Influence of Reactant Stoichiometry on Morphology and Structure of CH3NH3PbI3 Perovskite Films
Abstract
The structural and morphological evolution of CH3NH3PbI2.98Cl0.02 thin films was systematically examined as a function of the molar ratio of the precursor solutions (PbI2 : CH3NH3I + CH3NH3Cl). A stoichiometric 1:1 ratio of PbI2 to CH3NH3I yields a perovskite phase between 70–80 °C, whereas temperatures above 120 °C initiate thermal degradation. When the MAI excess is increased to 2 or 3, intermediate lead‑halide phases—(CH3NH3)2PbI4 and (CH3NH3)3PbI5—form before the final perovskite emerges. Importantly, the Pb/I ratio remains constant across all compositions, indicating that variations in film performance are governed by particle shape anisotropy, as corroborated by SEM and XRD data.
Background
Solar photovoltaics have shifted from silicon and II–VI compounds to organic‑inorganic perovskites (OIP) due to their rapid power‑conversion efficiency (PCE) gains—from ~3.4 % in 2004 to 23.3 % in 2018 (22.6 % certified) [8–10]. OIP’s high absorption, long carrier diffusion lengths, and direct bandgap enable ultra‑thin active layers, reducing cost and material usage [7,18]. However, their intrinsic instability—sensitivity to moisture, oxygen, heat (>100 °C), and UV light—poses a major challenge, as MAI volatilization leaves PbI2 residues [20–25]. Understanding the precise role of precursor stoichiometry is therefore essential for engineering robust, high‑performance perovskite solar cells.
Despite extensive research on MAPbI3 crystallization, the influence of non‑stoichiometric precursor ratios on film microstructure and phase evolution remains underexplored. Previous work has shown that a slight MAI excess improves film density and device performance, yet the mechanistic pathways—particularly the emergence of intermediate lead‑halide phases—are not fully resolved [16,32]. This study addresses this gap by combining Raman spectroscopy, X‑ray powder diffraction (XRPD), and scanning electron microscopy (SEM) to trace phase formation and morphological changes across a systematic range of PbI2 : CH3NH3I ratios.
Methods
Synthesis
Lead iodide (PbI2), methylammonium chloride (CH3NH3Cl), and pre‑synthesized methylammonium iodide (MAI) served as precursors. A 2 % molar amount of CH3NH3Cl relative to MAI was added to partially substitute iodine with chlorine, enhancing perovskite stability [16,34]. Dimethylformamide (DMF) was the solvent of choice. Precursor solutions were stirred at 70 °C for 1 h, then spin‑coated (1200 rpm, 30 s) onto cleaned glass or FTO/glass substrates in a nitrogen glovebox. Thermal annealing ranged from 70–180 °C for 30 min on a preheated hot plate.
Characterization
SEM imaging (SEC miniSEM SNE 4500 MB) and EDX spectroscopy assessed morphology and composition. XRPD (DRON‑4‑07, CuKα, 40 kW, 18 mA) collected 2Θ = 10–120°, step 0.04°, count 4 s; Rietveld refinement extracted lattice parameters. Raman spectra were recorded with 532 and 671 nm lasers; excitation power was minimized (< 5×102 W/cm2) to prevent photodegradation.
Results and discussion
Solution Chemistry
Raman spectra (Figure 1) reveal that mixing PbI2 with MAI in DMF induces the formation of lead polyiodide species (e.g., [PbI3]−, [PbI4]2−), evidenced by a shifting Pb–I mode from 114 to 121 cm−1 as MAI concentration increases. This shift correlates with the red‑shift of the optical absorption edge from 2.54 eV (pure PbI2) to 2.24 eV (1:3 mixture), confirming enhanced iodide coordination. The presence of 2 % CH3NH3Cl introduces additional Raman bands (e.g., 953, 997 cm−1) that are negligible in the final perovskite solutions due to the low chlorine content.
Film Morphology
SEM images (Figure 2) show that MAI‑only films form smooth, glass‑like surfaces with minor heterogeneities, whereas PbI2 films exhibit elongated, wire‑like grains that grow anisotropically at 90 °C. Perovskite films (Figure 3) exhibit pronounced particle anisotropy at a 1:1 ratio—needle‑like grains dominate. Increasing MAI excess to 1:2 yields maple‑leaf‑shaped particles with multiple growth directions; at 1:3 the grains become smaller and the film appears denser, reflecting the suppression of anisotropic growth by excess organic cations.
Phase Evolution
XRPD patterns (Figure 4) confirm that a stoichiometric 1:1 ratio produces a single‑phase MAPbI3 between 70–80 °C. Higher temperatures (>120 °C) introduce PbI2 peaks, indicating thermal decomposition per the reaction:
$$\mathrm{CH}_3\mathrm{NH}_3\mathrm{PbI}_3\overset{>80^{\circ}\mathrm{C}}{\to}\mathrm{PbI}_2+\mathrm{CH}_3\mathrm{I}\uparrow+\mathrm{NH}_3\uparrow$$
For a 1:2 ratio, an intermediate (CH3NH3)2PbI4 forms below 180 °C, which subsequently converts to MAPbI3 upon further heating. Similarly, the 1:3 ratio first yields (CH3NH3)3PbI5 and (CH3NH3)2PbI4 before the final perovskite crystallizes. The orthorhombic, tetragonal, and cubic phases of MAPbI3 are well documented; in all tested samples the tetragonal phase (I4/mcm) dominates, as evidenced by the split (220)/(004) peaks (Figure 5).
Raman Spectroscopy
Raman spectra (Figure 6) show that films derived from 1:1, 1:2, and 1:3 mixtures possess identical tetragonal perovskite signatures. However, prolonged laser irradiation (200–400 s) or elevated excitation power causes spectral shifts indicative of a transition toward a metastable PbI2‑rich state, ultimately leading to complete decomposition at higher fluences. This laser‑induced sensitivity underscores the necessity for careful handling during spectroscopic studies.
Additional Raman experiments on 1:3 films annealed up to 180 °C (Figure 7) reveal that the metastable phase is retained at the highest temperature, aligning with the XRPD evidence of perovskite decomposition.
Conclusions
The study demonstrates that tailoring the PbI2 : MAI ratio in DMF solution allows precise control over perovskite film morphology and phase evolution. A 1:1 stoichiometry yields a stable MAPbI3 phase at 70–80 °C, whereas higher MAI excess induces intermediate lead‑halide phases that ultimately transform into MAPbI3 upon annealing. The Pb/I stoichiometry remains constant across all compositions; therefore, variations in device‑relevant properties arise from anisotropic grain growth rather than elemental composition. Raman spectroscopy confirms the susceptibility of perovskite films to laser‑induced degradation, with a metastable transition to PbI2 preceding complete decomposition.
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