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Earth-abundant non-toxic perovskite nanocrystals for solution processed solar cells

Sergio Aina ab, Belén Villacampa ac and María Bernechea *abde
aInstituto de Nanociencia y Materiales de Aragón (INMA), CSIC-Universidad de Zaragoza, Zaragoza, 50009, Spain. E-mail: mbernechea@unizar.es
bDepartment of Chemical and Environmental Engineering (IQTMA), University of Zaragoza, 50018 Zaragoza, Spain
cDepartment of Condensed Matter Physics, University of Zaragoza, 50009 Zaragoza, Spain
dNetworking Research Center on Bioengineering, Biomaterials and Nanomedicine (CIBER-BBN), 28029, Madrid, Spain
eARAID, Government of Aragón, 50018, Zaragoza, Spain

Received 22nd March 2021 , Accepted 31st May 2021

First published on 1st June 2021


Abstract

Semiconductor nanocrystals, used in quantum dot solar cells, are interesting materials for photovoltaics because they can be obtained in solution and can be composed of abundant elements. Moreover, as compared to other photovoltaic materials, nanomaterials show unique features due to their novel size- and shape-dependent properties such as band gap tuning, multiple exciton generation, and modulation of n- or p-type behaviour by doping or by modifying the ligands on the surface of the nanocrystals. Quantum dot solar cells, together with perovskite solar cells, are the latest incorporation to photovoltaic technologies and have already shown impressive progress in efficiencies and great promise as alternatives to commercial solar cells. However, in all cases, the highest efficiencies are obtained with materials that contain lead in their composition. To solve the problem of toxicity, several materials have been proposed as substitutes. In this review, we summarize some of the non-toxic alternatives that have been synthesized as nanocrystals and incorporated in photovoltaic solar cells, specifically: tin (Sn), germanium (Ge), bismuth (Bi), and antimony (Sb)-based materials. Our findings show that this field has been scarcely covered; there are very few reports on non-toxic perovskite nanocrystals incorporated in solar cells and in general, the efficiencies are still modest. However, this area deserves more attention since some nanocrystal-based solar cells already outperform bulk counterparts. For each case, we also discuss factors limiting efficiency, the approaches followed to overcome these limitations, and the possible solutions to improve efficiency.


Introduction

In the last 10 years, two new types of photovoltaic solar cells have emerged: perovskites and quantum dots (QDs), also known as colloidal semiconductor nanocrystals (NCs). Starting from modest efficiencies around 3%, they have quickly escalated up to 25.5 and 18.1%, respectively, in this short period of time.1 In both cases, the active materials are composed of earth-abundant elements and can be processed from solutions, which offers easier manufacture and lower prices than commercial solar cells. Therefore, they might soon become an alternative to commercial solar cells, whether alone or in tandem with other photovoltaic technologies.

Semiconductor nanocrystals are nanomaterials with typical dimensions of less than 10 nm. They offer interesting and unique properties for their use in several optoelectronic devices and more precisely in solar cells. Traditional photovoltaic materials have a fixed band gap that determines the range of photons that solar cells will be able to absorb. However, the reduced size of nanocrystals leads to quantum confinement effects, i.e. their electrical and optical properties, including band gap, can be easily modified just by changing their shape and size (Fig. 1A). Multiple exciton generation (MEG), the generation of two (or more) electron–hole pairs from one absorbed high-energy photon, is more efficient in nanocrystals than in bulk semiconductors and this could produce efficiencies over the theoretical limit for single-junction solar cells (Shockley–Queisser limit).2,3 Moreover, their behaviour as n- or p-type semiconductors and doping density can be modified by introducing foreign atoms, like in traditional silicon technologies, and also by surface treatments. Nanocrystals are stabilized in solution thanks to the presence of long chain ligands on their surface that are replaced by shorter ligands or atoms during the fabrication of solar cells (Fig. 1B). Depending on the final ligands on the surface of NCs the position of the Fermi level and/or the valence and conduction bands can be modified, which is a unique feature of nanocrystals and a very powerful tool (Fig. 1C).4 Taking advantage of all these features efficiencies over 16% have been obtained using perovskite nanocrystals (Cs1−xFAxPbI3).5


image file: d1ma00245g-f1.tif
Fig. 1 (A) Scheme showcasing the band gap tunability in nanocrystals as a function of their size. (B) Scheme of a surface ligand exchange process where long chain capping molecules are replaced by shorter ligands. (C) Diagrams representing the shift of the valence and conduction bands (left) or the Fermi level (right) depending on the nature of ligands on the surface of the NCs (L1, L2, L3…). (D) Perovskite ABX3 structure. X site corresponds to a halide anion, A site to an organic (MA, FA…) or inorganic (Cs, Rb…) cation, and B (green sphere) to a metal (Pb, Sn, Ge…) cation. (E) Schematic representation of 0D, 1D, 2D, and 3D perovskite structures.

Perovskite solar cells (PSC) are based on materials with a general formula ABX3; where X is a halide anion (X = Cl, Br, I), B is an inorganic cation (usually Pb), and A can be an inorganic (usually Cs or Rb), or an organic cation (usually MA = methylammonium, or FA = formamidinium) leading to all-inorganic or hybrid organic–inorganic perovskites, respectively (Fig. 1D).6 They usually crystallize in a 3D structure, however, the dimensionality can change to 2D, 1D, or 0D (Fig. 1E) if Pb is replaced in the B position by a cation with a different charge (Cu+, Sb3+, Sn4+), which may consequently alter the perovskite formula (e.g. A2B2X6, A3B2X9). Additionally, the structure can also be modified depending on the volume of cation A (greater volumes can lead to distortions in the 3D structure) or the radius of the B atom (for example, Cu smaller radius favours 2D structures).7 In general, the fabrication of the active layer is performed by mixing the precursors in solution, depositing the solution on a substrate followed by a final thermal treatment, usually at low temperatures (<100 °C). This implies that, in these devices, synthesis, film deposition, and grain crystallization occur at the same time.

The best performing perovskite solar cells are based on lead-containing materials (Pb2+ cations in B position). They have high absorption coefficients, suitable direct band gaps (around 1.5–2.5 eV), small exciton energy, balanced and long charge-carrier diffusion-length, high carrier mobility, and trap-free carrier relaxation, which favour high efficiencies and make them ideal for photovoltaic applications.6,8–10 However, the long-term stability of lead-perovskite solar cells is poor, affected by moisture, oxidation, heat, or light, which causes losses in the efficiency of the devices over time when working at ambient conditions.11 For instance, MAPbI3 degrades into PbI2 and MAI in the presence of water, and high temperatures (150 °C) can also induce the perovskite material degradation.12–16

It has been proposed that the key feature that makes lead-based perovskites such great materials for photovoltaic applications is their defect tolerant nature, associated with the 6s2 lone pair configuration of Pb2+ that leads to large dielectric constants, small effective masses, a valence band maximum composed of antibonding states, and high levels of band dispersion.10,13,17,18 Following this rationale, perovskite materials composed of other ns2 cations, such as Sn2+, Ge2+, Sb3+, and Bi3+, have been proposed as alternatives for their use in solar cells, as they may offer similar attractive properties than lead-perovskites, but better stability in ambient conditions.10,13 Moreover, lead is a toxic heavy metal that dissolves in water and tends to bioaccumulate, which is problematic during fabrication, use, and disposal of lead-based devices.19–21 The suggested alternative cations are considered more benign than lead, or, like bismuth, non-toxic elements; therefore, they offer the additional advantage of eliminating health or environmental concerns. Indeed, these materials may be an attractive option for devices in close contact with humans, such as wearables or indoor applications.22–24

In the last years, there has been some progress in this area and some reviews have already summarised the most relevant results in lead-free bulk perovskite materials for solar cells.10,13,15,18,21,25–32 In this review, we focus on Sn2+, Ge2+, Bi3+, and Sb3+ perovskites that have been synthesized as nanocrystals and incorporated in photovoltaic solar cells. Some recent reviews have focused on the synthesis and light emission properties of lead-free perovskite NCs, but none of them has collected the efficiencies obtained incorporating the nanocrystals in solar cells.33–35

Perovskite nanocrystals for solar cells

Colloidal perovskite nanocrystals offer similar defect tolerance as bulk perovskite materials plus additional advantages related to nanoscale phenomena such as modification of the properties by changing the size or shape of the nanocrystals, multiple exciton generation features and, property-tuning by modifying the ligands on the surface, which at the same time could improve device stability by passivating surface defects. Additionally, the decoupling of material synthesis and material deposition simplifies fabrication and allows to prepare phases or compositions that are not stable in the bulk as well as better control on the stoichiometry when compared to the in situ preparation of bulk perovskites.2–4

The most common structure of a perovskite solar cell, also used in the perovskite nanocrystal solar cells, consists of an n–i–p junction (n-type, intrinsic, and p-type semiconductors). The light harvester layer (intrinsic semiconductor) is placed between a Hole Transport Layer (HTL, p-type semiconductor), an Electron Transport Layer (ETL, n-type semiconductor), and the two metallic contacts (Fig. 2A). Alternatively, NCs can be introduced in Dye Sensitized Solar Cells (DSSC). In a typical DSSC, upon light absorption the excited sensitizers inject electrons into the conduction band (CB) of TiO2. The oxidized dyes are regenerated by the electrolyte (Fig. 2B). NCs can be incorporated acting as sensitizers, either alone or in combination with other dyes to enhance light absorption.


image file: d1ma00245g-f2.tif
Fig. 2 (A) Left: n–i–p structure in perovskite solar cells. The perovskite material acts as light harvester, HTL and ETL are the hole and electron transport layers, respectively, M is the metallic contact, and TCO the transparent contact layer. Right: Charges flow in the structure (B) Left: Typical DSSC structure consisting of mesoporous TiO2 layer with adsorbed dye molecules, electrolyte (iodide/triiodide in this example), and metallic (M) and transparent contacts (TCO). Right: Charges flow in the structure.

