Surface passivation engineering strategy to fully-inorganic cubic CsPbI3 perovskites for high-performance solar cells

Owing to inevitable thermal/moisture instability for organic–inorganic hybrid perovskites, pure inorganic perovskite cesium lead halides with both inherent stability and prominent photovoltaic performance have become research hotspots as a promising candidate for commercial perovskite solar cells. However, it is still a serious challenge to synthesize desired cubic cesium lead iodides (CsPbI3) with superior photovoltaic performance for its thermodynamically metastable characteristics. Herein, polymer poly-vinylpyrrolidone (PVP)-induced surface passivation engineering is reported to synthesize extra-long-term stable cubic CsPbI3. It is revealed that acylamino groups of PVP induce electron cloud density enhancement on the surface of CsPbI3, thus lowering surface energy, conducive to stabilize cubic CsPbI3 even in micrometer scale. The cubic-CsPbI3 PSCs exhibit extra-long carrier diffusion length (over 1.5 μm), highest power conversion efficiency of 10.74% and excellent thermal/moisture stability. This result provides important progress towards understanding of phase stability in realization of large-scale preparations of efficient and stable inorganic PSCs. Inorganic cesium lead iodide perovskite is inherently more stable than the hybrid perovskites but it undergoes phase transition that degrades the solar cell performance. Here Li et al. stabilize it with poly-vinylpyrrolidone and obtain high efficiency of 10.74% with excellent thermal and moisture stability.

D ue to suitable direct bandgap, high absorption coefficient, and extra-long carrier diffusion length, excellent optoelectronic property, simple and reproducible solution/ vapor-chemistry processing 1-3 , organic-inorganic hybrid halide perovskite materials (ABX 3 , A=CH 3 NH 3 , B=Pb, X=Br, I) have been deemed as a promising candidate for light harvester for next-generation high-performance solar cells [4][5][6][7][8] . Despite great progress in photovoltaic performance in the last few years, commercial application of perovskite solar cell (PSC) still suffers from moisture and thermal instability owing to the degradation and volatilization of organic component, which presents the uppermost obstacle in further development and mass production 9 . For this reason, all inorganic halide perovskite formed by substituting the organic cation with cesium (Cs) is an optimal alternative for its native inorganic structure stability, and has demonstrated equally efficient and more stable compared to organic-inorganic halide perovskites [10][11][12][13] .
Of the various inorganic lead halide perovskites, especially, cesium lead iodide (CsPbI 3 ) in cubic phase (α phase) with a bandgap of around 1.73 eV and a visible-light-absorption spectrum up to 700 nm is the mostly desired light harvester in solar cells [14][15][16] . However, cubic CsPbI 3 can only keep stable at high temperature of above 300°C 14 . As temperature decreasing to ambient temperature, CsPbI 3 suffers from thermodynamically phase transition to undesired orthorhombic phase (δ phase) with a wide bandgap of 2.82 eV (Supplementary Figure 1), exhibiting an extremely poor photovoltaic conversion efficiency (PCE) of only 0.09% in PSC 17 . To overcome this obstacle, composition engineering which pursues a certain amount of bromide (Br) to substitute iodide (I) can be one of efficient methods by balancing the tolerance coefficient between PbX 6 octahedron and Cs ions [18][19][20] . For example, Sutton et al. 18 developed a full set of cesium lead halide films from CsPbBr 3 to CsPbI 3 , demonstrating a stabilized power output of 5.6% and J-V efficiency reaching 9.8% for PSC based on cubic CsPbI 2 Br, although CsPbI 2 Br still reverts to δ phase over prolonged exposure in air. Increasing continuously bromide proportion induces more prominent phase stability/moisture-stability, dispiritingly, which brings Brwidened bandgap near or above 2.0 eV compared with the ideal solar spectrum (from 1.1 eV to 1.7 eV) 21 . Another effectual method to stabilize cubic phase CsPbI 3 is synthesizing colloidal quantum dots (CQDs) with well-controlled size via hot injection process, and best-performance CsPbI 3 solar cells are achieved by assembling cubic phase CsPbI 3 CQDs as photoactive layer [22][23][24][25] . Unfortunately, the undesired α-to-δ phase transition of Cs-based inorganic perovskite has not been inhibited in the solutionchemistry processed film. It is of great and fundamental challenge to develop effective and facile route to synthesize cubic Cs-based inorganic perovskite film for high-performance PSC for potential large-scale industrial application.
