Metal–organic hybrid perovskites share the formula of ABX3 (A = organic group, B = metallic ion, X = anions) with a three-dimensional (3D) framework of corner-sharing (BX6)4− octahedron, which is also the reason for high carrier mobility. The importance of the 3D framework to the transport of charge carriers can be evidenced by performance dependence on crystal orientation in layered two-dimensional (2D) perovskites1. For example, in the photovoltaic context, films of 2D Ruddlesden–Popper phases, with randomly distributed crystallites, have shown promising stability, but poor efficiency at only 4.73%2 in contrast to the efficiency of around 20% in 3D perovskites3, which could be attributed to the inhibition of out-of-plane transport due to the insulating organic groups1, 2, 4, 5. On the contrary, with careful control of crystallinity and anisotropy, a 2D perovskite can also show high performance close to 3D perovskites1. As a collateral effect of this confinement of charge carriers in the atom-scale slab that increases the exciton recombination, the low-dimensional layered perovskites with layered corner-sharing (BX6)4− separated by organic cations have been reported to show structural relaxation and high luminescence when the thickness is decreased to few unit cells6. The dimensionality of a 2D perovskite can be reduced further to zero-dimensional clusters, noted as (B n X m )j surrounded by Ak+ (m, n, j, k are integers), by tuning the crystallography and valence of cations and anions7. For example, organic–inorganic hybrid bismuth halide can generate a single (BiX6)3− octahedron8, face-sharing (Bi2I9)3− or edge-sharing (Bi2I10)4− bioctahedra9, 10, which have a size of ~1 nm separated by organic groups.

Nanometre-sized quantum dots (QDs) can display optical, electronic, and structural properties that often are not present in either isolated molecules or macroscopic solids11. For example, QDs of Si and PbS can efficiently generate multiple excitons from one high-energy absorbed photon following a mechanism known as carrier multiplication (CM) owing to their discrete energy levels and enhanced Coulomb interactions12,13,14. This is one of the suggested phenomena that may allow the efficiency of a single-junction solar cell to exceed the Shockley–Queisser limit15. The production of additional electron–hole pairs is expected to be greatly enhanced in QDs because their limited electron density of states greatly reduces the electron–phonon interactions12; however, for a solar cell using PbS QDs as an absorber, the large number of higher-lying energy levels due to surface defects were reported to decrease CM16. This could be alleviated by surface passivation with ligands17, alternatively this might also be achieved by protecting with the organic cation in zero-dimensional hybrid organic–inorganic halides. Moreover, the intrinsic junction between the negative charge on the low-dimensional (B n X m )j cluster and opposite charge on the surrounding organic Ak+ could cause an internal electric field that controls the broadband emission that could be tuned via the electronegativity of the core cluster and surrounding organic groups18.

The coupling between QDs and perovskite is of interest since the heterocrystals of QDs embedded in perovskites exhibit remarkable optoelectronic properties that are traceable to their atom-scale crystalline coherence that involves the efficient transport of excitons between them19. A metal–organic material with the formula (CH3NH3)3Bi2I9 (MABI) that contains quantum confined clusters/dots of (Bi2I9)3− has been reported as an effective absorbing material in a solar cell, but the performance was low, 0.1%20, 21. With a small size (around 1 nm) of (Bi2I9)3−, MABI showed a separate excitonic peak in the absorption spectra due to the confinement of charge carriers, and the binding energy of charge carriers has been estimated to be over 0.3 eV22. An analogous explanation on the even poorer performance compared to the 2D layered perovskite could be the enhanced confinement of charge carriers, but this explanation has not been elucidated because the performance of a solar cell depends on multiple parameters, such as the band energy alignment of different components and the microstructure of the layers. In a more recent study, MABI shows a double-peak emission including one close to band gap coupled with one in the blue light region and is superior in stability over lead-based perovskite in ambient air23, 24. Interestingly, long-lived excitons on the scale of nanoseconds have also been observed, which contrasts with the low performance of devices based on MABI23, 24. In this study, we synthesised a highly orientated MABI film to explore these issues. We studied the photoluminescence (PL) anisotropy and lifetime of excitons on these low-dimensional hybrid materials in order to understand the charge-carrier transport property. The PL at high excitation energy above twice the band gap (E g) seems to show an enhancement in quantum yield that may be explained in terms of CM25, which could open up a horizon of low dimensionally bonded hybrid materials for third-generation photovoltaics.