The solar cell performance of Pb-perovskite NCs has progressed significantly from the first work by Kojima et al. in 2009 reporting an efficiency of 3.8% using MAPbI3 NCs as sensitizers in DSSCs.36 Two years later, it was found that by optimizing the thickness of the TiO2 layer, the efficiency could increase up to 6.5% for MAPbI3 NCs. Nonetheless, the perovskite layer was only stable for 10 minutes until the NCs dissolved in the electrolyte.37 Later, substituting the electrolyte by spiro-OMeTAD, acting as HTL, the efficiency achieved was 9.7%.38 In the field of all-inorganic perovskites, (without volatile components, detrimental in terms of stability) the use of colloidal NCs has allowed to stabilize structural phases desirable for photovoltaics. For instance, the cubic α-CsPbI3 form has an optimal bandgap for photovoltaic applications, but it is hardly achievable in bulk, where the orthorhombic δ form prevails below 320 °C. By using ligands such as oleic acid and oleylamine, α-CsPbI3 NCs were synthesized and stabilized at room temperature, and an efficiency of 10.77% was reported for perovskite NCs solar cells.39 The introduction of a polymer in the interface between the NCs and the HTL allowed to adjust the energy levels and consequently to enhance charge extraction. Efficiency values as high as 14% and 13.2% have been obtained for CsPbI3 and FAPbI3 NCs perovskite cells, respectively.40

Nowadays, Cs0.5FA0.5PbI3 NCs have delivered the highest published efficiency for nanocrystal-based PSC with a 16.6%, where FA addition played an essential role by reducing non-radiative recombination.5 The record for all-inorganic nanocrystal-based PSC is 16.07% obtained with Zn-doped CsPbI3 NCs.41 The optimization between energy levels, doping with other elements, or the introduction of stabilizing ligands/molecules have been essential for the development of devices with greater efficiencies.

Non-toxic perovskite nanocrystals for solar cells

Despite the high efficiency values achieved with lead-based perovskite NCs5 the stability and toxicity issues commented above have led to the proposal of several non-toxic materials to substitute them. The main non-toxic perovskite substitutes are composed of tin, germanium, bismuth, and antimony. Tin and germanium are the obvious alternatives to lead-based perovskites since they belong to the same group in the periodic table and they share analogous electronic configurations. Therefore, similar properties and crystalline structures are expected for these Pb-free perovskites. Moreover, they are relatively abundant on earth crust and considered as less toxic than lead. However, tin and germanium show a higher tendency to oxidize (from Sn2+ and Ge2+ to Sn4+ and Ge4+ cations) than Pb2+, a fact explained by the inert pair effect. Lead has the strongest inert pair effect, which means that its outermost ns2 electrons (6s2) are strongly bound to the nucleus due to the poor shielding of d and f orbitals. As the atomic number increases, the attraction force of the nucleus over the electrons is usually greater, as well as the shielding due to the higher number of energy levels. However, d and f electrons shielding effect is weak; therefore, the interaction between the 6s2 electrons and nucleus is stronger than expected, preventing their participation in any bonding. For that reason, the most stable form for lead is Pb2+, not Pb4+. In the case of tin, this inert pair effect is reduced because the 5s2 electrons are not as strongly tighten as 6s2 in Pb, which favours Sn2+ oxidation to Sn4+. Germanium is upper in the group, which makes the inert pair effect even weaker, 4s2 electrons are more likely to participate in chemical bonding and Ge2+ cations tend to oxidize to Ge4+.10,35,42–44 Being adjacent to Pb2+ and Sn2+ in the periodic table, Bi3+ and Sb3+ have similar ns2 electronic configuration, are more stable in ambient conditions, have demonstrated low toxicity, and are relatively abundant on the earth crust. Apart from the similar electronic configuration, Bi and Sb can be incorporated into the perovskite lattice because they have an ionic radius similar to Pb. However, in some cases, due to their different oxidation state (+3), they form low dimensionality (2D, 1D or 0D) structures in order to maintain charge neutrality. This may cause problems in charge transport and have a significant impact in the efficiency of devices.13,21,26,27,35

The next sections are organized as follows: first, characteristics of each material, application in bulk solar cells, and maximum efficiencies obtained are summarized. Finally, a detailed review of the corresponding perovskite NCs used in solar cells and their efficiencies (also referred as power conversion efficiency, PCE) are explained. We have observed that there are very few examples of perovskite NCs introduced as absorbing material in solar cells, therefore, in some cases, we have included materials that may not form the traditional lead-halide composition or the typical perovskite crystalline structure, but that share the main characteristics of perovskite materials used in solar cells.

Tin-based perovskites

Tin (Sn) is the natural alternative to lead-perovskite NCs. Sn is a non-toxic element that belongs to the same group in the periodic table as Pb and Ge. They have analogous electronic configurations; thus, they form similar compounds and similar properties are expected. However, as mentioned above, Sn2+ cations are unstable because they tend to oxidize to Sn4+. This oxidation process creates undesired vacancies in the crystalline structure that favours carrier recombination, which may result in low photoluminescence quantum yield (PLQY) and solar cell efficiency.33,45,46

The interest in substituting lead has fostered the use of several tin-based materials as absorption layers in bulk perovskite solar cells. For example, optimized all-inorganic CsSnI3 solar cells have shown a 4.81% power conversion efficiency,47 recently improved up to 7.5% by incorporating N,N′-methylenebis(acrylamide) into the perovskite layer.48 FASnI3 perovskite solar cells treated with SnF2–pyrazine showed an efficiency of 4.8%, maintained over 100 days,49 which was later improved up to 9% when mixing the 3D FASnI3 perovskite with a small quantity of the 2D Sn-perovskite PEA2SnI4 (PEA = phenylethylammonium). Apparently, the addition of the 2D material promotes the growth of highly crystalline and oriented FASnI3 grains which reduces the number of grain boundaries, suppresses tin vacancies, and improves charge carrier lifetime.50 Moreover, applying a passivation treatment with edamine (EDA), FA0.98EDA0.01SnI3 bulk perovskite solar cells achieved a 10.18% efficiency. Edamine molecules prevented the charge carrier recombination by suppressing tin oxidation and iodide vacancies.51 Recently this value has been improved up to 13% by employing GeI2 doped (FA0.9EA0.1)0.98EDA0.01SnI3, where EA corresponds to ethylammonium cations. The presence of EA in the perovskite enhanced the charge transport by presenting more favourable energy level adjustment between the perovskite and the charge transport layers.52 Also, other hybrid organic–inorganic Sn-perovskites have been tested in devices: ethylenediammonium–MASnI3 solar devices delivered a 6.63% efficiency.53 Mixing methylammonium and formamidinium a power conversion of 8.12% was achieved for FA0.75MA0.25SnI3 devices.54

Tin-based materials tend to suffer from bulk recombination due to the presence of Sn vacancies generated by Sn2+ oxidation, which strongly limits their properties as light absorbers. In order to prevent Sn2+ oxidation, additives such as SnI2 excess47 or pyrazine49 have been introduced. Another option has been the use of the most stable tetravalent cation (Sn4+).55,56 However, Sn4+-based perovskites offer lower efficiencies (1%), as shown in studies employing Cs2SnI6.45,56,57 Therefore, the key for achieving better performing devices might rely on the control of Sn2+ oxidation. The use of hypophosphorous acid (HPA) has shown to increase the efficiency of a CsSnBr2I perovskite solar cell from 1.67% to 3%. The HPA addition induced the formation of perovskite seeds and decreased recombination by lowering carrier mobility and charge carrier density. Moreover, devices showed excellent stability. Experiments under 1 sun at maximum power point showed a 98% retention of the original efficiency, even at temperatures as high as 200 °C, while in analogous experiments MAPbI3 devices lost almost 90% of the original efficiency at temperatures of 80 °C. Furthermore, encapsulated devices stored under ambient conditions (25 °C and uncontrolled moisture) maintained ≈100% of the initial efficiency over a period of 77 days.45

Lately, tin-perovskite NCs have risen as alternatives to bulk tin PSC. They offer the general advantages of nanocrystals such as easy synthesis, quantum confinement and high photoluminescence yield.33,58,59 Nevertheless, the aforementioned drawback caused by Sn2+ oxidation could be fostered in the nanoscale due to the high surface/volume ratio. Therefore, stabilization of the nanocrystals is crucial. By controlling the synthesis, functionalizing the surface with ligands60,61 and adding excess of SnX2, more stable tin-perovskite nanocrystals, such as CsSnX3 NCs, can be obtained.33,47,53 Only a few reports, including CsSnI3 NCs, rod shaped CsSnX3 NCs (X = Cl, Br, I), and CH3NH3SnBr3−xIx NCs (MASnBr3−xIx NCs) describe the use of tin-perovskite NCs as light harvesters in solar cells.

