AUG 6, 202650 MINS READ
Narrow bandgap perovskite materials are predominantly based on mixed Sn-Pb compositions that enable bandgap tuning below the 1.5 eV threshold of pure lead-based perovskites. The archetypal narrow bandgap perovskite adopts the general formula (FAxMA1-x)(SnyPb1-y)I3, where formamidinium (FA) and methylammonium (MA) occupy the A-site, while tin and lead share the B-site in the ABX3 perovskite structure 1. The incorporation of Sn2+ (ionic radius ~1.35 Å) alongside Pb2+ (1.49 Å) contracts the lattice and reduces the bandgap through modification of the conduction band minimum, which is primarily derived from metal p-orbitals 11. Representative compositions such as (FASn I3)0.6(MAPbI3)0.4 achieve bandgaps near 1.25 eV, positioning them ideally for bottom subcells in all-perovskite tandem configurations 1.
The structural integrity of narrow bandgap perovskite material is enhanced through quasi-2D/3D composite architectures. Introduction of large organic cations such as phenethylammonium (PEA+) and guanidinium (GA+) into the precursor solution induces formation of a quasi-2D perovskite-like phase with stoichiometry (PEA)2GAPb2I7, which becomes dispersed within the continuous 3D perovskite matrix 1. This composite morphology creates a heterogeneous energy landscape where the quasi-2D phase (wider bandgap ~2.0–2.3 eV) passivates grain boundaries and suppresses ion migration, while the 3D phase (narrow bandgap ~1.25 eV) serves as the primary photoactive component 1. X-ray diffraction analysis confirms retention of the cubic perovskite structure (space group Pm-3m) with characteristic (100), (200), and (220) reflections, alongside additional low-angle peaks corresponding to the layered quasi-2D phase 1.
Key structural parameters influencing narrow bandgap perovskite material performance include:
The chemical formula A1-xFAxSn1-yBy(I1-zXz)3 (where A = Cs, GA, or MA; B = Pb; X = Br or Cl; 0.5 ≤ x ≤ 0.9, 0.5 ≤ y ≤ 0.9, 0 ≤ z ≤ 1) provides a comprehensive framework for narrow bandgap engineering 11. Cesium incorporation (typically 10–30 mol%) enhances thermal stability by increasing the average A-site cation radius and strengthening the perovskite framework against moisture-induced degradation 11. The bandgap can be systematically tuned from 1.1 eV to 1.5 eV by adjusting the Sn:Pb ratio, with the relationship approximately following Vegard's law: Eg(y) ≈ 1.17 + 0.40y eV 1112.
The fabrication of high-quality narrow bandgap perovskite material demands stringent control over precursor chemistry, deposition kinetics, and post-treatment protocols to mitigate the inherent instability of Sn2+ oxidation. The predominant synthesis approach employs solution-based spin-coating with anti-solvent engineering, which enables rapid crystallization and uniform film formation 12.
A typical precursor formulation for (FASn I3)0.6(MAPbI3)0.4-based narrow bandgap perovskite material involves dissolving stoichiometric quantities of FAI, MAI, SnI2, and PbI2 in a mixed solvent system of dimethylformamide (DMF) and dimethyl sulfoxide (DMSO) at a 4:1 volume ratio 17. The total perovskite concentration ranges from 1.0–1.5 M to achieve film thicknesses of 400–600 nm after spin-coating 1. Critical additives include:
All solution preparation must occur in an inert atmosphere (N2 or Ar glovebox, O2 < 0.1 ppm, H2O < 0.1 ppm) to prevent premature Sn2+ oxidation 111.
The optimized deposition sequence for narrow bandgap perovskite material comprises:
The anti-solvent treatment is critical for achieving dense, pinhole-free films with controlled crystallite size. Chlorobenzene extraction of DMF/DMSO creates a supersaturated intermediate phase that crystallizes uniformly during annealing, whereas delayed or omitted anti-solvent application results in large, isolated grains with poor surface coverage 1.
Recent innovations in narrow bandgap perovskite material synthesis include:
For quasi-2D/3D composite narrow bandgap perovskite material, the molar ratio of PEAI:GASCN typically ranges from 1:1.5 to 1:2, with total additive concentration not exceeding 10 mol% to avoid excessive quasi-2D phase formation that would impede vertical charge transport 1.