Herein, poly-vinylpyrrolidone (PVP)-induced surface passivation strategy is reported to stabilize inorganic perovskite CsPbI 3 with cubic crystal structure via a reproducible solution-chemistry reaction process. The surface chemical state of cubic CsPbI 3 crystals synthesized in the presence of PVP is investigated via Fourier transformed infrared (FTIR) and nuclear magnetic resonance (NMR) techniques, demonstrating that decreased surface tension can be conducive to stabilize cubic CsPbI 3 even in large scale of film with micrometer scale, due to enhanced electron cloud density on the surface of CsPbI 3 originated from chemical bonding between acylamino group in PVP and CsPbI 3 . The obtained cubic CsPbI 3 exhibits extra-long carrier lifetime of 338.7 ns and diffusion length of greater than 1.5 μm, up to an order of magnitude compared to the active layer depth. The fabricated PSCs based cubic CsPbI 3 achieves the highest power conversion efficiency of 10.74% and excellent thermal/moisture stability.

Results
PVP-induced cubic phase stability studies. The specific cubicphase CsPbI 3 films were prepared via a simple and reproducible one-pot solution spin-coating process using a mixture of CsI, PbI 2 , and PVP as a precursor. X-ray diffraction (XRD) patterns of the CsPbI 3 films coated on the F-doped SnO 2 (FTO) substrates present the difference in the presence and absence of PVP. In the one-pot solution process without PVP, the CsPbI 3 film exhibits a prompt transition from cubic phase to orthorhombic phase when prolonging anneal time or cooling to room temperature, as shown in the XRD pattern (black line) in Fig. 1a and the photograph in Fig. 1b. After adding PVP and gradually increasing the concentration to 10 wt%, the CsPbI 3 can keep stable cubic phase both at high and room temperature, even stable at exceeding 80 days (Fig. 1a, b; Supplementary Fig. 2). Similarly, the prominent phase stability is demonstrated achievable in full series of inorganic perovskite compositions from CsPbI 3 to CsPbBr 3 shown in Supplementary Figures 3 and 4.
We further fabricate CsPbI 3 film on mesoporous TiO 2 via onestep solution spin-coating process with different PVP concentrations. As shown in SEM images of Fig. 1c, d, both orthorhombic and cubic CsPbI 3 exhibit high-surface coverage. Compared with irregular grain size distribution of orthorhombic ones, the obtained PVP-induced cubic CsPbI 3 film presents a dense grained uniform morphology with comparatively small grain size of around 100 nm. The cross-section morphology of the fabricated solar device architecture is shown in Fig. 1e, consisting mainly of two uniform layers containing a 400 nm mesoporous TiO 2 /CsPbI 3 nanocomposite film and a 100 nm pure CsPbI 3 perovskite overlayer. It is shown that the inorganic perovskite materials are fully permeated into TiO 2 mesoporous layer, forming a very uniform overlayer with 100% coverage. Intriguingly, tuning anneal time range, the spin-coating obtained CsPbI 3 exhibits crystalline size of over 1 μm and high-crystalline with cubic phase structure (Supplementary Figs. 5, 6 and 7), which is different from the previous reports involving of phase transition of perovskite materials in large grain size 22 .