CsSnI3 nanocrystals

A one-pot synthesis method was used to produce CsSnI3 NCs by a simple and mild process. CsI and SnI2 were used as precursors, and triphenyl phosphite (TPPi) was added as antioxidant solvent additive (ASA) to prevent Sn2+ oxidation to Sn4+ and the subsequent formation of vacancies in the perovskite lattice. Thanks to the addition of TPPi the nanocrystals solutions remained clear and stable for at least 90 days. The photovoltaic performance of CsSnI3 NCs was compared with a bulk CsSnI3 active layer using the solar cell structure depicted in Fig. 3A. The active layer was sandwiched between poly(3,4-ethylenedioxythiophene)polystyrene sulfonate (PEDOT:PSS), acting as hole transport layer, and [6,6]-phenyl-C61-butyric acid methyl ester (PCBM), acting as electron transport layer. The antioxidant agent TPPi showed to improve the performance of bulk-based and NCs-based CsSnI3 solar cells (Fig. 3B). Bulk CsSnI3 devices showed an efficiency of 0.022%, which was enhanced up to 1.202% when adding TPPi. For the NCs-based devices (with TPPi too), the average efficiency obtained was 4.13% with a maximum of 5.03%. In stability experiments the NCs solar cell outperformed the bulk one; its efficiency remained intact during 30 days, while it was constantly varying for the bulk device.58
image file: d1ma00245g-f3.tif
Fig. 3 (A) Device structure of the solar cell based on the CsSnI3 films. (B) JV curves of CsSnI3 bulk solar cell (black), CsSnI3 bulk solar cell with the addition of TPPi as antioxidant additive (green) and CsSnI3 NCs solar cell with TPPi (blue). Reproduced from ref. 58 with permission from the Royal Society of Chemistry (RSC, Journal of Materials Chemistry A).

These results highlight the importance of overcoming Sn2+ oxidation to reach better photovoltaic devices. Moreover, they show that the introduction of perovskite NCs could improve the efficiency and stability of devices. The NC-based device was better in every aspect than the corresponding bulk solar cell; nonetheless, the performance is still far from CsPbI3 NCs devices, that have achieved an efficiency over 16%.41

CsSnX3 nanocrystals (X = Cl, Br, I)

CsSnX3 rod-shaped nanocrystals (quantum rods, QRs) were synthesized using an easy, fast and clean solvothermal method. The advantage of QRs over spherical nanocrystals is that for the same diameter QRs have bigger volumes leading to a higher per-particle absorbance cross-section and, additionally, their elongated shape is supposed to improve charge injection to transport layers, which can improve device performance.62 In the reported synthesis SnX2 and Cs2CO3 were used as precursors, octadecene, oleylamine and oleic acid as solvents, and, to enhance the growth of high-quality QRs, trioctylphosphine oxide (TOPO) and diethylenetriamine were added as capping agents.63

A red shift in the band gap and PL emission, from 625 to 709 nm, was observed from the chloride to the iodide CsSnX3 (X = Cl, Br, I) QRs (Table 1). The nanocrystals were used as absorbing layers in solar cells including TiO2 as electron transport layer and spiro-OMeTAD as hole transport layer. The best efficiency was obtained for the CsSnI3 QRs (Table 1), probably due to its more adequate band gap among the three materials. Additionally, the stability of CsSnI3 QRs and bulk MAPbI3 sealed solar cells was tested. While CsSnX3 NCs solar cells showed a 40% efficiency decay after 16 days, the efficiency decay of MAPbI3 solar cell was 70%.63

Table 1 Band gaps (Eg), approximated from PL emission peaks, and power conversion efficiency (PCE) of the solar cells fabricated with CsSnX3 QRs. Extracted from ref. 63
E g (eV) PCE (%)
CsSnCl3 2.0 9.66
CsSnBr3 1.9 10.46
CsSnI3 1.7 12.96


The observed performance is very encouraging towards the development of lead-free inorganic solar cells. Indeed, the 12.96% efficiency obtained with CsSnI3 QRs is the best result for non-toxic perovskite NCs reported to date, surpasses the efficiency obtained with bulk CsSnI3 (7.5%),48 and is very close to the efficiency delivered by analogous lead-perovskite NCs devices (16%).

In this former case, CsPbI3 NCs were treated with ZnI2 to prevent iodine vacancies, which enhanced the stability.41 The loss in efficiency observed in CsSnI3 NCs devices after 4–5 days, which might be related to Sn2+ oxidation, can compromise their commercialization. The addition of an antioxidant agent, as commented in the previous example, or ZnI2 treatment like in CsPbI3 NCs, could be solutions to improve device stability.

CH3NH3SnBr3−xIx nanocrystals

H. Xu et al. reported a method to synthesize MASnBr3−xIx (x = 0–3) perovskite NCs and their use as light absorbers in DSSCs. The synthesis of MASnBr3−xIx NCs was performed using a hot-injection method and SnBr2, SnI2 and MABr as precursors. The NCs were stabilized with oleic acid and oleylamine as capping ligands. Different halide ratios were tested: MASnBr3, MASnBr2I, MASnBrI2 and MASnI3, showing a band gap of 2.3, 2.0, 1.8 and 1.5 eV, respectively. Nanocrystals were spin-coated on top of a mesoscopic TiO2 anode, I/I3 was used as electrolyte, and Pt as counter electrode. The PCE of the devices is collected in Table 2 with MASnBr2I showing the best efficiency.64
Table 2 Band gap (Eg) and power conversion efficiency (PCE) for different MASnBr3−xIx NCs. Extracted from ref. 64
NCs E g (eV) PCE (%)
MASnBr3 2.3 0.155
MASnBr2I 2.0 0.322
MASnBrI2 1.8 0.202
MASnI3 1.5 0.106


Electrochemical impedance spectra (EIS) showed that the resistance between the electrolyte and the NCs–TiO2 interface was much higher than for state-of-the-art DSSCs, which might be due to the presence of long chain molecules such as oleylamine around the perovskite NCs. In order to improve electron extraction, TiO2 interface was further decorated with graphene quantum dots reaching an efficiency of 0.60%. Alternatively, the introduction of the N719 dye as co-sensitizer to the MASnBr2I NCs improved the efficiency up to 8.79%, which is higher than the efficiency delivered by N719 alone (7.28%).65 As a preliminary result, an efficiency of 8.79% is very promising especially taking into account that state-of-the-art DSSCs show record efficiencies of 14.3%.66

To further improve these results some modifications could be introduced. For instance, great efficiencies have been achieved by substituting the I/I3 electrolyte by Co2+/Co3+ electrolyte,67 or using spiro-OMeTAD as HTL.5,38,68 Capping ligands are another important parameter since, as commented above, the presence of long chain ligands is detrimental for device efficiency. Moreover, it has been demonstrated that the nature of the capping ligands will influence the interaction between the perovskite NCs and the dye or the TiO2 interface, therefore the use of shorter or more adequate ligands could improve the device efficiency.69 Not only that, if co-sensitization is the key to boost performance, other dyes such as Ru complex N3 have also shown improvements combined with other NCs DSSCs.70

Summary

According to the cell performance parameters of the different studies introducing tin-perovskite NCs in solar cells (Table 3), the most interesting approach seems to be the solvothermal synthesis of CsSnX3 rod-shaped nanocrystals and the use of TiO2 as ETL and spiro-OMeTAD as HTL, that delivers a maximum efficiency (approx. 13%).63 The comparison of the Voc found in this study for CsSnI3 (0.87 V) with the value found for CsSnI3 in ref. 58 (0.42 V) points to a non-optimum energy alignment among the active material and the transport layers in the latter.
Table 3 Summary of solar cell performance parameters of champion devices fabricated with tin-based perovskite nanocrystals. Open circuit voltage (Voc), short circuit current density (Jsc), fill factor (FF), and power conversion efficiency (PCE)
NCs V oc (V) J sc (mA cm−2) FF PCE (%) Ref.
CsSnI3 + TPPi 0.42 23.79 0.42 4.13 58
CsSnCl3 0.87 19.82 0.56 9.66 63
CsSnBr3 0.85 21.23 0.58 10.46 63
CsSnI3 0.87 23.2 0.65 12.96 63
MASnBr3 0.53 0.62 0.48 0.155 64
MASnBr2I 0.56 0.87 0.65 0.322 64
MASnBrI2 0.52 0.70 0.56 0.202 64
MASnI3 0.46 0.55 0.43 0.106 64


In the case of the hybrid MASnBr3−xIx perovskites, the low currents obtained in the DSSC devices point to an inefficient charge transfer between the NCs–TiO2 interface and the electrolyte. As commented, the substitution of the long chain organic ligands might lead to a better contact between the nanocrystals and the electrolyte. Additionally, the introduction of these NCs in other cell configurations, like the one used in ref. 63, could provide better efficiencies and would allow a better comparison among the different materials and synthetic strategies.

