Charu Seth and
Deepa Khushalani*
Materials Chemistry Research Group, Department of Chemical Sciences, Tata Institute of Fundamental Research, Homi Bhabha Rd, Colaba, Mumbai, India 400005. E-mail: khushalani@tifr.res.in
First published on 20th October 2016
A hybrid organic inorganic perovskite, CH3NH3PbI3, has been deposited, using a two-step deposition technique, on three different substrates: bare FTO and two different types of TiO2 electron transport layers. These structures have then been monitored, using XRD, for degradation under exclusively ultraviolet (UV) and visible light. It has been observed that the topography of the underlying substrate is shown to impose a substantial effect on the particle size of the HOIP phase that gets deposited on top. Furthermore, subsequently it has been observed that the particle size, the level of crystallinity and also type of irradiation (UV vs. visible light) all are important parameters that substantially influence the rate and manner of degradation of HOIPs. These are in addition to the oft-cited parameters such as moisture, O2 and temperature. Moreover, depending on the level of degradation, it has been intriguingly observed that the HOIP phase can be regenerated upon a simple treatment involving I2 deposition. This latter aspect has the potential to circumvent the deleterious degradation that is hindering further progress with this highly promising material.
Irrespective of the mechanism of degradation, it is important to note, that for a fully viable solar cell device, all the aforementioned parameters (H2O, O2, light) are present under ambient conditions, and it would be difficult to mitigate their influence during operation of any device. This is especially important if the cost of the device has to be maintained at a reasonable level.
As such, presented here is a study of the XRD evaluation of the formation and degradation of HOIPs, specifically methyl ammonium lead iodide, all the while being exposed to ambient conditions (hence humidity, oxygen and light). We have evaluated two specific parameters: (a) primarily we have explicitly varied the nature of the underlying electron transport layer. Specifically, we have deposited HOIP on a conducting electrode and then subsequently on two different types of TiO2. One consists of the oft-cited P25 phase (nanoparticles of titanium oxide) and the other consists of in situ synthesized TiO2 nanowires, grown uni-directionally on FTO. To the best of our knowledge, this is the first study whereby degradation has been monitored by manipulating the underlying substrate morphology whilst keeping all other parameters constant, even the chemical composition of the underlying electron transport layer. We have observed that surprisingly the morphology and surface roughness of the underlying substrate imparts another condition on the degradation rate of perovskites and therefore it adds to the list of parameters that need to be paid attention to in order to minimize the degradation process. (b) Moreover, we have also evaluated the influence, individually, of UV and visible light on the degradation of these HOIP coated substrates. UV irradiation imposes a more dramatic effect on the degradation rate and this is irrespective of the underlying substrate present.
Furthermore, making a successful, degradation resistant device is possible, but involves deposition of additional layers (e.g., hydrophobic layers to minimize interaction of perovskite with moisture), adding to the cost of the overall device. The current study, in addition to describing the substrate dependent degradation, introduces a simple and cheap method to reverse the degradation itself caused by moisture and light. This method involves treatment of degraded perovskite samples with iodine that, depending on the degree of degradation, regenerates the tetragonal lattice of methyl ammonium lead triiodide as confirmed by the XRD and UV-visible absorption.
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Fig. 1 Top view scanning electron micrographs of (a) FTO, (b) NP–FTO, (c) NW–FTO, and (d) cross-sectional view of NW–FTO. |
Fig. 2 shows the SEM images of the perovskite layer that was deposited. Interestingly, it can be seen that the HOIP morphology is similar on the FTO and NW–FTO substrates (Fig. 2a and c) however different for NP–FTO (Fig. 2b). For FTO and NW–FTO, a range of sizes are observed, the smallest being irregular spheres about 100 nm in size, rods about 400 nm long, and cuboids about 500 nm in size. However, for NP–FTO, predominantly small particles with sizes less than 200 nm are observed. For clarity, a low magnification image of NW–FTO is also shown in Fig. 2d where a crack in the perovskite layer is imaged to showcase that the underlying TiO2 nanowires have maintained their integrity. For all the three samples, X-ray diffraction analysis confirmed the sole presence of the tetragonal phase of methyl ammonium lead triiodide, Fig. 3.