In order to gain insight into the PVP stabilization mechanism on cubic CsPbI 3 , we examine the infrared transmittance spectra of CsPbI 3 films (Fig. 2a) for pure PVP, CsPbI 3 film synthesized in the presence of PVP, and the CsPbI 3 film after removing PVP washed with isopropanol (IPA). The IR spectrum of pure PVP shows absorption bands in the region of 1668, 1421, and 1297 cm −1 , which are attributed to typically functional groups of C=O, C-H, and C-N stretching vibration in acylamino of PVP, respectively 26,27 . For the IR spectrum of the CsPbI 3 film synthesized in the presence of PVP, these characteristic vibrations are still persisted, but only blue-shifting to 1652 cm −1 for the C=O stretching, and 1282 cm −1 for the C-N stretching, respectively, indicating an interaction effect between functional groups of PVP and precursor ions of CsPbI 3 . For the CsPbI 3 film washed with IPA, characteristic bands for C=O, C-N, and C-H stretching decreases considerably in terms of intensity, while it remains at the same location. A similar binding energy variation of CsPbI 3 surface elements can be found in X-ray photoelectron spectroscopy (XPS) measurements in Supplementary Figure 9. The variation tendency demonstrates that PVP is not only absorbed on the surface of CsPbI 3 physically, but also functions chemically in formation and stabilization of cubic CsPbI 3 through N-C=O bond of acylamino group 27 .
On the basis of the above IR information, it is indicated that acylamino group of PVP plays a dominant role on the nucleation and growth of cubic CsPbI 3 perovskite film. For further understanding this specific effect of acylamino group of PVP, the liquid-state 1 H/ 13 C NMR measurement is conducted on pure PVP samples and CsPbI 3 perovskite synthesized in the presence In 1 H NMR spectra ( Fig. 2b) of neat PVP sample, resonance signals attributed to the acylamino group appear at δ = 2.5 and 3.35 ppm, which are characteristic of CH 2 attached to C=O group and N atom, respectively 28 . The interaction of unique groups in PVP with precursor ions of CsPbI 3 induces a downfield chemical shift of Δδ ≈ 0.5 ppm for CH 2 adjoining with acylamino group. Reversely, almost no variation for the resonances of hydrogen in backbone chain appears. This can be rationally explained in terms of strengthening effects of resonance for organic constituents through the interaction between cesium cations of perovskite and atoms in organic molecules of PVP, reflecting on the shift of chemical resonances 29 . Moreover, the result indicates that the N and O atoms in acylamino group are jointly responsible for the chemical shift and can be as two possible centers for coordination with cesium ions. Furthermore, 13 C NMR spectroscopy in Fig. 2c show that resonance signal of δ = 175 ppm arising from C=O group undergoes a significant downfield shift of Δδ ≈ 2 ppm on interaction of PVP with CsPbI 3 , which is indicative of the coordination-bonding interaction between oxygen atoms of acylamino group and cesium ions in perovskite 30 . In contrast, the resonances at δ = 41 and 43 ppm for C(1)H 2 and C(α)H attached to nitrogen atoms exhibit slight chemical shift. Such variation of PVP molecule structure further confirms that there exist two potential centers, i.e. the nitrogen and the carbonyl oxygen, interacting with Cs + ions of perovskite exposed 31 . Moreover, the oxygen in acylamino group occupies a dominate position in the formation of C=O···Cs bonds, since nitrogen in planar conformation of internal amide can only have relatively weak influence. A conceivable PVP-induced surface tension-driven mechanism for the formation of stable cubic phase CsPbI 3 is proposed based on the above experiment facts. It is known that the acylamino group in N-vinylpyrrolidone molecule of PVP has donated lone pairs related to oxygen and nitrogen atoms, which offer a large number of coordination centers. As shown in Fig. 3a, the coordination modus indicates the polymer molecules coordinate onto the surface of CsPbI 3 through the oxygen atoms, to a lesser extent, via the nitrogen of N-C=O groups, resulting in a weakening of the C=O bonding and an increasing of N-C bond. At the initial stage (Fig. 3b), PVP molecules initiate to attract cations of CsPbI 3 precursors due to long backbone chain and electronegative acylamino group structure. The positive and negative ions of CsPbI 3 tend to assemble and bond to form cubic CsPbI 3 a metastable state