Germanium-based perovskites

Germanium also belongs to group 14 in the periodic table, together with Pb and Sn, and shares the ns2np2 external electronic configuration (4s2 for Ge2+). Therefore, analogous properties close to those observed in Pb-based perovskite materials are expected but using a non-toxic relatively abundant material. In spite of this, Ge has received little attention as light absorber for solar cells, most likely because of the significant tendency of Ge2+ ions to oxidize to Ge4+.

Some theoretical calculations have predicted promising efficiencies for Ge perovskite solar cells. For instance, 1D-Solar Cell Capacitance Simulator (1D-SCAPS) simulations estimate a 23.58% efficiency for a CH3NH3GeI3 (MAGeI3) PSC employing CuSbS2 as HTL, and by introducing Shockley–Queisser maximum solar cell efficiency (S–Q) and Spectroscopic Limited Maximum Efficiency (SLME) models in DFT calculations a theoretical value of 27.9% PCE is obtained for a CsGeI3 PSC.71,72 This reflects their great optical properties and the potential application of germanium-based materials in photovoltaic devices. Based on these good results some Ge-based bulk PSCs have been fabricated. CsGeI3 solar cells achieved an initial efficiency of 0.11%,73 which was further improved up to 3% and patented by Huang et al.74 Moreover, germanium was included in a mixed all-inorganic tin-PSC, CsSn0.5Ge0.5I3, reaching an efficiency of 7.11% as well as enhanced stability due to the growth of a Sn-containing GeO2 native passivation oxide layer (formed spontaneously when exposed to air).75 Hybrid organic inorganic materials, like MAGeI3, have also been tested delivering a 0.2% efficiency,73 which was later increased up to a 0.56% by introducing a 10% of bromide in the composition (MAGeI2.7Br0.3).76 Additionally, germanium has been used in a formamidinium antimony-PSC (FA4GeSbCl12) achieving a 4.7% efficiency.77 Finally, a FA and MA Ge-doped Sn perovskite, FA0.75MA0.25Sn1−xGexI3, was used as active layer leading to an efficiency of 7.9% when a 5% of Ge was present.78 In summary, thin-film photovoltaics using Ge-perovskites are scarce and have reached efficiency values up to 3%; however, when combined with other non-toxic elements such as Sn or Sb, the efficiency is greatly increased, attributed to an improved passivation, suppression of recombination, and reduction of trap states, which improve carrier dynamics.75,77,78

As the oxidation of Ge2+ to Ge4+ in air is quite straightforward, reports of Ge perovskite NCs applied in photovoltaics are limited, as spontaneous oxidation is favoured in NCs because of their high surface/volume ratio. Although there are some reports of Ge perovskite NCs synthesis,42,79 very few address their use in solar cells.80

CsGeX3 nanocrystals (X = Cl, Br, I)

A simple solvothermal method was proposed to synthesize rod-shaped CsGeX3 (X = Cl, Br, I) NCs using diethylenetriamine (DIEN) and TOPO as capping ligands. Fig. 4 shows the current density–voltage (JV) curves for solar cells fabricated with the different halides, using TiO2 as electron transport layer and spiro-OMeTAD as hole transport layer.
image file: d1ma00245g-f4.tif
Fig. 4 (A) JV characteristics of CsGeI3 (blue), CsGeBr3 (red), and CsGeCl3 (black) solar cells. The inset shows a picture of a solar cell. (B) Incident Photon-to-electron Conversion Efficiency (IPCE) of CsGeX3 perovskite devices with different halides. Reproduced from ref. 80 with permission from the Royal Society of Chemistry. (RSC, RSC Advances).

Results are shown in Table 4. Iodide QRs show the highest efficiency, closely followed by the bromide ones, probably due to their more adequate band gap.80 The obtained currents are very encouraging and the strategies to improve efficiency should focus on improving Voc and FF. In that sense, it would be interesting to explore alternative transport layers. In any case this result is very promising since the 5% efficiency obtained with CsGeI3 NCs surpasses the efficiency obtained in CsGeI3 bulk PSC (0.11% and 3%).73,74 However, there is room for improvement; devices based on other inorganic perovskite NCs such as CsPbI3 NCs achieved an efficiency up to 16.07% and the analogous Sn NCs (CsSnI3 QRs) offered an efficiency of 12.96%.63 As stated above, Ge2+ inert pair effect is less prominent than in Sn or Pb; therefore, its tendency to oxidize to Ge4+ is greater. This instability is a major concern for Ge-based perovskites and one possible solution would be the addition of antioxidant compounds. As described in the previous section, this strategy has successfully been explored in Sn materials where the addition of edamine, pyrazine, triphenyl phosphite, or SnI2 excess improved the device stability.47,49,58 Moreover, the use of CuSbS2 as HTL instead of spiro-OMeTAD could be a better match for this material.71

Table 4 Band gap (Eg) of CsGeX3 (X = Cl, Br, I) NCs and solar cell performance parameters of devices fabricated with them. Band gap values have been calculated from absorption spectra. Extracted from ref. 80
QRs E g (eV) V oc (V) J sc (mA cm−2) FF PCE (%)
CsGeCl3 2 0.35 18.57 0.40 2.57
CsGeBr3 1.9 0.49 19.49 0.52 4.92
CsGeI3 1.8 0.52 18.78 0.51 4.94


Bismuth-based perovskites

Bismuth perovskites have been studied as potential substitutes of lead perovskites in solar cells. Bismuth(III) is a trivalent metal cation isoelectronic with lead(II) (both Bi3+ and Pb2+ have a 6s26p0 electronic configuration) and their compounds share similar properties. In spite of being a heavy metal, it is considered as a non-toxic element even used in biomedicine.81 Additionally bismuth materials have shown exceptional stability in ambient conditions. Bismuth perovskite solar cells maintained their composition and structural integrity after 72 h under moisture conditions at 100 °C, while Pb devices showed decomposition after 72 h in air at 60 °C.82 Not only that, even bismuth doping of lead perovskites induce an improvement in stability. Fan Bai et al. reported a mixed perovskite α-CsPb1−xBixI3 with an efficiency of 13.21% and a significant improvement of the durability (around 70% of the efficiency is maintained after 168 h).83

Different examples of bismuth-perovskite solar cells have been reported, such as (CH3NH3)3Bi2I9 (MA3Bi2I9) PSC fabricated by vapour deposition that achieved a 3.17% efficiency.84 Additionally, all-inorganic perovskite solar cells like Cs3Bi2I9, employing CuI as HTL and TiO2 as ETL, led to an efficiency of 3.20%.85 One year later, using ZnO instead of TiO2, the efficiency was enhanced up to 9.20%.86 BiI3 was tested in thin-film solar cell leading to an efficiency of 1.21%15 that has recently increased to 1.33% in a device with V2O5 as HTL and ZnO as ETL.87 Other Bi-based perovskite materials are the silver bismuth iodide family, with a maximum efficiency of 4.3% obtained for Ag3BiI6,28 or double perovskites (A2M+M3+X6), where one M+ and one M3+ cations substitute two Pb2+ cations. Cs2AgBiBr6 films deposited by vacuum sublimation have delivered an efficiency of 1.41%, and 2.51% for films obtained by spin-coating onto a TiO2 layer.88 Recently, the introduction of a N719 dye interlayer between the Cs2AgBiBr6 and spiro-OMeTAD layers has shown to enhance the efficiency to 2.84%, also improving the stability under ambient conditions.89 Finally, a bulk heterojunction perovskite solar cell with the photoactive layer consisting of Cs3Bi2I9 and Ag3Bi2I9 has led to a 3.6% efficiency.90 Although these are promising results, bismuth-perovskites suffer from the presence of a high number of defects that induce non-radiative recombination of charges and decrease the power conversion efficiency.10,91

In the last years several bismuth perovskite NCs have been synthesized and their optical properties have been studied showing good absorption and emissive properties, with PLQY as high as 62%.92 However, in spite of these promising optical properties, only a few examples of Bi-perovskite NCs have been used to fabricate solar devices. In this section, studies focusing on Cs3Bi2I9, Cs2AgBiBr6, KBaTeBiO6 NCs, and Bi13S18I2 nanorods are discussed.