The defining characteristic of narrow bandgap perovskite material is its extended absorption onset into the near-infrared region, enabling photocurrent generation from photons with wavelengths up to 900–1000 nm. High-quality (FASn I3)0.6(MAPbI3)0.4 films exhibit an absorption coefficient exceeding 104 cm-1 at wavelengths below 800 nm, comparable to GaAs and superior to crystalline silicon in the visible range 111.
The bandgap of narrow bandgap perovskite material can be precisely controlled through compositional variation:
Tauc plot analysis of UV-Vis absorption spectra confirms direct bandgap transitions in optimized narrow bandgap perovskite material, with absorption edges exhibiting sharp onsets (Urbach energy <15 meV) indicative of low energetic disorder 111.
Time-resolved photoluminescence (TRPL) and transient absorption spectroscopy reveal exceptional carrier lifetimes in state-of-the-art narrow bandgap perovskite material:
Photoluminescence quantum efficiency (PLQE) of narrow bandgap perovskite material on glass substrates reaches 1–3%, lower than wide-bandgap analogues (10–20% for FAPbI3) due to increased non-radiative recombination from Sn-related defects, but sufficient for photovoltaic applications where radiative efficiency limits are less stringent 111.
Four-point probe conductivity measurements and space-charge-limited current (SCLC) analysis provide insights into charge transport:
The reduced trap density directly translates to higher open-circuit voltages (Voc) in photov
| Org | Application Scenarios | Product/Project | Technical Outcomes |
|---|---|---|---|
| Alliance for Sustainable Energy LLC | Bottom subcells in all-perovskite tandem solar cells requiring narrow bandgap (1.25 eV) absorbers for efficient near-infrared light harvesting and maximized current matching. | Narrow-bandgap Sn-Pb Perovskite Solar Cells | Achieved ~22.1% efficiency with open-circuit voltage >0.91V through quasi-2D/3D composite engineering using PEAI and GASCN additives, resulting in low background carrier density (~10^14 cm^-3) and long bulk carrier lifetime (~9 μs) in 1.25 eV bandgap perovskite materials. |
| The Regents of the University of California | Near-infrared photodetector devices and organic photovoltaic systems requiring extended spectral response beyond 1000 nm for sensing and energy harvesting applications. | Ultra-narrow Bandgap Non-Fullerene Acceptor Photodetectors | Developed ultra-narrow bandgap (0.86-0.99 eV) non-fullerene acceptors with A-D-A′-D-A structure achieving specific detectivity of 2.41×10^12 Jones at 1040 nm wavelength for near-infrared detection applications. |
| Brown University | Single-junction and tandem perovskite solar cells requiring lead-free, environmentally stable narrow bandgap materials with tunable optical properties for photovoltaic applications. | Titanium-based Double Perovskite Solar Cells | Developed Ti(IV)-based double perovskite materials (Cs2TiIxBr6-x) with continuously tunable bandgaps from 1.02 eV to 1.78 eV, achieving stable power conversion efficiency of 2.36% with open-circuit voltage of 0.97V and enhanced thermal/environmental stability. |
| Oxford Photovoltaics Limited | Bottom subcells in all-perovskite tandem photovoltaic devices and multijunction solar cells requiring narrow bandgap (1.3-1.5 eV) absorbers to maximize photon energy extraction and minimize thermalization losses. | Mixed Sn-Pb Perovskite Tandem Photovoltaic Devices | Developed mixed Sn/Pb perovskite materials with bandgaps tunable from 1.3 eV to 1.65 eV through compositional engineering, enabling optimized spectral harvesting with high crystallinity and phase stability for bottom subcells in all-perovskite tandem configurations. |
| TOYOTA JIDOSHA KABUSHIKI KAISHA | Top subcells in all-perovskite tandem solar cell architectures requiring wide bandgap materials (1.85 eV) with suppressed halide segregation for pairing with narrow bandgap bottom cells to achieve maximum power conversion efficiency. | Wide Bandgap Perovskite for Tandem Solar Cells | Developed photostable wide bandgap perovskite (1.85 eV) through alloying with ethylenediammonium and chloride ions into mixed-cation mixed-halide compositions, achieving reduced bromide content while minimizing lattice strain and trap densities for Pb/Pb perovskite tandems. |