Dong
Ding
,
Luis
Lanzetta‡
,
Xinxing
Liang‡
,
Ganghong
Min
,
Marcin
Giza
,
Thomas J.
Macdonald
and
Saif A.
Haque
*
Department of Chemistry, Molecular Sciences Research Hub, Imperial College London, London W12 0BZ, UK. E-mail: s.a.haque@imperial.ac.uk
First published on 21st April 2021
Introducing a polymethylmethacrylate (PMMA) layer at the (PEA)0.2(FA)0.8SnI3 perovskite/hole transport layer interface leads to a remarkable improvement in the photogenerated current density and fill factor, resulting in an increase in the power conversion efficiency from 6.5% to 10%. PMMA is proposed to mitigate interfacial charge losses and to induce a more favourable distribution of 2D perovskite phases, elucidating a pathway towards the development of high-performance tin-based perovskite solar cells.
We fabricated a control device based on the following architecture: ITO/PEDOT:PSS/(PEA)0.2(FA)0.8SnI3/PCBM/BCP/Ag. For PMMA-based devices, the PMMA solution was dynamically spin coated onto an ITO/PEDOT:PSS electrode to form a PEDOT:PSS/PMMA heterojunction. The presence of PMMA layers was confirmed via water contact-angle measurements (Fig. S1, ESI†), showing the PMMA-based sample lower wetting (higher angle; 13.9° > 8.9°) due to the hydrophobic character of the polymer. The Sn perovskite film was deposited using a two-step spin coating method from a precursor solution comprising formamidinium iodide (FAI), SnI2, SnF2 and phenylethylammonium iodide (PEAI) in an N,N-dimethylformamide (DMF) and DMSO mixed solvent system.18 The formation of high-quality (PEA)0.2(FA)0.8SnI3 films was confirmed by UV-Visible spectroscopy and X-ray diffraction (XRD) as shown in Fig. S2a and b (ESI†) respectively. These data also indicate that the PMMA layer does not influence the absorption characteristics of the tin perovskite absorber layer. The (PEA)0.2(FA)0.8SnI3 devices were fabricated based on an inverted heterojunction solar cell architecture: ITO/PEDOT:PSS/PMMA/(PEA)0.2(FA)0.8SnI3/PCBM/BCP/Ag as depicted in Fig. 1a. Current density–voltage (J–V) curves of the best performing control and PMMA-based devices are shown in Fig. 1b. The control device yielded a PCE of 6.5% with open circuit voltage Voc = 0.60 V, short circuit current density Jsc = 16.2 mA cm−2 and fill factor FF = 0.67. Upon introduction of the PMMA interlayer at the PEDOT:PSS/perovskite interface, the PCE increased from 6.5% to 10%, which is an improvement of over 53%. This dramatic enhancement in PCE of the PMMA-based device can be mainly attributed to the high Jsc of 22.9 mA cm−2; this being an ∼40% improvement relative to the control device. We note that the PMMA-based device also exhibited an increased FF of 0.73. The integrated photocurrent densities of the control and PMMA-devices obtained from external quantum efficiency (EQE) in Fig. 1c are 16.0 and 22.5 mA cm−2 respectively, which closely match the Jsc values from J–V curves, further confirming the role of PMMA layer in improving the photocurrent density. As can be seen in Fig. 1c, the introduction of the PMMA layer within the device stack improves the EQE across the entire wavelength range (400 to 800 nm). The PMMA-based devices also showed high stability. Fig. 1d shows device performance of the PMMA-based solar cells biased at the maximum power point (MPP) voltage under continuous illumination. The PMMA-based Sn PSCs retained their initial performance after continuous operation for 70 min under one sun illumination. The PCE value increased slightly within the first 5 min of MPP operation, which is most likely due to a light-induced healing in the perovskite layer.19,20 To investigate the shelf stability of the perovskite solar cells, the PCE of PMMA-based device was measured 15 days after fabrication. During this time period, the devices were kept in an inert atmosphere under dark conditions. J–V curves measured on the day of fabrication and after 15 days are shown in Fig. 1d inset. The device shows a small increase in PCE with increasing storage time. This improvement may be attributed to self-healing or the release of crystal strain in the perovskite under dark conditions.21,22
In order to further verify the impact of the thin layer of PMMA on device performance, we fabricated 40 cells for both control and PMMA based solar cells. The box charts of each parameter (Jsc, FF & Voc) are shown in Fig. 2a–d. The PMMA devices show not only high values in each parameter but also great reproducibility relative to the control devices. Device performance statistics for both control and PMMA based solar cells are shown in Fig. S3 (ESI†).