Cs3Bi2I9 nanocrystals

A3B2X9 NCs (where A = CH3NH3, Cs, or Rb, B = Bi or Sb, and X = Cl, Br, or I) were synthesized using a colloidal hot-injection method in which 1-dodecanol was added to act as solvent and capping agent. Cs3Bi2I9 NCs, with a band gap around 2 eV, were used to fabricate solar cells with SnO2 as ETL and spiro-OMeTAD as HTL. The efficiency was 0.0103%,93 which is far from the 9.2% of the bulk analogue.86 However, in the bulk analogue, the PCE was enhanced by substituting spiro-OMeTAD by CuI as HTL.85,86 By changing the HTL or the ETL in Cs3Bi2I9 NCs solar cells the efficiency could also be improved. Moreover, the dodecanol chains on the surface of the NCs could be replaced following a ligand exchange process, which may improve the optical properties and charge transport.4,94,95

Cs2AgBiBr6 nanocrystals

Employing a colloidal synthesis route, Cs2AgBiBr6 double perovskite NCs were synthesized and deposited as thin-films, obtaining stable absorbing layers for PSC. The colloidal stability can be attributed to the surface passivation treatment with oleylamine, oleic acid, and trioctylphosphine. These ligands were substituted by bromide ions after treatment with TBAB (tetrabutylammonium bromide) during film fabrication. The Cs2AgBiBr6 NCs absorber layer, indirect band gap of 2.28 eV, was sandwiched between compact TiO2 and spiro-OMeTAD as the electron and hole transport material, respectively. The best performing device, obtained for NCs with optimum size (7.6 nm), exhibited a 0.46% efficiency. Additionally, larger NCs were also synthesized and tested obtaining a lower value of 0.028%, attributed to problems in the morphology of the film.96 These values are low when compared to previous reports for the analogous bulk material which delivered efficiencies of 2.51%. The underperformance of these devices has been attributed to the low charge carrier mobility, trap-assisted recombination and poor charge collection. More research is needed in the optimization of the energy levels between NCs and transport layers; for instance, the presence of ethylammonium has been proved to enhance the charge transport by adjusting the energy levels in Sn-based PSC.52

KBaTeBiO6 nanocrystals

By using computational calculations, it was predicted that KBaTeBiO6 (double perovskite oxide) is a potential non-toxic candidate for photovoltaic applications. The calculated maximum efficiency was around 4% for a 1 μm thick film, which could be tuned by changing the cation stoichiometry in the material. Following a simple wet-chemistry route and mixing solutions of the respective precursors, KNO3, Ba(NO3)2, Bi(NO3)3·5H2O and Te(OH)6 in the adequate proportions, KBaTeBiO6 NCs were obtained. The NCs (direct band gap of 1.88 eV), were dispersed in ethanol and water with and without binders (terpineol and ethyl cellulose), drop-casted on top of a TiO2 electrode, and used as sensitizer in a DSSC. The average efficiency obtained was 0.04%, with a best efficiency of 0.06% for the material dispersed without binders.97 This may appear as a very low value, especially as compared to the 14.3% record efficiency for DSSCs,66 and to the 6.5% achieved employing MAPbI3 as sensitizer in DSSC.98 However, KBaTeBiO6 NCs show better material stability than bismuth-based halide perovskites and their solar cells show similar performance to those based on high quality thin films of other inorganic oxide perovskites. Furthermore, the study and control of defects including oxygen vacancies, cation nonstoichiometry, and disorder in KBaTeBiO6 will be a crucial task to achieve optimal performance from these semiconductors.

Bi13S18I2 nanocrystals

Bi13S18I2 NCs were synthesized following a solvothermal method, mixing the precursors BiI3, thiourea (CH4N2S), and CH3NH3I (MAI) in ethylene glycol at 195 °C in a 2[thin space (1/6-em)]:[thin space (1/6-em)]4[thin space (1/6-em)]:[thin space (1/6-em)]3 ratio, respectively. The obtained nanorods had a diameter of 50 nm and a band gap of 0.75 eV,100 a value smaller than the ideal band gap for a single p–n junction solar cell.99

Bi13S18I2 nanorods were used as sensitizer in DSSC (Fig. 5A), and a maximum efficiency of 0.85% was achieved, showing low variability among the 8 different devices (Fig. 5B).100 The low PCE is due to the low current and fill factor values, which may be improved optimising the thickness of Bi13S18I2 and TiO2 films, or using a different electrolyte or hole transport material. Along this line, the use of polysulfide electrolytes led to better efficiencies for NCs DSSCs.101


image file: d1ma00245g-f5.tif
Fig. 5 (A) Scheme of the Bi13S18I2 NCs solar cell structure. (B) JV curves of eight Bi13S18I2 solar cells. Reproduced from ref. 100 with permission from the Royal Society of Chemistry. (RSC, Journal of Materials Chemistry C).

Summary

Table 5 summarizes the solar cell parameters of the Bi-perovskite NCs devices. Cs3Bi2I9 and Cs2AgBiBr6 NCs were synthesized using a colloidal synthesis that provides a precise control over the composition and size of the final material. The devices fabricated with these NCs used an almost identical solar cell structure with compact TiO2 and spiro-OMeTAD as transport layers.93,96 However, the device fabricated with Cs2AgBiBr6 NCs,96 that follows a ligand exchange process, showed better currents and Voc, pointing to the effectiveness of this approach in improving charge transport. A different selection of final ligands could further improve charge transport and adjust energy levels between the absorbing and transport layers, leading to better efficiencies.
Table 5 Summary of solar cell performance parameters of champion devices fabricated with bismuth-based perovskite nanocrystals. Open circuit voltage (Voc), short circuit current density (Jsc), fill factor (FF), and power conversion efficiency (PCE)
NCs V oc (V) J sc (mA cm−2) FF PCE (%) Ref.
Cs3Bi2I9 0.22 0.14 0.34 0.01 93
Cs2AgBiBr6 0.80 1.17 0.49 0.46 96
KBaTeBiO6 0.54 0.09 0.58 0.06 97
Bi13S18I2 0.58 3.82 0.38 0.85 100


KBaTeBiO6 and Bi13S18I2 NCs have been used as dyes in DSSC devices employing the same counter electrode, solar cell area (0.25 cm2), and a similar electrolyte, based on the I/I3 couple.97,100 The device incorporating the KBaTeBiO6 NCs showed very low current probably because of the presence of defects in the crystalline structure, coming from the lack of control over the composition of the mixed oxide, and on the surface, originated by the absence of passivating agents. Better results are obtained with the Bi13S18I2 NCs, synthesized using a simple solvothermal method. It would be interesting to explore the introduction of this material in a n–i–p solar cell structure to compare with ref. 93 and 96.

Antimony-based perovskites

Antimony belongs to the same group as bismuth and, consequently, Sb-perovskites have also been proposed as non-toxic alternative to lead-based perovskites. Like Bi3+, Sb3+ cations are isoelectronic to Pb2+ and, usually, form perovskites with the formula A3Sb2X9 (where A = MA, Cs or Rb and X = Cl, Br or I). Similarly, to Bi-perovskites, they exhibit high absorption coefficients, small effective masses (facilitating mobility) and suitable band gaps for photovoltaic applications (usually between 1 eV and 2 eV). Moreover, their properties can be tuned depending on the structure (0D or 2D layered).102 Antimony can be a good alternative to other non-toxic materials mentioned in this text; it does not suffer from oxidation processes like Sn or Ge, and is more abundant in the earth-crust than Bi.103 In spite of this, Sb-perovskite reports are less common than those focusing on Sn or Bi, probably because they suffer from a high presence of deep defects that act as recombination centres.10,104

Some bulk Sb-perovskite materials have been synthesized, characterized, and introduced as light harvesters in solar cells. In 2016, 0D methylammonium MA3Sb2I9 thin-film solar cells were fabricated achieving a power conversion efficiency of 0.5%.105 Two years later, it was demonstrated that 0D MA3Sb2I9 perovskite had an indirect band gap, reduced carrier transport, and their films suffered from nonradiative recombination and it was suggested that a 2D layered structure could produce better results. This 2D-perovskite could be easily obtained by adding chloride to MA3Sb2I9 films. Thus, 2D MA3Sb2ClxI9−x films were introduced in solar cells achieving an efficiency of 2.19%, the best result so far for Sb-only perovskite solar cells.106 Another type of 2D antimony-perovskite, Rb3Sb2I9, led to a maximum efficiency of 0.66%.104

In addition to these studies on bulk Sb-perovskites, antimony perovskite nanocrystals have also received some attention. Cs3Sb2X9 (X = Cl, Br, I) NCs have been synthesized and stabilized with oleic acid and octadecene capping ligands. The photoluminescence quantum yields are 11% for Cs3Sb2Cl9, 46% for Cs3Sb2Br9, and 23% for Cs3Sb2I9 NCs, and the band gaps are 3.35, 3.02, and 2.21 eV, respectively.107 In spite of having the higher PLQY value, Cs3Sb2Br9 NCs band gap is not optimal for solar cells. Nevertheless, the band gap could be tuned by modifying the nanocrystal diameter and, additionally, Sb-perovskites can be used for other applications. Furthermore, as discussed in the next section, (NH4)3Sb2IxBr9−x NCs have been used as light absorbers in solar cells.

