1 Introduction
Perovskite is a general term for a class of crystal structures with formula of ABX
3, which was named in 1830s by Gustav Rose in honor of Russian mineralogist, L. A. Perovski [
1]. Those perovskite crystals have a similar crystal structure as that of calcium titanate (CaTiO
3). The first inorganic halide perovskite cesium lead halide (CsPbX
3) (X = Cl
-, Br
- or I
-) and the first organic-inorganic hybrid perovskite (OIHP) methylammonium lead halide (MAPbX
3) (
; X = Cl
-, Br
- or I
-) were reported in 1958 and 1978, by Moller [
2] and Weber [
3], respectively. In 1990s, Mitzi and coworkers extended the OIHP family with 2D perovskite structure and applied the 2D perovskite to thin film transistor and light-emitting diodes (LEDs) [
4-
6]. However, OIHP did not receive broad attention until 2009 when the first OIHP sensitized solar cells were reported by Miyasaka
et al. [
7] with MAPbBr
3 and MAPbI
3 as the “dyes”. The ABX
3 structure of perovskite was composed by corner shared [BX
6]
4- octahedrons along with A
+ cation filling the voids, as shown in Fig. 1(a) [
8]. The structure stability of ABX
3 can be evaluated by Goldschmidt’s tolerance factor
and the octahedral factor
, where
rA,
rB, and
rX are the ionic radii of the corresponding ions [
9], respectively. To achieve 3D perovskite structure of ABX
3, t and
μ should empirically satisfy
and
, respectively. Thus, when the radii of A cation excessed a critical size, low-dimensional perovskite structures (0D, 1D and 2D) would form [
10,
11]. The 2D perovskites can be categorized by the cutting plane of 3D structure as shown in Fig. 1(c) [
12,
13]. For 2D OIHP, the Dion–Jacobson (DJ) phases were distinguished from the Ruddlesden–Popper (RP) phases [
14], where DJ phases possess divalent long-chain cation and inorganic perovskite slabs show little displacement between each other. This review will mainly focus on the controlled formation of (100)-oriented 2D OIHP, which can be expressed as
or
, where A′ and A″ are 1+ and 2+ valent aromatic or aliphatic alkyl ammonium cations, respectively. The ammonium cations slice the 3D perovskite phase ABX
3 into quantum wells (QWs) with inorganic BX
6 octahedrons layer number of
n.
The rapid development of perovskite solar cells promoted the research of perovskite optoelectronic devices such as LEDs [
15-
17], photodetectors [
18-
24], field effect transistors [
25-
27] and other photonic devices [
28]. However, the instability of 3D perovskite impeded its commercialization [
29-
32]. To improve the intrinsic stability of hybrid perovskites, RP perovskite combined both high performance and stability gradually becomes the frontier of current research. First principles calculation showed that the formation energy of RP perovskite decreased with increasing of layer number
n [
33], which predicted that better thermal dynamic stability of RP perovskite than 3D perovskite. Bulky hydrophobic ammonium cations can cause steric effects and strain the Pb-I bonds at the surface, which effectively hinders the diffusion of water molecules [
34]. The improved stability against moisture in 2D perovskites than that of MAPbI
3 has been demonstrated in the cases of PEA
2Ma
n-1Pb
nI
3n+1 (PEA
+: phenylethylammonium) [
35] and BA
2Ma
n-1Pb
nI
3n+1 (BA
+:
n-butylammmonium) [
36]. Moreover, the tunable bandgap and the higher exciton binding energy of 2D perovskite enabled its application to LEDs [
37,
38]. However, the power conversion efficiency of solar cells based on 2D perovskite still lagged behind that of 3D perovskite solar cells, resulting from inferior charge transport efficiency. Since the insulating organic spacing layers sandwiched between BX
6 octahedrons layers cause significant anisotropic charge transporting in RP perovskites, vertically or horizontally orientated QWs of RP perovskite were particularly suitable for optoelectronic device with different configurations and functions. Therefore, the orientations of 2D perovskite crystal need to be well controlled to satisfy the different charge transport demands. This review aimed to summarize the recent advances in controlling the crystallization of 2D perovskite.