Structure analysis of MABI crystal and orientated film

Figure 1 shows the structure of MABI determined by single-crystal diffraction measured at room temperature24. The materials show hexagonal symmetry (P 63/m m c) and the face-shared BiI6 bioctahedra or (Bi2I9)3−clusters are separated by CH3NH3 + groups. The unit cell is a = 8.5821(3) Å and c = 21.7678(8) Å, leading to a volume of 1388.46(11) Å3 and a density of 3.8 g cm−3. Considering the size of an iodine anion, the (Bi2I9)3−clusters are ca. 1.11 nm in size and are separated from each other by ca. 0.16 nm. The density of the (Bi2I9)3− clusters is 1.69 × 1027 cm−3, which is much higher than the likely concentration of nanoparticles (1017–20 cm−3) suspended in solvent25. The thermal stability of MABI as a function of temperature was studied with differential scanning calorimetry, and no phase transformation was observed between −50 and 140 °C (Supplementary Fig. 1). This differs from the perovskite structure that changes from orthorhombic at room temperature to hexagonal or cubic structure at higher temperature26. The stable structure of MABI could be beneficial in the stability and lifetime of the device. In previous studies involving Si nanocrystals with quantum cutting phenomena, the spatial distribution showed that 50% of the nearest-neighbour distances are below 1 nm12. The CH3NH3 + group surrounding the (Bi2I9)3−clusters at the atomic level behaves like the atomic ligands that separates and passivates PbS QDs17.

Fig. 1
figure 1

Crystal structure of (CH3NH3)3Bi2I9 from single-crystal diffraction The hydrogen atoms are omitted. The thick light-blue line (0.43 nm) shows the shortest distance between two Bi2I9 bioctohedra and the thick red line (0.85 nm) shows the distance between two furthest iodine atoms. ½ C and ½ N represent the half-occupied carbon and nitrogen sites, respectively

Figure 2 shows the results of X-ray diffraction (XRD), optical microscopy and scanning electron microscopy (SEM) obtained from the coating. The film is mostly composed of large grains with good crystallinity. The XRD pattern of a large area film shows only peaks in the highly orientated structure in the <002> direction, while the XRD of the powder by crushing the film showed more peaks from the other crystal planes. The refined unit cell parameters, a = 8.5792(1) Å, c = 21.7588(4) and V = 1386.95(5) Å3, are in good agreement with those previously reported for MABI24. The X-ray photoemission spectroscopy (XPS) and Raman spectroscopy on the prepared film (see Supplementary Figs. 2 and 3 and Supplementary Table 1) indicate that the surface of the film is not degraded in ambient air. The ultraviolet-visible spectroscopy (Supplementary Fig. 4) shows a band gap of 2.19 eV with a direct transition due to the excitonic nature of the absorption peak, similar to the value reported by Kawai et al. on MABI single crystal22. Although there was a report on the indirect transition of band gap for MABI based on the density functional theory calculations that imply a split of conduction band21, 23, it should be noted that the absorption spectra of MABI is dependent on the orientation of crystals24, which is a strong indication of charge carrier localisation. The absorption spectrum of a MABI film shows an excitonic peak at 2.44 eV, which is slightly different to that of a similar (C6H11NH3)3Bi2I9 (2.47 eV22, 27) containing (Bi2I9)3− clusters but with a larger organic group. Since this peak is usually assigned to the (Bi2I9)3− group22, the organic group does not contribute to the absorption at this energy level. The lowest exciton state arises from excitations between the valence band, which consists of a mixture of Bi(6 s) and I(5p) states, and the conduction band, which derives primarily from Bi(6p) states, and is confined zero-dimensionally in the bioctahedra Bi2I9 3− 27. Substitution of Cs or formanidinium on methylamonium (MA) site in MAPbI3 has been shown to cause significant shift (larger than 100 meV) of the band edge20, 28, contrasting with MABI where the band gap is unchanged between Cs and MA20.