(NH4)3Sb2IxBr9−x nanocrystals

(NH4)3Sb2IxBr9−x NCs were synthesized following an anti-solvent vapor-assisted crystallization method using ethanol as solvent, considered as a low-cost, hypotoxic, and environmentally friendly solvent. NCs with 54 nm diameter and different halide compositions were characterized and incorporated in photovoltaic devices. Table 6 collects the direct band gap of the NCs and the power conversion efficiencies of the solar cells fabricated with them. The structure of the devices was ITO/PEDOT:PSS/(NH4)3Sb2IxBr9−x NCs/PC61BM/Al, where PEDOT:PSS is the electron transport layer, and PC61BM the hole transport layer. The stability of the best performing device, employing (NH4)3Sb2I9 NCs, was tested. The film became colourless and the device showed no performance after storage in air for 2 days, but when stored in a glovebox for 40 days, 80% of the efficiency was maintained, demonstrating that device stability can be improved via encapsulation.108
Table 6 Band gap (Eg) of NCs and solar cell performance parameters of the solar cells fabricated with them. Extracted from ref. 108
NCs E g (eV) V oc (V) J sc (mA cm−2) FF PCE (%)
(NH4)3Sb2Br9 2.78 0.29 0.09 0.28 0.01
(NH4)3Sb2I3Br6 2.66 0.67 0.20 0.44 0.06
(NH4)3Sb2I6Br3 2.49 0.76 0.77 0.32 0.19
(NH4)3Sb2I9 2.27 1.03 1.15 0.43 0.51


The iodide (NH4)3Sb2I9 NCs provided the best performance parameters, with a 0.51% efficiency, probably due to the most adequate band gap and a more optimum band alignment between the active and the transport layers. The low currents and FF point to problems in charge transport and extraction, which could be improved with a better film morphology and the use of alternative transport layers. The best efficiency is similar to the highest value obtained for Bi perovskite NCs (0.85% for Bi13S18I2);100 however, the different stoichiometry and composition make them hardly comparable. The efficiency obtained is still far from other tin or lead-based NCs perovskite solar cells, but close to values obtained for bulk inorganic Sb-perovskites Rb3Sb2I9 and 0D MA3Sb2I9 thin-films mentioned above (0.66% and 0.5% respectively), and still inferior to the best-performing antimony solar cell, 2D MA3Sb2ClxI9−x (2.2%). As a final remark concerning Sb-perovskites, a recent study suggests that Sb-perovskites have much deeper defects than Pb-perovskite NCs, which can reduce significantly the efficiency of the photovoltaic devices.109

Conclusions

Non-toxic perovskites are becoming more relevant in photovoltaics due to the raising concerns about lead toxicity. Even though the efficiencies of these non-toxic materials are slightly behind lead, they seem to be particularly appealing for specific applications such as indoor and wearable photovoltaics, where safety is of primary importance.

The efficiency of lead perovskite cells has grown from 3.8% in 2009 to current 25.5% for bulk and 16.6% for NCs. These improvements have been achieved thanks to the adjustment of the energy levels, enhanced stability, suppression of defects, surface treatments, charge transport improvement, and the use of different and more complex stoichiometries. In this sense, complex and tailored compositions are not easily achievable for bulk perovskites where synthesis and deposition are simultaneous. On the contrary, perovskite NCs offer the advantage of separating both processes, which allows a better control over the stoichiometry of the material. Although the use of non-toxic perovskite NCs in solar cells is quite recent, they have already shown promising results surpassing in some cases the efficiency values obtained for their bulk counterparts: CsSnI3 quantum rods show an efficiency of almost 13% (bulk material 7.5%), and CsGeI3 NCs an efficiency close to 5% (bulk material ≈3%). It is worth mentioning that some of the best results are already close to the efficiency obtained for lead NCs (16.6%), and the stoichiometry or solar cell structure have not been optimized.

In this review, the main issues of non-toxic perovskite NCs have been addressed. Some of the materials suffer from oxidation problems (Ge, Sn) or high number of defects (Bi, Sb) that may harm the solar device performance. In this sense, more complex compositions could be a solution to some of the aforementioned problems. For example, including in the composition edamine that acts as antioxidant cation, ethylammonium that improves charge transport, or formamide which prevents non-radiative recombination. Additionally, the addition of antioxidant additives, more adequate transport layers, different cell structures, or surface passivation treatments are other possible approaches to improve performance.

Research on non-toxic perovskite NCs is a novel field, reports incorporating these NCs in solar cells are scarce, and many alternatives remain unexplored. Indeed, in the studies here summarized, each work uses a synthetic methodology and a solar cell structure making it difficult to compare among them and select the most promising approach. Still, impressive results have already been reported showing that non-toxic NCs could be candidates to substitute lead in the near future with more research in this area.

Conflicts of interest

There are no conflicts of interest to declare.

Acknowledgements

Authors acknowledge Fundación Iberdrola España, CIBER-BBN (financed by the Instituto de Salud Carlos III with assistance from the European Regional Development Fund), the ICTS “NANBIOSIS”, Agencia Estatal de Investigación-AEI (Ref. PID2019-107893RB-I00 and PID2019-104307GB-I00), and Gobierno de Aragón (Ref. T57_20R and E47_20R) for financial support.