2 Tunable composition and bandgap of 2D perovskites
For 2D perovskite with formula of
or A″A
n-1B
nX3
n+1, considerable researches have been devoted to the exploring of new 2D materials intermediated by different A′ cations. The employed long-chain cations A′ were well summarized in Ref. [
13]. Replacing the cations on A′ or A″ site does not contribute directly to the electronic structures of 2D perovskites. According to first principle calculation, the conduction band minimum of MAPbI
3 is mainly composed of nonbonding 6p-orbitals of lead (Pb) and the valence band maximum mainly comes from the anti-bonding of the hybridized Pb 6s and iodine (I) 5p orbitals. The MA
+ cation just functioned as charge compensator and influenced the band gap indirectly by size effect, i.e., A
+ cation usually affect the metal-halide-metal bond angle with its volume [
39,
40]. Although the long chain cations also don’t contribute directly to the formation of perovskite band structures, they can subtly influence the electronic structure of perovskites and hence their photoluminescence (PL) peak position by: (i) distorting the inorganic lattice and change the electron cloud overlapping between Pb-I bonds [
41]; (ii) the strong quantum and dielectric confinement caused by the intrinsic 2D crystal structures of RP perovskites or the morphological dimensions, which cause the band gap to increase. Taking BA
+ as long-chain cation as example, the band gap increased from 1.59 eV for MAPbI
3 to 1.85 eV for BA
2MA
3Pb
4I
13 and then to 2.35 eV for BA
2PbI
4 [
37]. The exciton binding energy
can be obtained by the difference in energy of the absorption edge to the emission maximum as shown in Figs. 2(a) and (b). It was found that the
EB of 2D perovskite increases from 10 meV to 80 meV with decreasing
n from 4 to 1 [
37]. Besides layer number
n, both metal and halide ions can also modify the band gap of RP perovskites, as shown in Figs. 2(c) and (d) [
42]. Similar with BA
2Ma
n-1Pb
nI
3n+1, the band gap modification by layer number was also reported for POEA
2Ma
n-1Pb
nBr
3n+1 (POEA
+: 2-phenoxyethylamine) [
43] and 2D MAPbBr
3 nanoplates [
44]. Controlling the average layer number (
) of 2D perovskite is usually achieved by adding different amount of long-chain cations in precursor solution [
37,
43,
45] or in anti-solution [
44]. For the long-chain cation, the high dipole moment 2,2,2-trifluoroethylamine cations might attract charges, in which way, the exciton binding energy of RP perovskite could be reduced [
46]. Moreover, when the distance between neighboring inorganic layers was shorten by applying small propane-1, 3-diammonium cations, a weaker quantum confinement was proposed, which might enable the efficient charge transport between neighboring inorganic layers [
47].
3 Controlled thin-film orientation
3.1 Out-of-plane orientation
Out-of-plane (OP) orientation is defined as the vertical alignment of QWs, which are composed by inorganic BX
6 octahedrons layer, with respect to the plane of the substrates [as shown in Fig. 3(a)] [
48]. Since the charge transport is limited within the QWs, the OP orientation of QWs of RP perovskites is quite desirable for high efficient vertical-structure-based optoelectronic devices, such as perovskite solar cells. For the first demonstration of RP perovskite solar cells (PSCs), the power conversion efficiency (PCE) was modest 4.73% [
35]. Later, RP PSCs based on BA
2Ma
n-1Pb
nI
3n+1 with a similar PCE of 4.02% was reported [
36]. In those studies, mixed solvent of nitromethane/acetone [
35] or a high concentration of precursor solution (1.8 M Pb
2+) [
36] was adopted, X-ray diffraction (XRD) patterns demonstrate the presence of RP perovskite with OP orientation since clear (111) and (202) diffraction peaks were observed. Probably, the inferior short circuit current (
Jsc) and fill factor (FF), which limited the PCEs of the early RP PSCs, is attributed to the non-ideal orientation regions or misalignment of QWs, as shown in Figs. 3(c) and (d) [
49,
50].