Fig. 2
figure 2

Structure characterisation of the orientated (CH3NH3)3Bi2I9 coating on quartz. a X-ray diffraction results from the coating and powdered samples. b Optical microscope and c scanning electron micrograph of the (CH3NH3)3Bi2I9 coating processed by depositing and drying of the solution of BiI3 and CH3NH3I in N,N-Dimethylmethanamide. The scale bars represent 25 μm

PL anisotropy of MABI coating

The fundamental property of a crystalline material is the periodic spatial arrangement of atoms and clusters. The MABI crystals containing periodically aligned Bi2I9 3− clusters could be viewed as QDs with organic groups as separators, resembling a core–shell structure due to the nanometre size of the photoactive Bi2I9 3− clusters. Since the MABI crystals are aligned in the <002> direction on the quartz substrate and orientated randomly in the perpendicular directions, there would be PL anisotropy in the <002> direction. PL anisotropy is investigated by varying the angle of the coating with the incident beam while fixing the position of the detector. Distinct PL spectra are obtained as shown in Fig. 3: at 25°, only one peak is shown, while at 45° and 65°, the spectra split into two peaks, and the relative height of the peak at the blue side tends to increase with the incident angle, θ. On the other hand, the cathodoluminescence (CL) of MABI coating in Supplementary Fig. 5 does not show luminescence anisotropy but a continuous emission from 490 to 750 nm. One of the fundamental differences between CL and PL is that, while a photon in PL generates only one electron–hole pair, one 5-keV electron in CL, for example, can generate hundreds of electron–hole pairs in the excitation volume, which is usually several microns in diameter29. Specifically, the penetration depth of the electron beam of 5 keV would be around 200 nm based on the density of 3.8 g cm−3. This difference makes the actual incident angle of a high-energy electron beam in CL very difficult to control because of the re-absorption of photons.

Fig. 3
figure 3

Photoluminescence (PL) anisotropy of (CH3NH3)3Bi2I9 coating. a Experimental set-up and coating orientation. The detector and incident angle are positioned at right angles and the substrate is rotated to control the angle. The sample is positioned vertically and the wavelength of incident beam is 350 nm. bd show the respective PL spectra at 25°, 45° and 65°. The black lines at the bottom of bd are the PL measurement on the bare fused silica substrate at the respective angles

Charge-carrier localisation and intercluster transport in (CH3NH3)3Bi2I9

The PL excitation (PLE) technique allows one to measure all the allowed intersub-band absorption transitions, and therefore to make a much more complete characterisation of low-dimensional system. The PLE spectra (Fig. 4a) for emission detection at 650 nm (λ det = 650 nm) can be fitted by four peaks (Supplementary Fig. 6) centred, respectively, at 385, 464, 557 and 615 nm, showing a discrete absorption. The change of incident angle has a pronounced effect on the relative height of these peaks, corresponding to the absorption variation with the crystal directions24. As anisotropic crystals have a light absorption coefficient depending on the direction of the light wave and its polarisation, the variations of peak heights with incident angle confirm the optical anisotropy of MABI. More importantly, the PLE spectra for different λ det (Fig. 4b) show distinct features, an indication of localised excitons that are not free to move into all parts of the QDs. As the λ det shifts to the blue side from 650 nm, the bleaching of low-energy absorption peak is probably associated with the well that is heavily electron-occupied30 (as in the charge on Bi2I9 3−) or the increasing emission overlap of trapped states.

Fig. 4
figure 4

Excitation property of the charge carriers. a Ultraviolet–visible absorption derived from diffuse reflectance spectra of (CH3NH3)3Bi2I9 and the angular dependence of photoluminescence excitation (PLE) of 650 nm emission (λ det = 650 nm) at 25°, 45° and 65°. b PLE spectra for emission at λ det = 650, 610 and 600 nm while keeping incident angle, θ, at 45°. The open circles show the major PLE peaks. c Time-resolved photoluminescence of the coating placed at θ = 0° under a excitation beam of 375 nm (λ ex = 375 nm) and 450 nm (λ ex = 450 nm). d Schematics of quantum-well structure and multiphonon relaxation. The mid-gap energy level is from the organic termination. E hh represents the energy level of heavy hole state, while E 1, E 2 and E 3 show the discrete energy levels in the conduction band