References

  1. NREL, Best Research-Cell Efficiency Chart, 2020.
  2. G. H. Carey, A. L. Abdelhady, Z. Ning, S. M. Thon, O. M. Bakr and E. H. Sargent, Chem. Rev., 2015, 115, 12732 Search PubMed .
  3. H. Lu, Z. Huang, M. S. Martinez, J. C. Johnson, J. M. Luther and M. C. Beard, Energy Environ. Sci., 2020, 13, 1347 Search PubMed .
  4. P. R. Brown, D. Kim, R. R. Lunt, N. Zhao, M. G. Bawendi, J. C. Grossman and V. Bulović, ACS Nano, 2014, 8, 5863 Search PubMed .
  5. M. Hao, Y. Bai, S. Zeiske, L. Ren, J. Liu, Y. Yuan, N. Zarrabi, N. Cheng, M. Ghasemi, P. Chen, M. Lyu, D. He, J. H. Yun, Y. Du, Y. Wang, S. Ding, A. Armin, P. Meredith, G. Liu, H. M. Cheng and L. Wang, Nat. Energy, 2020, 5, 79 Search PubMed .
  6. H. Yang, Y. Zhang, K. Hills-Kimball, Y. Zhou and O. Chen, Sustainable Energy Fuels, 2018, 2, 2381 Search PubMed .
  7. D. B. Mitzi, J. Chem. Soc., Dalton Trans., 2001, 1 Search PubMed .
  8. X. Li, J. Wu, S. Wang and Y. Qi, Chem. Lett., 2019, 48, 989 Search PubMed .
  9. S. A. Bretschneider, F. Laquai and M. Bonn, J. Phys. Chem. C, 2017, 121, 11201 Search PubMed .
  10. A. M. Ganose, C. N. Savory and D. O. Scanlon, Chem. Commun., 2017, 53, 20 Search PubMed .
  11. J. Bisquert and E. J. Juarez-Perez, J. Phys. Chem. Lett., 2019, 10, 5889 Search PubMed .
  12. Y. Deng, L. Jiang, L. Xu, X. Hao, S. Zhang, M. Xu, P. Zhu, S. Fu, Y. Liang, H. Yin, X. Liu, L. Bai, H. Jiang and H. Liu, Ecotoxicol. Environ. Saf., 2019, 171, 281 Search PubMed .
  13. Z. Xiao, Z. Song and Y. Yan, Adv. Mater., 2019, 31, 1 Search PubMed .
  14. Q. Zhang and Y. Yin, ACS Cent. Sci., 2018, 4, 668 Search PubMed .
  15. C. Wu, Q. Zhang, G. Liu, Z. Zhang, D. Wang, B. Qu, Z. Chen and L. Xiao, Adv. Energy Mater., 2019, 1902496 Search PubMed .
  16. X. Zhao and N. G. Park, Photonics, 2015, 2, 1139 Search PubMed .
  17. R. E. Brandt, J. R. Poindexter, P. Gorai, R. C. Kurchin, R. L. Z. Hoye, L. Nienhaus, M. W. B. Wilson, J. A. Polizzotti, R. Sereika, R. Žaltauskas, L. C. Lee, J. L. Macmanus-Driscoll, M. Bawendi, V. Stevanović and T. Buonassisi, Chem. Mater., 2017, 29, 4667 Search PubMed .
  18. L. C. Lee, T. N. Huq, J. L. Macmanus-Driscoll and R. L. Z. Hoye, APL Mater., 2018, 6, 084502 Search PubMed .
  19. A. Babayigit, H.-G. Boyen and B. Conings, MRS Energy Sustainability, 2018, 5, 15 Search PubMed .
  20. P. Su, Y. Liu, J. Zhang, C. Chen, B. Yang, C. Zhang and X. Zhao, J. Phys. Chem. Lett., 2020, 11, 2812 Search PubMed .
  21. T. Miyasaka, A. Kulkarni, G. M. Kim, S. Öz and A. K. Jena, Adv. Energy Mater., 2020, 10, 1 Search PubMed .
  22. Y. Peng, T. N. Huq, J. Mei, L. Portilla, R. A. Jagt, L. G. Occhipinti, J. L. MacManus-Driscoll, R. L. Z. Hoye and V. Pecunia, Adv. Energy Mater., 2021, 11, 2002761 Search PubMed .
  23. S. A. Hashemi, S. Ramakrishna and A. G. Aberle, Energy Environ. Sci., 2020, 13, 685 Search PubMed .
  24. X. Hou, Y. Wang, H. K. H. Lee, R. Datt, N. Uslar Miano, D. Yan, M. Li, F. Zhu, B. Hou, W. C. Tsoi and Z. Li, J. Mater. Chem. A, 2020, 8, 21503 Search PubMed .
  25. M. Lyu, J. H. Yun, P. Chen, M. Hao and L. Wang, Adv. Energy Mater., 2017, 7, 1602512 Search PubMed .
  26. L. Liang and P. Gao, Adv. Sci., 2017, 5, 1700331 Search PubMed .
  27. S. Attique, N. Ali, S. Ali, R. Khatoon, N. Li, A. Khesro, S. Rauf, S. Yang and H. Wu, Adv. Sci., 2020, 7, 1903143 Search PubMed .
  28. I. Turkevych, S. Kazaoui, E. Ito, T. Urano, K. Yamada, H. Tomiyasu, H. Yamagishi, M. Kondo and S. Aramaki, ChemSusChem, 2017, 10, 3754 Search PubMed .
  29. D. Shi, Y. Zeng and W. Shen, Sci. Rep., 2015, 5, 1 Search PubMed .
  30. T. Saga, NPG Asia Mater., 2010, 2, 96 Search PubMed .
  31. W. Ke, C. C. Stoumpos and M. G. Kanatzidis, Adv. Mater., 2019, 31, 1803230 Search PubMed .
  32. N. C. Miller and M. Bernechea, APL Mater., 2018, 8, 084503 Search PubMed .
  33. A. Swarnkar, V. K. Ravi and A. Nag, ACS Energy Lett., 2017, 2, 1089 Search PubMed .
  34. H. Siddiqui, Mater. Lett., 2019, 249, 99 Search PubMed .
  35. S. Ghosh and B. Pradhan, ChemNanoMat, 2019, 5, 300 Search PubMed .
  36. A. Kojima, K. Teshima, Y. Shirai and T. Miyasaka, J. Am. Chem. Soc., 2009, 131, 6050 Search PubMed .
  37. J. H. Im, C. R. Lee, J. W. Lee, S. W. Park and N. G. Park, Nanoscale, 2011, 3, 4088 Search PubMed .
  38. H. S. Kim, C. R. Lee, J. H. Im, K. B. Lee, T. Moehl, A. Marchioro, S. J. Moon, R. Humphry-Baker, J. H. Yum, J. E. Moser, M. Grätzel and N. G. Park, Sci. Rep., 2012, 2, 591 Search PubMed .
  39. A. Swarnkar, A. R. Marshall, E. M. Sanehira, B. D. Chernomordik, D. T. Moore, J. A. Christians, T. Chakrabarti and J. M. Luther, Science, 2016, 354, 92 Search PubMed .
  40. K. Ji, J. Yuan, F. Li, Y. Shi, X. Ling, X. Zhang, Y. Zhang, H. Lu, J. Yuan and W. Ma, J. Mater. Chem. A, 2020, 8, 8104 Search PubMed .
  41. L. Zhang, C. Kang, G. Zhang, Z. Pan, Z. Huang, S. Xu, H. Rao, H. Liu, S. Wu, X. Wu, X. Li, Z. Zhu, X. Zhong and A. K.-Y. Jen, Adv. Funct. Mater., 2020, 2005930 Search PubMed .
  42. D. Carolan, Prog. Mater. Sci., 2017, 90, 128 Search PubMed .
  43. S. F. Hoefler, G. Trimmel and T. Rath, Monatsh. Chem., 2017, 148, 795 Search PubMed .
  44. A. Abate, Joule, 2017, 1, 659 Search PubMed .
  45. W. Li, J. J. Li, J. J. Li, J. Fan, Y. Mai and L. Wang, J. Mater. Chem. A, 2016, 4, 17104 Search PubMed .
  46. T. C. Jellicoe, J. M. Richter, H. F. J. Glass, M. Tabachnyk, R. Brady, S. E. Dutton, A. Rao, R. H. Friend, D. Credgington, N. C. Greenham and M. L. Böhm, J. Am. Chem. Soc., 2016, 138, 2941 Search PubMed .
  47. T. Bin Song, T. Yokoyama, S. Aramaki and M. G. Kanatzidis, ACS Energy Lett., 2017, 2, 897 Search PubMed .
  48. T. Ye, K. Wang, Y. Hou, D. Yang, N. Smith, B. Magill, J. Yoon, R. R. H. H. Mudiyanselage, G. A. Khodaparast, K. Wang and S. Priya, J. Am. Chem. Soc., 2021, 143, 4319–4328 Search PubMed .
  49. S. J. Lee, S. S. Shin, Y. C. Kim, D. Kim, T. K. Ahn, J. H. Noh, J. Seo and S. Il Seok, J. Am. Chem. Soc., 2016, 138, 3974 Search PubMed .
  50. S. Shao, J. Liu, G. Portale, H.-H. Fang, G. R. Blake, G. H. ten Brink, L. J. A. Koster and M. A. Loi, Adv. Energy Mater., 2018, 8, 1702019 Search PubMed .
  51. M. A. Kamarudin, D. Hirotani, Z. Wang, K. Hamada, K. Nishimura, Q. Shen, T. Toyoda, S. Iikubo, T. Minemoto, K. Yoshino and S. Hayase, J. Phys. Chem. Lett., 2019, 10, 5277 Search PubMed .
  52. K. Nishimura, M. A. Kamarudin, D. Hirotani, K. Hamada, Q. Shen, S. Iikubo, T. Minemoto, K. Yoshino and S. Hayase, Nano Energy, 2020, 74, 104858 Search PubMed .
  53. W. Ke, C. C. Stoumpos, I. Spanopoulos, L. Mao, M. Chen, M. R. Wasielewski and M. G. Kanatzidis, J. Am. Chem. Soc., 2017, 139, 14800 Search PubMed .
  54. Z. Zhao, F. Gu, Y. Li, W. Sun, S. Ye, H. Rao, Z. Liu, Z. Bian and C. Huang, Adv. Sci., 2017, 4, 1700204 Search PubMed .
  55. A. Kaltzoglou, M. Antoniadou, A. G. Kontos, C. C. Stoumpos, D. Perganti, E. Siranidi, V. Raptis, K. Trohidou, V. Psycharis, M. G. Kanatzidis and P. Falaras, J. Phys. Chem. C, 2016, 120, 11777 Search PubMed .
  56. X. Qiu, B. Cao, S. Yuan, X. Chen, Z. Qiu, Y. Jiang, Q. Ye, H. Wang, H. Zeng, J. Liu and M. G. Kanatzidis, Sol. Energy Mater. Sol. Cells, 2017, 159, 227 Search PubMed .