around the N-C=O coordination centers of PVP. With time increasing, more nuclei of CsPbI 3 are promptly launched with PVP attached. The PVP molecules, in the meantime, stabilize the CsPbI 3 nanocrystals from aggregation owing to the intermolecular rejection effect, as shown in Fig. 3c. For the grown CsPbI 3 nanocrystals, long-chain PVP molecules with a large number of acylamino groups anchored at the surface of CsPbI 3 provide more coordination polymer units for interactions between oxygen, nitrogen in acylamino and cesium ions of inorganic perovskite. With the growth of CsPbI 3 stabilized with PVP, the interactions between N-C=O of acylamino and Cs + of inorganic perovskite exposed at the surface are enhanced, contributing increasing negative field in Cs + -PVP complex on the surface of CsPbI 3 (Fig. 3d), which results in the enhancement of the electron cloud for Cs + of CsPbI 3 26,32 . According to study by Grätzel's group that the surface free energy is a function of the surface tension 33 . While the surface tension is related to charge density 34 . An increase in charge density decreases the surface tension. Therefore, in the CsPbI 3 -PVP complex, the increase in the electron cloud density may result in low surface tension, thus greatly reduces the surface energy of CsPbI 3 . As a result, the cubic CsPbI 3 can be maintained at ambient temperature. Furthermore, cubic structure of CsPbI 3 can even be still maintained after 80 days for the PVP chemically functionalized CsPbI 3 . Owing to the increase of surface charge originated from the interaction between PVP and CsPbI 3 , the surface tension of CsPbI 3 grains reduced significantly, which plays an essential role in the stabilization of cubic phase CsPbI 3 .
Optical and photovoltaic performance. Weighing the phase stability and power conversion efficiency (Supplementary Figs. 8,14,15 and 16), the optimal synthetic condition (10 wt% of PVP, 5 min annealing, and 30 min IPA treatment) was selected and applied for the following optical, electrical and photovoltaic investigation. Figure 4a presents the ultraviolet-visible absorption spectra of the obtained cubic and orthorhombic phase CsPbI 3 films. The orthorhombic CsPbI 3 exhibits limited visible-lightabsorption range less than 450 nm, demonstrating that it is unsatisfactory as an optical active material for solar devices. Oppositely, the cubic CsPbI 3 shows a desired absorption width to 700 nm, nearly covering full visible-light region. Furthermore, we investigate the effect of anneal time (crystalline grains) on the optical properties and carry out the PL measurement of cubic CsPbI 3 perovskite films. The result shows that, tuning size of cubic CsPbI 3 grains, the emission peaks red-shift gradually until to a constant value of around 710 nm (Supplementary Fig. 10).
The time-resolved photoluminescence (TRPL) measurement ( Fig. 4b; Supplementary Figure 18) is conducted to investigate the carrier lifetime of cubic and orthorhombic CsPbI 3 films. To eliminate the effect of quenching treatment, the CsPbI 3 films are deposited on glass slides under the same solution-method and the same thickness. The corresponding steady-state PL spectra of cubic and orthorhombic CsPbI 3 films are shown in in which n(x,t) is the number of excitations within a certain thickness of perovskite film, k(t) is the PL decay rate without quenching layer, and D is the diffusion coefficient. Table 1 shows the carrier diffusion length for both orthorhombic and cubic CsPbI 3 films, which depends on electron or hole quenching layer used, and it is assumed that all photogenerated carriers reach the quenching interface. It is clear the diffusion length of both electron and hole in orthorhombic CsPbI 3 film is around 120 nm. However, for cubic CsPbI 3 film, the carriers exhibit a diffusion length for electrons over 1 μm, and even over 1.5 μm. As reported (Supplementary Table 1), the average carrier diffusion length in organic-inorganic hybrid perovskites MAPbI 3 and FAPbI 3 is 129 and 813 nm, respectively 1,8 . In addition, in pure/mixed Br based inorganic perovskite, the carrier diffusion length is less than 200 nm 12 . The ultra-long carrier diffusion length not only originates from the excellent carrier transport capability of cubic CsPbI 3 , but also from the inhibition of defect recombination via the surface passivation effect, which provides the feasibility in planarstructure PSCs or even thicker light-absorption layers.