In 2016, a dramatically improved PCE of 12.5% for RP perovskite solar cells based on BA
2Ma
n-1Pb
nI
3n+1 was achieved by hot-casting method [
48]. Preferential OP orientation of RP perovskite was supported by grazing-incidence wide-angle X-ray scattering (GIWAXS) [as shown in Fig. 3(b)] for the first time [
48]. This hot casting method then initiated a lot of related investigations with a purpose of further improving the solar cell performance. By partially replacing MA
+ with FA
+ (formamidinium) [
51] or Cs
+ (cesium) [
52], the PCEs of BA
2MA
3Pb
4I
13 perovskite solar cells were further improved to 12.8% and 13.7%, respectively. All the achievements suggested that the RP perovskite can adopt an OP orientation and offer a promising charge transport and hence a high PCE. After this encouraging discovery, an increasing number of methods beyond hot-casting method have been developed. It should be emphasized that applying additives such as such as HI [
53,
54], NH
4SCN [
55-
57], MACl [
58,
59], or solvent engineering [
49,
60,
61] has been found to also enable OP orientation. Apart from the different methods to achieve OP orientation of RP perovskite, some common results were shared by different reports. When the high concentration of precursor solution was spin-coated at room temperature (RT), in-plane (IP) orientation was observed for BA
2Ma
n-1Pb
nI
3n+1 and OP orientation was showed for BA
2Ma
n-1Pb
nI
3n+1 perovskite film [
36]. IP orientation preference for low layer number
was also observed for hot-casting method [
52]. The orientation preference was inferred to the competition between the BA ions, which try to confine the growth within the planar layer, and the MA ions, which try to expand the perovskite QWs growth outside the layer [
36]. For RT spin-coated ThMA
2MA
2Pb
3I
10 (ThMA
+: 2-thiophenemethylammonium), a dense web of nanorod-like film was formed when 0.33 molar ratio of MACl/Pb
2+ was added [
59]. The nanorod-like crystals were also observed for BA
0.05(FA
0.83Cs
0.17)
0.95Pb(I
0.8Br
0.2)
3 film with HI as additive [
62]. The nanorod-like crystals were regarded as OP oriented RP perovskite [
59,
62]. For hot-casting method, appropriate amount of dimethyl sulfoxide (DMSO) in perovskite precursor solution promote OP orientation of BA
2Ma
n-1Pb
nI
3n+1 perovskite [
52,
63,
64]. When 6.7 vol% of DMSO was added into dimethylformamide (DMF) as solvent, and meanwhile 0.1 molar ratio of MACl/Pb
2+ was added, OP orientation of PEA
2MA
3Pb
4I
13 was achieved by RT spin-coating method [
58]. When dimethylacetamide (DMAc) was applied as solvent, the nucleation and crystal growth was found to arising from the liquid–air interface [
49]. The top-down crystal growth process was also observed when BA
2MA
3Pb
4I
13 perovskite DMF precursor solution was deposited on PEDOT substrate at 50 °C [
65]. On the other hand, for hot-casting method, a bottom to top crystallization process initiated by bonding of BA
2MA
3Pb
4I
13 perovskite with TiO
2 was also proposed as an alternative explanation [
64]. When both MACl as additive and hot-casting method was applied for (3BBA)
2Ma
n-1Pb
nI
3n+1 (
, 3BBA
+: 3-bromobenzylammonium) film, perovskite grains grown perpendicular to the substrate at the bottom region of the film was observed from cross-sectional scanning transmission electron microscope (STEM) [
66]. For NH
4SCN additive, OP orientation was achieved for both PEA
2Ma
n-1Pb
nI
3n+1 (
) [
55] and BA
2Ma
n-1Pb
nI
3n+1 [
57]. Moreover, NH
4SCN can more effectively drive the PEA
2MA
4Pb
5I
16 thin film into a vertically orientated 2D structure [
56]. Detailed information about PSCs based on OP oriented small-
RP perovskite mentioned above was summarized in Table 1.
Though many strategies for facilitating the OP orientation of RP perovskite have been reported, the in-depth understanding of the mechanism about OP orientation is still sparse. For the IP orientation of BA
2Ma
n-1Pb
nI
3n+1 [
36], the competition mechanism between the BA
+ and MA
+ ions on orientation was left less explained. For the nucleation and crystal growth initiated from the liquid–air interface [
49], it was observed that a low supersaturation of perovskite precursor solution beneath the nucleation at the liquid-air interface was necessary to crystallize vertically oriented thin films [
67], however the driving force for the OP orientation is still unknown. For the proposed bottom to top crystallization process [
64], the proposed mechanism cannot be used to explain the OP orientation of RP perovskite on poly(3,4-ethylenedioxythiophene) (PEDOT) substrate [
48] or nickel oxide (NiO
x) substrate [
60], where the bonding of BA
2MA
3Pb
4I
13 perovskite with TiO
2 was absent. Therefore, the most favoured grow direction of RP perovskite (top-down or bottom-up) is also confusing. The difficulty for understanding the mechanism of OP orientation lies in the in-situ characterization of the crystallization process during the drying of precursor solution. In-situ GIWAXS was applied for characterization of the crystallization process of RP perovskite deposited by hot-casting [
64]. However, the crystallization process was still too fast to be observed.