The lifetime measurements on the excitons when the sample is placed perpendicular to the excitation beam (θ = 0°; Fig. 4c) were performed using two excitation wavelengths (λ ex = 375 or 450 nm) close to the PLE peaks, while detecting emission, λ det, is between 580 and 660 nm. When excited at 375 nm the samples show very fast (life time of excitons, τ < 1 ps), slower (τ = 10 ps) and very slow (τ > 2 ns) PL decays, while when excited with 450 nm light it is just very fast (τ < 1 ps) and very slow (τ > 12 ns). The picosecond excitons under 450 or 375 nm excitation could perhaps be inside the cluster of Bi2I9 3− and the distinct lifetime profile indicates that the emissions at these two excitations are from trapped states of different sites. The early-time emission (Supplementary Fig. 7) with both excitation wavelengths is centred on ~600 nm, while the long time 20-ps emission is centred on ~725 nm. Because the PL from the fluorometer (steady state) is an integral of what we see with the streak camera and only one peak at ~700 nm is shown at low incident angle, the long-lived excitons will contribute mostly to the PL spectra. The nanosecond lifetime of a small portion of excitons indicates perhaps that some of them tunnel through the gap of CH3NH3 + and become delocalised because of the interdot coupling24.

For a QD, the cooling of carriers would require multiphonon processes when the quantised levels are separated in energy by more than the fundamental phonon energy, as shown in Fig. 4d. Excitons might travel between dots through multistep, phonon-assisted tunnelling, or homo-Förster resonance energy transfer that increases the lifetime of the acceptors. The tunnelling of excitons is very sensitive to the interdot distance. Showing the same type of absorptions, CdSe nanocrystallites in a closely packed superlattice show a red-shifted PL in a dilute colloidal system due to the interdot coupling11, 31, but, in an anisotropic crystalline MABI, we demonstrated that the incident angle is an additional parameter for the emission spectra.

PL quantum yield and quantum cutting

Because of the high degree of orientation of the MABI film, the PL is anisotropic, so overall PL of the coating near the band gap is measured on a powder sample under different excitation beam, ranging from 400 to 250 nm, as shown in Fig. 5a. A set of parasitic peaks at the low-energy side of the main peak is an indication of cascade excitations, suggesting that the re-absorption and re-emission of photons among the micron-scale crystals is possible since the absorption edge from the diffuse reflectance spectroscopy of a powdered sample is as low as 1.77 eV (700 nm). Because of the low dimension of Bi2I9 3− (ca. 1 nm, close to that of a molecule), the Stokes shift causes lower-energy emission when an emitted photon from one crystal is reabsorbed by a neighbouring one. Because of the anisotropic nature of the Bi2I9 3− cluster, two main peaks rather than one are observed according to the anisotropic PL of a coating, and a Stokes shift energy of 0.13 eV can be obtained from the PL spectra. As the band gap of the highly orientated film (θ = 0°) is determined to be 2.19 eV, while the peak energy of PL singlet at θ = 25° is 1.86 eV, giving a binding energy in this situation ~0.33 eV at low angles. Kawai et al. studied the absorption of MABI single crystals of different thicknesses in the temperature range between 78 and 301 K, and the excitonic nature of the absorption peak at 2.43 eV was proven via the fitting of Urbach tail at the low-energy side of the peak and the binding energy was estimated to be higher than 0.3 eV22. The Stokes shift of the powdered sample is lowered to 0.13 eV because of the higher-energy level at higher angles, as illustrated in Fig. 5b. A relative PL quantum yield (PLQY)25 under each excitation energy as shown in Fig. 5d was obtained by normalising the integration of PL spectra (Fig. 5c) by the pump intensity (Supplementary Fig. 8) and absorption. An increase in the PLQY was observed when the excitation energy is above 4.13 eV. The nearly linear increase in the quantum efficiency, rather than an abrupt jump, after the photon energy is higher than twice the band gap, 2E g, implies that the possible CM process happens possibly via the impact ionisation mechanism as simulated by Allan et al.32 In MABI, a second (Bi2I9)3− may be excited by a neighbouring (Bi2I9)3− cluster containing a hot electron–hole pair, since the 0.11-nm separating distance controlled by the size of CH3NH3 + groups is sufficiently small to facilitate the energy transfer. MABI contains a small number of delocalised excitons with lifetime on the scale of nanoseconds, but such systems can still be expected to produce CM33. The difference in the lifetime of excitons at λ ex = 450 and 375 nm showed limited impact on either the PL intensity or PLQY. The Tauc plot (Supplementary Fig. 9) of bulk CH3NH3I was presented to estimate the excitation energy of the organic separator, showing a large band gap of 4.83 eV, but MABI still loses its low-dimensionality in CL with excitation energy as high as 5 keV.