On the basis of optical and carrier transport properties, we conduct the photovoltaic measurements of the cubic CsPbI 3 PSCs fabricated with mesoporous TiO 2 scaffold. Of the solar devices acquired, Fig. 4d Table 2) 18,19,35 . Moreover, the stability of J sc and PCE for both devices is shown in Supplementary Figure 19. The cubic CsPbI 3 device shows a stable output with a J sc of 13.1 mA cm −2 and a PCE of 10.0%. The corresponding incident photo-to-current efficiency (IPCE) spectrum in Fig. 4c for the best cell exhibits a broad plateau of over 60% between 350 and 700 nm. The integrated J sc of 14.7 mA cm −2 is in good agreement with the current density acquired from the current-voltage measurement. Intriguingly, compared with other inorganic PSCs 18,19,35 , the CsPbI 3 based solar cell exhibits a much higher J sc , which can be attributed to the extended visible-lightabsorption range and extra-long carrier diffusion length for CsPbI 3 , beneficial to more photoelectrons/hole generations and captures by corresponding transport layers. Moreover, the PVP covered on CsPbI 3 grains decreases surface defects and suppresses nonradiative recombination, significantly (Supplementary Figure 17). Figure 4e shows a histogram of average PCEs from all of the cubic CsPbI 3 PSCs fabricated under the same condition for the repeatability purpose. Over 70% of the devices exhibit over 8% PCE, and the average PCE summarized shows 8.50%, which is better than most current stable and efficient CsPbI 2 Br perovskite cells (Supplementary Figure 20).
Moisture and thermal stability. The excellent stability of PSCs is an essential factor for the reproducibility and commercial application. To investigate the moisture and thermal stability under different conditions, the performance of inorganic cubic perovskite (CsPbI 3 ) PSCs with average PCE is comparatively measured with that of solar cells based on typical organic-inorganic hybrid perovskite (MAPbI 3 ). The ambient-humidity-stability test was conducted under ambient condition for 500 h without encapsulation (average humidity of 45-55% with temperature of 26°C fixed). Fig. 5a shows the device moisture-stability as a function of aging time in terms of normalized power conversion efficiency (PCE). During 500 h, the cell of MAPbI 3 shows a dramatic drop with 70% efficiency loss with respect to the fresh solar cell. Comparatively, cubic CsPbI 3 based device exhibits a better moisture-stability with 75% retention after 500 h. Figure 5b shows the thermal-stability measurement of PSCs with cubic CsPbI 3 and MAPbI 3 , which was conducted at different temperature ranging from 20 to 100°C. It is clear that, with the increasing of temperature, the inorganic cubic perovskite exhibits more prominent thermal stability, showing over 90% efficiency retention even at 80°C. It is worth noting that, as increasing the temperature to 100°C, the devices of both CsPbI 3 and MAPbI 3 show obvious decay in PCE, which might result from the failure of the organic hole transport material. For further investigating the long-term thermal stability of the inorganic perovskite CsPbI 3 solar cell, we measured the device performance as stored at high temperature (60°C) under normal sunlight exposure, which is shown in Fig. 5c. During 500 h measurement, the cubic CsPbI 3 based PSC shows a slight efficiency decay of only around 10%, demonstrating an outstanding superiority in thermal stability compared to MAPbI 3 based solar cell (70% efficiency loss). Notably, the thermal-stability efficiency test for inorganic perovskite exhibits a slower decay rate than the humidity stability. The result demonstrates that the CsPbI 3 inorganic perovskite possesses more outstanding stability, especially in thermal stability.

Discussion
In summary, we developed a surface passivation engineering for preparing long-term stable cubic phase CsPbI 3 films via a reproducible solution-chemistry process with the assistant of PVP. We proposed a plausible mechanism for the formation of stable cubic CsPbI 3 by investigating the surface chemical states of the perovskite crystals. The decreased surface tension can be obtained to stabilize CsPbI 3 grains in cubic phase even in micrometer scale, due to electron cloud density enhancement on the surface of CsPbI 3 originated from chemical bonding between acylamino in PVP and CsPbI 3 . Furthermore, we found the a Efficiency evolution of the devices exposed in ambient air under relative humidity of 45-55% without any sealing. The measurements were carried every 50 h during 500 h. b Efficiency variation as a function of temperature from 20 to 100°C. The PCEs were measured under nitrogen atmosphere after an equilibration time of 30 min at each temperature setting. c Efficiency evolution of the cells in a nitrogen atmosphere at 60°C during 500 h obtained cubic CsPbI 3 exhibits prominent photoelectronic properties with extra-long carrier lifetime of 338.7 ns and diffusion length of greater than 1.5 μm, up to an order of magnitude compared to the absorption depth. Based on this strategy, we have achieved the highest PCE of 10.74%, as well as excellent thermal/moisture stability in the fabricated inorganic PSCs. This result provides important progress towards the understanding of phase stability in the realization of large-scale preparations of efficient and stable inorganic PSCs.