3.2 In-plane orientation
For polycrystalline film, RT spin-coated PentA
2Ma
n-1-Pb
nI
3n+1 (PentA
+: pentylammonium) with IP orientation was obtained by adding tetrahydrothiophene-1-oxide (THTO) or DMSO into the precursor solution [
68]. The IP orientation control by adding DMSO or THTO was suspected by forming the complexes of the sulfoxide group of DMSO or THTO with Pb
2+ ions [
68]. The complexes held the Pb
2+ within the liquid phase and reduced the crystallization process where Pb
2+ was locked in the OP oriented QWs by bonding with MA
+. Since the single crystal grows along QWs direction, the IP oriented RP perovskite can be obtained by mechanical exfoliation method on target substrates. As a widely-applied technique in 2D materials researches, the mechanical exfoliation is also available for the formation of ultrathin BA
2PbI
4 and PEA
2PbI
4 sheets [
69,
70]. However, the 2D perovskite sheet formed by this method is low-productive and hard to control the layer number of the exfoliated RP perovskite, and so that directly forming 2D perovskite with in-plane orientation by solution method is worth to pursue. By solution method, atomically thin 2D BA
2PbBr
4 crystals (~1.6 nm thickness, 1–10 μm lateral size) can be formed by controlling the crystallization with a ternary solvent: dimethylformamide (DMF) chlorobenzene (CB) and acetonitrile (ACN) [
42]. In the ternary solvent, DMF facilitates the dissolution of the precursors. CB helps to adjust the solubility of precursors in DMF. The acetonitrile has a higher vapor pressure and it leave the solution quickly under heating, it is used to balance the dissolution and crystallization of the 2D hybrid perovskites [
42,
71]. Moreover, the -CN/-OH group in ACN is proposed to be adsorbed on specific polar crystal planes of perovskites during their self-assembly which further inhibited the
c-axis growth of 2D perovskite sheets [
71]. Furthermore, branched growth and large lateral sized 2D perovskite (up to ~40 μm) BA
2PbBr
4 cross-stars sheets were obtained by slowing down the drying of the solvent [
71]. Recently, a “induced peripheral crystallization” method was developed to grow multi-inch single-crystalline PEA
2PbI
4 perovskite membrane, which displayed ultralow defect density, long-term stability, and excellent flexibility [
72].
Besides one-step solution methods, 2D perovskite nanosheets can also be obtained by reacting lead halide nanosheets with methylammonium halide (MAX) vapor. Here we involve the formation of ultra-thin perovskite sheets without bulky ammonium cations (steric effects) into discussion, although there is not organic spacing inserted between adjacent 2D perovskite sheets. In Fig. 3(e), a two-step vapor-phase method for the formation of methyl ammonium halide nanoplatelets (Ma
n+1Pb
nX
3n+1) was illustrated. MA
n+1Pb
nX
3n nanoplates was synthesized by first van der Waals (VDW) epitaxy of PbX
2 nanoplates and then converting the PbI
2 nanoplates to MA
n+1Pb
nX
3n in MAX vapor [
73]. The resulting MA
n+1Pb
nI
3n+1 nanoplates were 70 nm thick with
. Furthermore, if the thickness of PbI
2 was controlled within few atomic layers, quasi-2D perovskite (MA
n+1Pb
nX
3n+1) with larger lateral size can be fabricated. For example, by hot casting the PbI
2 solution for 2D PbI
2 nanosheets, single-layered MA
2PbI
4 nanosheets were fabricated after reacting the 2D PbI
2 nanosheets with MAI vapor [
74]. Besides the two-step vapor-phase method, one-step vapor-phase method was further developed by co-evaporated the PbX
2 and MAX. For example, with PbCl
2 placed in the furnace heated at 360°–380° and MACl placed
cm away from PbCl
2 in the upper stream at its melting temperature, MACl and PbCl
2 were co-evaporated on the mica substrate and MA
n+1Pb
nCl
3n+1 nanoplate with a thickness of 8.7 nm and lateral dimension of over 20 μm was obtained [
75]. Different morphologies of the MA
n+1Pb
nCl