Fig. 5
figure 5

Photoluminescence (PL) at difference excitation energies. a PL spectra of the powdered (CH3NH3)3Bi2I9 under different excitation energies. The blue and red arrows show the Stokes shift of 0.13 eV. The dashed line at the bottom is the PL measured on the substrate excited at 400 nm. b Energy diagram for the band gap of orientated film and the peak energy of PL at different angles. c Integration of PL intensities at different excitation energies. d Relative PL quantum yield (PLQY) for the (CH3NH3)3Bi2I9 powder and coating on quartz, respectively


A low-dimensional hybrid material, MABI, showing a band gap of 2.19 eV and absorbing visible light has been obtained via solution processing. The film resulting from drying the solution showed a high degree of preferred orientation in the <002> direction. The close coordination between the negatively charged core cluster, (Bi2I9)3−, surrounded by positive CH3NH3 + seems to facilitate the localisation of excitons. The resultant anisotropic electron density would give rise to the Stokes shift in the PL. A small portion of long-lived excitons arises from the coupling and energy transfer between the clusters. The quantum yield from the QD core clusters separated by insulating organic cations is seen to increase when the excitation is above 2E g, indicating quantum cutting.



Bi2O2(CO3) (2 g, Alfa Aesar 99.9%) was dissolved in hydroiodic acid (HI) (10 ml, Alfa Aesar) using ethanol as solvent (500 ml) and then the product, BiI3, collected after the solution was evaporated at 80 °C. Methylammonium iodide was prepared by reacting methylammonia (24 ml) solution in hydriodic acid solution (10 ml) in ethanol (100 ml). The solvent was removed at 50 °C using a rotary evaporator. The resulting white solid was washed in diethylether and dried in a vacuum oven overnight.

Characterisation of coating and powdered sample

BiI3 and CH3NH3I (1:2 in mole ratio) were dissolved in dimethyl formamide (DMF) to form a clear solution (20 wt.% of salts) when heated at 60 °C with stirring. The solution is spin-coated on to a fused silica substrate at 2000 r.p.m., and dried in air for 30 min before baking on a hotplate at 100 °C for 1 h. Absorption measurements were carried out using a Cary Varian 300 spectrometer. PL emission and excitation spectroscopy of the coating were performed on a FLS980 spectrometer (Edinburgh Instruments, UK) and ultrafast luminescence measurements were performed using up-conversion spectroscopy. CL was carried out on an inclined sample in a low-vacuum field emission SEM using a 5 keV, 1.5 nA electron beam. The luminescence was collected using a reflecting objective, dispersed with a 1/8-m spectrograph and detected with an electron-multiplying CCD. X-ray photoemission spectra and Raman spectra on the coating were carried out on Kratos Axis Ultra DLD photoelectron spectrometer and Lab Ram 300 (Horiba Jobin Yvon SAS), respectively, and more detail and analysis were provided in Supplementary Information. SEM images were taken on a Jeol 6700 F microscope. Powder sample of MABI was prepared by scratching and grinding a large area of coating on a quartz substrate. Phase purity was confirmed by powder XRD on a Panalytical expert monochromated X-ray diffractometer with Cu-Kα target (λ  = 0.15418 nm), and unit cell parameters of the powdered sample were analysed using General Structure Analysis System software. The absorption of the powdered sample was recorded with a V650 spectrophotometer (Jasco). PL of the powder sample was measured on a Horiba Jobin Yvon spectrofluorometer and the powder was sandwiched between two quartz plates with an illuminated spot size of about 0.6 cm2.

Data availability

All new data associated with this manuscript are available from the University of St Andrews repository