  57. X. Qiu, Y. Jiang, H. Zhang, Z. Qiu, S. Yuan, P. Wang and B. Cao, Phys. Status Solidi RRL, 2016, 10, 587 Search PubMed .
  58. Y. Wang, J. Tu, T. Li, C. Tao, X. Deng and Z. Li, J. Mater. Chem. A, 2019, 7, 7683 Search PubMed .
  59. F. Zhang, H. Zhong, C. Chen, X. G. Wu, X. Hu, H. Huang, J. Han, B. Zou and Y. Dong, ACS Nano, 2015, 9, 4533 Search PubMed .
  60. C. H. M. Chuang, P. R. Brown, V. Bulović and M. G. Bawendi, Nat. Mater., 2014, 13, 796 Search PubMed .
  61. R. Abargues, J. Navarro, P. J. Rodríguez-Cantó, A. Maulu, J. F. Sánchez-Royo and J. P. Martínez-Pastor, Nanoscale, 2019, 11, 1978 Search PubMed .
  62. A. Salant, M. Shalom, Z. Tachan, S. Buhbut, A. Zaban and U. Banin, Nano Lett., 2012, 12, 2095 Search PubMed .
  63. L. J. Chen, C. R. Lee, Y. J. Chuang, Z. H. Wu and C. Chen, J. Phys. Chem. Lett., 2016, 7, 5028 Search PubMed .
  64. H. Xu, H. Yuan, J. Duan, Y. Zhao, Z. Jiao and Q. Tang, Electrochim. Acta, 2018, 282, 807 Search PubMed .
  65. Z. Wu, Y. Wei, Z. An, X. Chen and P. Chen, Bull. Korean Chem. Soc., 2014, 35, 1449 Search PubMed .
  66. K. Kakiage, Y. Aoyama, T. Yano, K. Oya, J. I. Fujisawa and M. Hanaya, Chem. Commun., 2015, 51, 15894 Search PubMed .
  67. S. Mathew, A. Yella, P. Gao, R. Humphry-baker, B. F. E. Curchod, N. Ashari-astani, I. Tavernelli, U. Rothlisberger, K. Nazeeruddin and M. Grätzel, Nat. Chem., 2014, 6, 242 Search PubMed .
  68. S. S. Mali, C. S. Shim and C. K. Hong, NPG Asia Mater., 2015, 7, e208 Search PubMed .
  69. S. Giménez, A. L. Rogach, A. A. Lutich, D. Gross, A. Poeschl, A. S. Susha, I. Mora-Seró, T. Lana-Villarreal and J. Bisquert, J. Appl. Phys., 2011, 110, 014314 Search PubMed .
  70. T. Ganesh, R. S. Mane, G. Cai, J. H. Chang and S. H. Han, J. Phys. Chem. C, 2009, 113, 7666 Search PubMed .
  71. A. Hima and N. Lakhdar, Opt. Mater., 2020, 99, 109607 Search PubMed .
  72. J. Qian, B. Xu and W. Tian, Org. Electron., 2016, 37, 61 Search PubMed .
  73. T. Krishnamoorthy, H. Ding, C. Yan, W. L. Leong, T. Baikie, Z. Zhang, M. Sherburne, S. Li, M. Asta, N. Mathews and S. G. Mhaisalkar, J. Mater. Chem. A, 2015, 3, 23829 Search PubMed .
  74. C. Huang, X. C. X. C. Yan, G. G. Cui, Z. Z. Liu, S. S. Pang and H. Xu, Novel Germanium-Containing Perovskite Material and Solar Cell Comprising Same, CN 201410173750, 2014 Search PubMed .
  75. M. Chen, M. G. Ju, H. F. Garces, A. D. Carl, L. K. Ono, Z. Hawash, Y. Zhang, T. Shen, Y. Qi, R. L. Grimm, D. Pacifici, X. C. Zeng, Y. Zhou and N. P. Padture, Nat. Commun., 2019, 10, 1 Search PubMed .
  76. I. Kopacic, B. Friesenbichler, S. F. Hoefler, B. Kunert, H. Plank, T. Rath and G. Trimmel, ACS Appl. Energy Mater., 2018, 1, 343 Search PubMed .
  77. W. B. Dai, S. Xu, J. Zhou, J. Hu, K. Huang and M. Xu, Sol. Energy Mater. Sol. Cells, 2019, 192, 140 Search PubMed .
  78. C. H. Ng, K. Nishimura, N. Ito, K. Hamada, D. Hirotani, Z. Wang, F. Yang, S. likubo, Q. Shen, K. Yoshino, T. Minemoto and S. Hayase, Nano Energy, 2019, 58, 130 Search PubMed .
  79. X. Wu, W. Song, Q. Li, X. Zhao, D. He and Z. Quan, Chem. – Asian J., 2018, 13, 1654 Search PubMed .
  80. L. J. Chen, RSC Adv., 2018, 8, 18396 Search PubMed .
  81. Y. Yang, R. Ouyang, L. Xu, N. Guo, W. Li, K. Feng, L. Ouyang, Z. Yang, S. Zhou and Y. Miao, J. Coord. Chem., 2015, 68, 379 Search PubMed .
  82. A. H. Slavney, T. Hu, A. M. Lindenberg and H. I. Karunadasa, J. Am. Chem. Soc., 2016, 138, 2138 Search PubMed .
  83. Y. Hu, F. Bai, X. Liu, Q. Ji, X. Miao, T. Qiu and S. Zhang, ACS Energy Lett., 2017, 2, 2219 Search PubMed .
  84. S. M. Jain, D. Phuyal, M. L. Davies, M. Li, B. Philippe, C. De Castro, Z. Qiu, J. Kim, T. Watson, W. C. Tsoi, O. Karis, H. Rensmo, G. Boschloo, T. Edvinsson and J. R. Durrant, Nano Energy, 2018, 49, 614 Search PubMed .
  85. F. Bai, Y. Hu, Y. Hu, T. Qiu, X. Miao and S. Zhang, Sol. Energy Mater. Sol. Cells, 2018, 184, 15 Search PubMed .
  86. J. H. Heo, M. H. Lee, D. H. Song, N. M. S. Aung, J.-J. Lee, C. E. Song, K.-H. Hong and S. Hyuk Im, J. Nanoelectron. Optoelectron., 2019, 13, 1764 Search PubMed .
  87. Y. Wang, X. Shi, G. Wang, J. Tong and D. Pan, J. Mater. Chem. C, 2020, 8, 14066 Search PubMed .
  88. F. Igbari, R. Wang, Z. K. Wang, X. J. Ma, Q. Wang, K. L. Wang, Y. Zhang, L. S. Liao and Y. Yang, Nano Lett., 2019, 19, 2066 Search PubMed .
  89. X. Yang, Y. Chen, P. Liu, H. Xiang, W. Wang, R. Ran, W. Zhou and Z. Shao, Adv. Funct. Mater., 2020, 30, 2001557 Search PubMed .
  90. W. Hu, X. He, Z. Fang, W. Lian, Y. Shang, X. Li, W. Zhou, M. Zhang, T. Chen, Y. Lu, L. Zhang, L. Ding and S. Yang, Nano Energy, 2020, 68, 104362 Search PubMed .
  91. B. W. Park, B. Philippe, X. Zhang, H. Rensmo, G. Boschloo and E. M. J. Johansson, Adv. Mater., 2015, 27, 6806 Search PubMed .
  92. Y. Lou, M. Fang, J. Chen and Y. Zhao, Chem. Commun., 2018, 54, 3779 Search PubMed .
  93. M. M. Yao, C. H. Jiang, J. S. Yao, K. H. Wang, C. Chen, Y. C. Yin, B. S. Zhu, T. Chen and H. Bin Yao, Inorg. Chem., 2019, 58, 11807 Search PubMed .
  94. M. Soreni-Harari, N. Yaacobi-Gross, D. Steiner, A. Aharoni, U. Banin, O. Millo and N. Tessler, Nano Lett., 2008, 8, 678 Search PubMed .
  95. M. Leng, Y. Yang, Z. Chen, W. Gao, J. Zhang, G. Niu, D. Li, H. Song, J. Zhang, S. Jin and J. Tang, Nano Lett., 2018, 18, 6076 Search PubMed .
  96. R. Ahmad, G. V. Nutan, D. Singh, G. Gupta, U. Soni, S. Sapra and R. Srivastava, Nano Res., 2021, 14, 1126 Search PubMed .
  97. A. S. Thind, S. Kavadiya, M. Kouhnavard, R. Wheelus, S. B. Cho, L. Y. Lin, C. Kacica, H. K. Mulmudi, K. A. Unocic, A. Y. Borisevich, G. Pilania, P. Biswas and R. Mishra, Chem. Mater., 2019, 31, 4769 Search PubMed .
  98. J. H. Im, C. R. Lee, J. W. Lee, S. W. Park and N. G. Park, Nanoscale, 2011, 3, 4088 Search PubMed .
  99. W. Shockley and H. J. Queisser, J. Appl. Phys., 1961, 32, 510 Search PubMed .
  100. S. Li, L. Xu, X. Kong, T. Kusunose, N. Tsurumachi and Q. Feng, J. Mater. Chem. C, 2020, 8, 3821 Search PubMed .
  101. S. S. Mali, J. V. Patil, H. Kim, P. S. Patil and C. K. Hong, Nanomaterials for Solar Cell Applications, Elsevier, 2019, pp. 513–555 Search PubMed .
  102. B. Saparov, F. Hong, J. P. Sun, H. S. Duan, W. Meng, S. Cameron, I. G. Hill, Y. Yan and D. B. Mitzi, Chem. Mater., 2015, 27, 5622 Search PubMed .
  103. N. N. Greenwood and A. Earnshaw, Chemical Element, Elsevier, 1997, pp. 547–599 Search PubMed .
  104. P. C. Harikesh, H. K. Mulmudi, B. Ghosh, T. W. Goh, Y. T. Teng, K. Thirumal, M. Lockrey, K. Weber, T. M. Koh, S. Li, S. Mhaisalkar and N. Mathews, Chem. Mater., 2016, 28, 7496 Search PubMed .
  105. J. C. Hebig, I. Kühn, J. Flohre and T. Kirchartz, ACS Energy Lett., 2016, 1, 309 Search PubMed .
  106. F. Jiang, D. Yang, Y. Jiang, T. Liu, X. Zhao, Y. Ming, B. Luo, F. Qin, J. Fan, H. Han, L. Zhang and Y. Zhou, J. Am. Chem. Soc., 2018, 140, 1019 Search PubMed .
  107. J. Zhang, Y. Yang, H. Deng, U. Farooq, X. Yang, J. Khan, J. Tang and H. Song, ACS Nano, 2017, 11, 9294 Search PubMed .
  108. C. Zuo and L. Ding, Angew. Chem., Int. Ed., 2017, 56, 6528 Search PubMed .
  109. J. Pal, S. Manna, A. Mondal, S. Das, K. V. Adarsh and A. Nag, Angew. Chem., Int. Ed., 2017, 56, 14187 Search PubMed .

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