3n+1 nanoplates were obtained at different locations from the precursor vapor. The growth rate was determined by the adatoms of VDW-type diffusion and anisotropic surface free energy of the perovskite film. At the initial stage of film growth, surface energy dominates and a square shape was formed. Then the anisotropy in the adatom-capturing capability of different sites at the film edges resulted in a
fractal growth [
75]. The perfect in-plane orientation of perovskite nanoplates by vapor-phase method showed promising application for field effect transistors [
74]. Moreover, it is found that the PbI
2 crystal preferred to epitaxial grow on the other 2D materials such as graphene, hexagonal boron nitride (h-BN), and molybdenum disulfide (MoS
2), when these 2D materials located separately on SiO
2/Si substrate [
76]. After conversion of the PbI
2 to 2D perovskite via vapor method, 2D perovskite/inorganic 2D materials heterojunctions were formed, which showed promising potentials for the application combined with inorganic 2D materials [
76,
77]. In addition, combined the ternary solvent method processed single-layered RP perovskite nanoplates with the vapor-phase method, in-plane orientated RP perovskite BA
2Ma
n-1Pb
nBr
3n+1 nanoplates could be obtained by reacting in-plane orientated BA
2PbBr
4 nanoplate with MABr vapor [
78]. As shown in Fig. 3(f), the reaction of BA
2PbBr
4 nanoplate and MABr took place by intercalation of MABr between the layers and excluding BABr at 120°, in which the layer number
n to be tuneable by reaction time [
78].
4 Phase separation
For polycrystalline RP perovskite film, the result film was composed of RP perovskite with different layer number n, thus we defined
as the average n that determined by the composition in precursor solution. The phase separation between RP with different layer number in polycrystalline BA
2Ma
n-1Pb
nI
3n+1RP perovskite film prepared by hot-casting can be detected by steady state PL and transient absorption (TA) spectra as shown in Figs. 4(a)–(c) [
79]. When the perovskite film was illuminated from bottom side, exciton emission peaks of small-
n (
, peaks at
, 608, and 645 nm, respectively) and large-
n (
, at
nm) RP perovskites were observed. However, when the perovskite film was illuminated from top side, emission peak of large-
n (
nm) RP perovskite dominated. This indicated that the large-
n and small-
n RP perovskite phase preferred to locate at the surface and the bottom of the RP perovskite film, respectively. Moreover, the separation between large-
n and small-
n RP perovskite phases can be identified from TA results [
80]. Moreover, it was found that the absorption bleaching of large-
n RP perovskite phase raised along with the decay of absorption bleaching of small-
n RP perovskite [
79]. This indicated that there is a phase separation in resulted RP perovskite film with a scale level of carrier diffusion length or even energy transfer length, so that considerable electrons transferred from small-
n RP perovskite to large-
n RP perovskite. Remarkably, the phase separation was directly observed with high-resolution TEM and position-resolved absorption spectra recently [
81], in that study, both vertical and lateral phase segregation were observed. The formation of the phase separation is explained by the prior precipitation of quasi-3D perovskite, which resulted in the vertical phase segregation, and regional fast growth of 2D perovskite, which explained the lateral phase segregation. Based on this observation, energy transfer from 2D perovskite to quasi-3D perovskite was proposed, where after energy transfer, excitons were generated in quasi-3D perovskites, which would dissociate into free charges quickly due to the very small exciton binding energy in 3D-like perovskites. Since the exciton binding energy in 2D perovskites is much larger than thermal energy at room temperature, the energy transfer process may explain the effective exciton dissociation in 2D perovskite film.