Methods
Inorganic perovskite film preparation. A certain amount of PVP (Aladdin, K13-18) was first dissolved in mixed solvent with DMF (Aladdin, 99.9%) and DMSO (Aladdin, anhydrous) (1:1) and stirred for 30 min at room temperature. The CsPbI 3 precursor solution (0.8 M) was synthesized by dissolving stoichiometric CsI (Aladdin, 99.9%) and PbI 2 (Aladdin, 99.9%) in above solution, then, was stirred at 90°C for 1 h on hot plate. The perovskite precursor solution was spin-coated on glass substrate or mesoporous TiO 2 film at 2500 rpm for 45 s and sintered at 300°C for 5 min to form CsPbI 3 film. The other series of cesium lead halide perovskite films with different iodide/bromide proportions were synthesized by changing the percentage of PbI 2 and PbBr 2 , and keeping other methods fixed.
Device fabrication. A compact TiO 2 layer (about 50 nm) was deposited on the FTO substrates (OPV Tech) which were ultrasonically washed and underwent oxygen plasma treatment by spin-coating a mildly acidic solution of titanium isopropoxide in ethanol (2000 rpm, 30 s), and annealed at 500°C for 30 min. A 400-500 nm thick mesoporous TiO 2 film was coated on the compact layer via TiO 2 paste (2500 rpm, 45 s), next, heated for 30 min at 500°C. Then, the CsPbI 3 active layer was deposited on mesoporous TiO 2 scaffold with 300°C annealing treatment for 5 min. To increase the surface coverage of the inorganic perovskite, the substrates with TiO 2 coated were preheated at 150°C. After cooling to room temperature, the substrates were immersed into IPA for 30 min to remove redundant PVP. Finally, an around 200 nm hole transport layer of spiro-OMeTAD (OPV Tech, 99.5%) was spin-coated at 2500 rpm for 30 s and a 50 nm gold counter electrode was prepared by thermal evaporation. The optical active layer and hole transport layer were fabricated in glove box.
Characterization. The XRD spectra of inorganic perovskite films were measured by Phillips Rigaku D/Max-kA X-ray diffractometer. The surface-section/crosssection morphologies of the perovskite films were characterized using fieldemission scanning electron microscopy (FESEM, SU-70). The high-resolution transition electron microscope (HRTEM, Phillips, Tecnai 20U-Twin) was applied to analyze the structures and morphologies of the perovskite crystalline grains. The ultraviolet-visible absorption spectra of the perovskite films were recorded on the TU-1901 spectro-photometer. The FTIR spectra (NEXUS 670) were used to measure the surface functional group of the films. The liquid-state NMR were conducted by VNMRS 600. The XPS measurement was carried out using the Escalab 250Xi electron spectrometer via monochromatized Al Kαradiation (hν = 1486.7 eV). The TRPL measurement were carried by FLS920 all functional fluorescence spectrometer (Edinburgh) with an excitation wavelength of 400 nm. The photovoltaic performances (J-V curves) were analyzed by a solar simulator (Newport, Class 3 A, 94023 A) set an AM 1.5 G simulated sunlight (100 mW cm −2 ) equipped with a Keithley 2420, and the solar cells were measured using a metal aperture to define the active area to be around 0.09 cm 2 . The IPCE was characterized using a power source (Newport 300 W xenon lamp, 66920) equipped with a monochromator (Newport Cornerstone 260) and a multimeter (Keithley 2400) at 100 mW cm −2 , AM 1.5 G illumination, and was corrected by a calibrated Sireference cell (NREL).