It is pertinent to note that a strict control of the experimental procedures, including fabrication and testing, is essential to achieve the high device performance reported herein. First, the PMMA precursor (0.1 mg mL−1) was spin-coated dynamically at a fast speed (4000 rpm) with the aim of achieving a very thin layer, as we expect PMMA could either form an ultrathin layer where tunnelling effect is strongly dependent on the insulating layer thickness,23 or the carbonyl group on the PMMA could form a network and effectively passivate the perovskite at surface and its grain boundaries.14,24 Second, the fabrication process, including precursor preparation and film synthesis, as well as the testing procedure were carried out carefully in a nitrogen-filled environment to avoid rapid degradation of the Sn-PSC.
We now consider the possible origins of the improved device performance upon the addition of the PMMA interlayer. The increase in Jsc may be rationalised as follows. We studied the microstructure of the (PEA)0.2(FA)0.8SnI3 films with and without PMMA using scanning electron microscopy (SEM; Fig. 3a and b, respectively). Top-view images of the films reveal that their microstructures are similar. However, we note that the PMMA-based Sn perovskite film has slightly better coverage, possibly leading to improved crystallinity; this being consistent with the observed improvement in device performance reported herein. The almost identical absorption and PL characteristics of the perovskite films with and without PMMA interlayers as discussed earlier also suggest that the PMMA layer has negligible impact on the charge generation and separation, and the bulk properties of both samples are very similar. Fig. S4a (ESI†) presents steady-state PL and Fig. S4b (ESI†) presents time-resolved PL for Sn perovskite samples with and without the PMMA layer. Slightly longer fluorescence lifetime is observed in the PMMA sample (with PMMA: τ = 4.03 ns > without PMMA: τ = 3.52 ns); this being consistent with PMMA surface passivation (vide supra). We further hypothesise that the PMMA layer between PEDOT:PSS and Sn perovskite may allow photogenerated holes to tunnel through selectively while blocking electrons as illustrated in Fig. 3d; without the PMMA interlayer, electrons and holes are able to quickly recombine as shown in Fig. 3c. This is expected to reduce interfacial photocarrier recombination and is in agreement with the improvement in Jsc; a similar mechanism has been reported for insulating interlayers for lead-based perovskite solar cells.23 In support of this hypothesis, Lin et al. demonstrated that an ultra-thin layer of PMMA at the perovskite/ETL interface can enable charge injection into the perovskite via tunnelling.25,26 Furthermore, Fig. S5 (ESI†) presents steady-state PL for 2D (PEA)2(FA)n−1SnnI3n+1 Ruddlesden–Popper (RP) phases (where n is the number of octahedra sheets per 2D layer) in Sn perovskite samples with and without PMMA; a small increase in PL intensity in both sample sides (i.e. glass and film sides) is observed in the sample with PMMA, indicating a larger amount of 2D phases. This may be indicative of a more favourable 2D phase distribution in the film, allowing unrestricted charge transport in the perovskite layer and hence leading to the observed higher Jsc. The enhanced EQE in the PMMA-based cell (Fig. 1c) presents a new feature at ∼685 nm, which is attributed to the n = 2 RP phase. This further supports the role of 2D perovskite distribution in the increase of Jsc and device performance. We note that further detailed studies are underway to establish the exact mechanism by which PMMA improves device performance and will be reported in future work.
In summary, we fabricated 10.0% efficient (PEA)0.2(FA)0.8SnI3 perovskite solar cells with high reproducibility and we demonstrated that the insertion of an insulating PMMA layer at HTL/Sn-PSC interface could dramatically improve Jsc and FF. We note that our PMMA-based (PEA)0.2(FA)0.8SnI3 devices exhibited a ∼40% improvement in Jsc and, overall, a ∼53% increase in PCE relative to control solar cells. However, there is still room to improve the device performance, especially via increasing Voc. The work presented herein based on the use of ultrathin PMMA layers shows a promising, broadly applicable, and cost-effective direction towards the further development of highly efficient Sn-PSC solar cells.
Footnotes |
† Electronic supplementary information (ESI) available: Experimental details, Fig. S1–S8. See DOI: 10.1039/d0cc07418g |
‡ These authors contributed equally. |
This journal is © The Royal Society of Chemistry 2021 |