d)). By invoking the proposed model, kR–Vph relations were respectively fitted within the framework of transfer-limited recombination mechanism at low voltage and of transport-limited recombination mechanism at high voltage. It's noted that the scale of Vph was determined by the density of electrons in photoanode. The high coincide between the results of TPV and model fitting, once again, proved that the dynamics of charge recombination is limited by charge transfer at low electron density while by electron transport at high electron density.
Having proved the reasonability of the proposed model, we now unravel the reasons of resulting in the distinct recombination dynamics between cell-1 and cell-2 in details. At low electron density, charge recombination is described by transfer-limited model. In this case, the kR–n relation is expressed by eqn (3) which indicates the value of kR is determined by a series of variable parameters, i.e. T, ks, λ and cox. The redox specials are identical for target samples and the experimental temperature is same, which implies T, λ and cox are changeless, as a result, the difference of kR values totally arises from the different ks. It's noted that the TBP concentration in cell-2 (0.01 M) is much lower than that in cell-1 (0.5 M), which is the only difference between the target samples. Because TBP could block the contact between TiO2 and electrolyte which is beneficial for blocking charge transfer from TiO2 surface to electrolyte,45 one can now understand the enhancement of ks and kR in cell-2 due to the reduced concentration of TBP. On the other hand, the situation at high electron density is quite different. In this case, recombination dynamics is limited by electron transport in photoanode and kR depends on n in power (see Fig. 3(b)), which is now determined by k0, Nc, Nt, α and β (see eqn (4)). k0 is expected to be larger in cell-2 than that in cell-1, because the reduced TBP in cell-2 results in more intimate contact between TiO2 and electrolyte as discussed above. Consequently, the difference of the k0 values is one of the factors leading the different kR between cell-1 and cell-2. Meanwhile, the TiO2 photoanode, which is assembled by sintered P25 particles, is same for the target samples; therefore the difference of Nc is expected to be negligible. The rest parameters, Nt, α and β, are related to the distribution of bandgap trap states in TiO2, so we investigate the Q–V relations to check the density-of-states (DOS) in cell-1 and cell-2 by means of TRCE following reported method.36,37 In the region of 100–580 mV, as seen in Fig. 5, the Q–V plots are fitted by monoexponential functions exhibiting the same slope, which indicates the value of α is same for the target samples. Meanwhile, the slope of kR–n under log–log coordinate, which is determined by both of α and β (eqn (4)), is also similar between cell-1 and cell-2, hence the value of β is expected to be identical. The value of Nt is suggested to be larger in cell-2 than that in cell-1, when taking the “physical trap states” into account.49 Compared to the structural trap states which may be caused by Ti4+(3d0) sites and/or oxygen vacancies,50,51 the electrostatic attraction between the electrons in TiO2 phase and the cations in electrolyte is termed as physical trap states.49 Because the higher TBP concentration in cell-1 is more effective to block the contact between TiO2 and cations in electrolyte, the larger Nt in cell-2 could be understood. In fact, as seen from Fig. 5, the Q–V plot of cell-2 shifts upward versus that of cell-1, which confirms the larger Nt in cell-2. As a conclusion, the difference between the values of kR in cell-1 and cell-2 at high electron density comprehensively results from the variation of k0 and Nt; while the same slope of kR–n plots under log–log coordinate arises from the same α and β. To sum up, the effect of TBP concentration on charge recombination dynamics is summarized as below: at low electron density, TBP suppresses recombination by blocking the contact between TiO2 and electrolyte, which is responsible for the reduction of interfacial charge transfer coefficient; at high electron density, TBP influences recombination rate by hindering the contact between TiO2 and electrolyte on one hand, and by adjusting the DOS in photoanode on the other hand.
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| Fig. 5 Q–Vph plots of cell-1 (black circle) and cell-2 (red circle). The solid lines are monoexponential fitting in the region of 100–580 mV. | ||
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