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Fig. 2 Top view scanning electron micrographs of HOIP coated on (a) FTO, (b) NP–FTO, (c) NW–FTO, and (d) low magnification view of HOIP/NW–FTO showing a crack in the film where NW is visible. |
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Fig. 3 X-ray diffractograms of HOIP coated on (a) FTO, (b) NP–FTO, and (c) NW–FTO. #, A, and R represent FTO, anatase, and rutile peaks, respectively coming from the substrates. |
It should be highlighted that the NP–FTO underlying substrate gave additional peaks belonging to rutile and anatase phase while NW–FTO only showed the rutile peaks. The level of crystallinity could be gauged by the full width half maxima (FWHM) of the lattice planes in the XRD patterns.
Table S2† shows the FWHM of the initial crystalline HOIP phase, and it was observed that FWHM of the HOIP on FTO and NW–FTO were similar and consistent while, the HOIP phase on NP–FTO appeared to show disorder and there was anomalous broadening of some lattice planes. This aspect is important as it denotes that the level of crystallinity was similar for HOIP phase grown on FTO and NW–FTO. However there was heterogeneity in the HOIP phase grown on NP–FTO. These films, as deposited were then allowed to age temporally under identical conditions (room temperature at 25 °C, humidity at 65%). Fig. S2† depicts an optical image of the degraded material as observed after 4 days. Visually, the degraded materials appear to be different for the different substrates present. Interestingly, X-ray diffraction patterns of the degraded HOIP on FTO and NW–FTO appear to be quite similar to each other, whereas the XRD pattern is unique for the degraded HOIP layer on NP–FTO, Fig. 4. The degraded sample on FTO and NW–FTO show low intensity peaks corresponding to the tetragonal phase of HOIP and additional peaks appear corresponding to the hydrated HOIP lattice.11 On the other hand, the degraded HOIP on NP–FTO shows prevalence of lead iodide phase along with peaks of HOIP that have dramatically decreased intensity. As a further to this, a systematic temporal study of degradation of HOIP was performed. This was monitored using XRD and the degradation conditions involved irradiating with exclusively UV or visible light, at 65% humidity and since irradiation causes a slight increase in temperature, all the samples (including those maintained under dark conditions) were maintained at 45 °C temperature. Fig. 5 shows the variation in the XRD intensity of peaks for three types of samples-HOIP/FTO, HOIP/NP–FTO, and HOIP/NW–FTO-in dark, and while being irradiated with exclusively UV light and visible light whilst keeping other parameters constant. Peak intensities of (110), (310), and (224) planes were carefully monitored as a function of time. For brevity, the data for only (224) plane has been shown and the trend observed is similar to those obtained for (110) and (310). The decrease in intensity of XRD lattice planes is a signature of loss of crystallinity and therefore loss of structure. As such, the in-dark profiles for all the samples show negligible slopes (Fig. 5a) which implies that little or no decrease in crystallinity and/or degradation is occurring. The profile for UV irradiated samples (Fig. 5b) shows different extents of degradation for the three samples as suggested by the negative slopes. The fastest to degrade was HOIP on NP–FTO, while the rate of decrease in the intensity of the (224) plane for HOIP on FTO and NW–FTO appears to be relatively similar.
The profile for visible light irradiated samples (Fig. 5c) suggests that HOIP on NP–FTO is the most unstable, an observation that correlates with Fig. 5b. The HOIP on FTO and NW–FTO remain stable (under visible light) for 44 hours of experiment as shown by the almost negligible slope of their respective (224) plane intensity. At this point, it needs to be noted that data was plotted only after an elapse of 10 hours since there was in fact an increase in the intensity of the XRD data for FTO and NW–FTO samples during these initial hours of irradiation, Fig. S3.† For these samples, be in-dark or in-light conditions, slightly positive slopes were observed in these first few hours (<10 hours) suggesting some level of re-organization such that crystallinity was being augmented (Fig. S3†). It is being hypothesized that as a temperature of 45 °C was being maintained for all the samples, this was perhaps leading to annealing of the HOIP phase in the initial hours. It was observed that this effect of temperature seemed to be pronounced only in the initial period and other parameters took precedence during the subsequent 10–44 hours that induced degradation.