The phase separation impact a lot on the working process of RP perovskite based solar cells and light emitting diodes [
58,
82,
83]. Both energy transfer and charge transfer between large-
n and small-
n RP perovskite phases have been investigated by many groups [
58,
79,
82-
85]. The charge transfer process was proposed in BA
2Ma
n-1Pb
nI
3n+1 film by applying electron or hole transfer materials [
58,
79]. When electron transfer materials (ETM) covered on the top of RP perovskite film, the electrons of large-
n RP perovskite further transferred electrons to ETM, resulting the disappearance of photobleaching (PB) raising of large-
n RP perovskite. When the hole transfer materials (HTM) was covered on the top, the photobleaching (PB) raising of large-
n RP perovskite remains, indicating the holes generated of the small-
n RP perovskite cannot diffuse to the top large-
n RP perovskite [
58,
79]. Moreover, contrast to the PB raising, time-resolved PL of large-
n RP perovskite decayed at the beginning, suggested the charge transfer process in BA
2Ma
n-1Pb
nI
3n+1 film [
79]. The charge transfer process between BA-based RP perovskite phase was also observed in ref. [
84], where vertical phase separation was achieved by spin-coating BAI on top of MAPbI
3 film. Moreover, the charge transfer process also applied to PEA
2Ma
n-1Pb
nI
3n+1 perovskite [
58,
85]. On the other hand, the energy transfer process is also proposed as an important process for the efficient charge collection in RP perovskite based solar cells. The energy transfer process with both electrons and holes transferred from small-
n RP perovskite to large-
n RP perovskite [as shown in Figs. 4(d) and (e)] was also utilized in the field of perovskite LEDs [
82,
83]. The cascade energy transfer of photon excitation for small-
n RP perovskites to large-
n RP perovskite was revealed by observation of the fast and slow exciton localization time of large-
n RP perovskite [
82]. The energy transfer process was also revealed for IP orientated PEA
2Ma
n-1Pb
nI
3n+1 film by TA and time-resolved PL spectra. The PL decay from small-
n exhibited a bi-exponential behavior with the fast decay attributed to a carrier funneling process [
83]. At last, to demonstrate precisely controlled phase separation, an example of lateral and vertical phase separation with
heterostructures was shown in Fig. 4(f) [
86]. For both vertical and lateral heterostructures, centimeter-size BA
2PbI
4 (BA
2PbBr
4 and PEA
2PbI
4) plates was placed at the downstream of the quartz tube and reacted with the MACl or MAI vapor blown from upstream. For the synthesis of the lateral heterostructures, the as-grown
plate was partially covered by using a shadow mask [
86].
5 Formation of 2D perovskite crystals on 3D perovskites surface
To avoid the trade-off between efficiency and stability when 2D perovskites were adopted as absorbers in solar cells, strategies of combining 2D perovskites with 3D perovskites while maintaining the structural integrity of the two phases were proposed [
87-
90].
The first strategy is ion exchange by spin coating A′X/isopropanol [
91] on the top of 3D perovskite where long cations such as BA
+ [
92], iso-butylammonium [
93], octylammonium [
92], cyclopropylammonium [
94], PEA
+ [
95-
97], 5-aminovaleric acid [
98],
[
99],
[
99],
[
99], tetra-methyl ammonium [
34], hexadecyl trimethyl ammonium [
34], tetra-ethyl ammonium [
34], tetra-butyl ammonium [
34] and tetra-hexyl ammonium [
34] were investigated. In addition, A′X could also be added into antisolvent to achieve graded 3D–2D halide perovskite interface [
100]. As a common method for fabricating 3D perovskite film, antisolvent was dropped on the film during spin-coating process to induce fast crystallization of 3D perovskite [
101,
102]. When antisolvent with PEAI was dropped on the film, some PEA
+ remained on the surface, resulting a gradually increased concentration of 2D perovskite from bottom to top. The 2D perovskite on the top has a higher conductive band level and disfavors the interface recombination [
103], resulting an improved open circuit voltage (Voc) and PCE of the solar cells [
100]. Besides the ion exchange, the A′X could also react with the remnant PbI
2 to achieve passivation effect [
104,
105]. The remnant PbI
2, which was formed by over annealing or by adding excess ratio of PbI
2 in precursor solution, was found to locate at the 3D perovskite grain boundaries and at the interfaces between 3D perovskite layer and ETM or HTM layer [
106-
110]. The capping PbI
2 formed type I band gap alignment with the inner 3D perovskite and suppressed the interface defect trapping [
107,
110]. However, the perovskite film with remnant PbI
2 showed poorer stability against illumination and humidity [
111]. Therefore, by spin-coating guanidinium bromide (GABr) or PEAI solution on top of PbI
2 capped 3D perovskite, the capping PbI
2 can be transferred to capping 2D perovskite, in which way, the passivation effect was retained while the stability against illumination and humidity was improved [
104,
105]. Similar to ion-exchange passivation method, n-butylamine [
112], aniline [
113], benzylamine [
113] and phenethylamine [
113] diluted in chlorobenzene could be spin-coated on the 3D perovskite surface to induce the reaction of 2BA + MAI + MAPbI
3 → BA
2PbI
4 + 2MA↑ for BA case.