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Fig. 6 X-ray diffractograms of fresh, degraded, and I2 treated HOIP deposited on (a) FTO, (b) NP–FTO, and (c) NW–FTO. |
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Fig. 7 Diffuse reflectance spectra of fresh, degraded and I2 treated HOIP deposited on (a) FTO, (b) NP–FTO, and (c) NW–FTO. |
Moreover, the DRS spectrum of the I2 treated sample on NP–FTO remained unchanged while again with the FTO and NW–FTO sample, the absorption profile, after I2 treatment, resembled that of the fresh sample. The scanning electron micrographs revealed a change in topography of the HOIP phase, Fig. 8. It can be observed that the regenerated HOIP phase on FTO and NW–FTO appears to now consist of non-faceted structures and a contiguous film is observed, similar to that seen in Fig. 2d.
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Fig. 8 Top view scanning electron micrographs of I2 treated HOIP coated on (a) FTO, (b) NP–FTO, and (c) NW–FTO. |
For these initial 44 hours that were monitored, the HOIP phase formed on FTO and NW–FTO appears to consist of larger particles with better crystallinity when compared to the HOIP phase on NP–FTO. Considering that the same method of deposition was employed, it appears that the physical topography of the underlying substrate and its surface roughness imparts a strain on the depositing HOIP phase such that in some cases smooth nanometer sized particles are obtained which are less ordered and more easily prone to degradation. While for the FTO and NW–FTO substrates, these contributed by aiding a much more organized HOIP phase that seems to be able to withstand degradation to a longer extent. These larger particles are perhaps able to withstand the perturbations on the lattice to a larger extent than the relatively nano-sized crystals that formed on the NP–FTO. This observation corroborates the work showcased by Mohite et al.12 and Song et al.13 who have also stated that level of crystallinity is crucial, and large crystalline grain sizes are better able to contribute to structure (and therefore electronic) stability. Although it is not currently clear as to why the particle sizes are bigger on FTO and NW–FTO, however the observation lends itself to the idea that if robust HOIP layers have to be fabricated, rather than forming nanoparticles of HOIP on any given substrate, it is in fact more important to form structurally ordered HOIP crystalline films and such structures appear to be better at enduring any degradation perturbations.
Furthermore, UV light irradiation seems to have a larger detrimental effect on the HOIP when compared to visible light. The different extents of stability of perovskite on the two different kinds of TiO2 used in this study (TiO2 nanowires and P25) within the time frame of the photo-degradation experiment can be explained by the photoactivity of these two different TiO2. TiO2 is a well-known UV photocatalyst, known to degrade organic materials via the formation of reactive oxygen species. P25 is in fact a model photocatalyst because of the co-existence of two phases: anatase and rutile in a specific ratio of 75:
25 which have a synergistic effect on rate of catalysis.14 As such, it can be inferred that this underlying substrate in fact easily photocatalyzes the degradation of the HOIP phase, while in the case of NW–FTO, the sample, although TiO2 in composition, only consists of the rutile phase10 and hence is not expected to be as efficient a photocatalyst. As such, this sample did not degrade as rapidly in the initial 44 hours. To further prove this aspect, two control experiments were performed whereby the P25 phase was replaced with pure anatase and pure rutile phase. Both these phases now consisted of nanometer sized particles similar to P25. Fig. S4† displays the data for the (224) plane's degradation profile and it can be clearly observed that the better the photocatalyst of the underlying substrate, the more prone to degradation is the HOIP deposited phase. Under UV irradiation, both P25 and pure anatase phases seem to augment the rate of HOIP degradation, whereas the pure rutile phase has less of an impact on the degradation rate. Both P25 and anatase are known to be good photocatalysts as compared to rutile.15,16
I2 + H2O ⇆ H+ + I− + HIO, E° = −1.45 V |
Furthermore, in the case of HOIP on NP–FTO, it was observed that extraneous PbI2 formed after the I2 treatment. Lindblad et al. had observed that for HOIPs on TiO2 (using also a two-step deposition technique, akin to that detailed above), the stoichiometry was not only deficient in iodine but also metallic lead was detected by photoelectron spectroscopy.18 Therefore, it can be purported that I2 aids in oxidizing any Pb0 that is known to exist and in turn form PbI2. This can be considered viable considering that the standard oxidation potential of Pb0 is 0.13 V and reduction potential of I2 is 0.54 V.20
Footnote |
† Electronic supplementary information (ESI) available: Surface profile line scans, optical micrographs, XRD profiles in the initial 10 hours of irradiation, FWHM peak data from XRD, and EDX data for I/Pb ratio have been provided. See DOI: 10.1039/c6ra22094k |
This journal is © The Royal Society of Chemistry 2016 |