When small ratio of 2D perovskite was added into 3D perovskite precursor solution, the 2D perovskite was found to spontaneously crystallize at the boundaries of the 3D perovskite grain or between grains [
62,
114]. For example, when PEA
2PbI
4 was added into FAPbI
3 perovskite precursor solution, the formed capping PEA
2PbI
4 protected the FAPbI
3 perovskite from moisture and suppress ion migration [
114]. When BA
+ cations were introduced into FA
0.83Cs
0.17Pb(I
yBr
1-y)
3 3D perovskite, 2D perovskite platelets between highly (h00) orientated 3D perovskite grains were formed [
62].
6 Impact of 2D perovskites on phase/device stability
Due to the hydrophobic nature of long cation ions, the stability against moisture was much improved for RP perovskite than 3D perovskite [
35,
36]. As shown in Figs. 5(c) and (d), after 2-month storage at 40% relative humidity environment, while MAPbI
3 decayed to PbI
2, no PbI
2 XRD peak and color change was observed for RR perovskite film, which indicated the better stability of RP perovskite than 3D perovskite. The improved device stability again moisture was demonstrated after applying hydrophobic cations
and
for solar cells [
115] and LEDs [
116], respectively. Moreover, the improved stability against humidity was also demonstrated for 2D passivated 3D perovskite film [
34]. Using in situ neutron and X-ray scattering techniques, rapid disproportionation of the initial 2D phase (
on top of MAPbI
3) into lower-n phases under humidity was observed, which further suppressed the escape of MAI, thus in turn improved the stability of the film against moisture [
117]. Apart from hydrophobicity of long-chain cation, since MAI can decompose into volatile MA gas and HI [
118], the better thermal stability of long-chain iodide cation than MA might also contribute to the improved overall stability.
In addition, the frequently observed ion migration problem is one of the important factors for current–voltage hysteresis and structural instability of perovskites [
119-
121]. Noticeably, suppressed ion migration along both OP and IP directions in RP perovskite have been demonstrated, which might be due to the blocking effect of long-chain cations or the lower density of vacancies [
122,
123]. The suppressed ion migration and the protecting effect of the long-chain cation in turn provides much improved stability of photovoltaic device against moisture and sun illumination [
48,
114].
Noting that FAPbI
3 and CsPbI
3 were more stable at hexagonal and orthorhombic phase, respectively [
124]. However, both two phases are unfavorable for solar cells application due to their large bandgap. Therefore, 2D perovskite were added into the 3D perovskite precursor solution to stabilize both FAPbI
3 and CsPbI
3 at the cubic phase [
114,
125]. The mechanism to stabilize cubic phase was explained by improved cubic phase purity at formation stage of perovskite film or by the reduced grain size for FAPbI
3 [
114] [as shown in Figs. 5(a), (b)] and CsPbI
3 [
125], respectively.
7 Controlled nanostructure
RP perovskite with nanostructures is favored in the development of perovskite light emitting devices [
126-
128], solar cells [
129,
130], photodetector [
131,
132] or lasing [
133,
134]. To control the shape of the nanocrystals (NCs), solvent-induced reprecipitation method and ligand-assisted reprecipitation method were usually adopted. For solvent-induced reprecipitation method, octadecene was used as solvent and 3D perovskite precursor was reacted in octadecene with crystallization controlled by octylamine (OM) and oleic acid (OA). When reaction was usually quenched by adding acetone or by the ice-water bath. By this method, MAPbBr
3 perovskite NCs were synthesized by adding PbBr
2, MABr, and octylammonium bromide to a stirring solution of oleic acid and 1-octadecene at 80 °C, followed by quenching the reaction with acetone [
135]. The resulting NCs contained both nanoparticles and nanoplatelets. The 2D perovskite nanoplatelets can be isolated by diluting the precipitation toluene and reprecipitated by adding acetone [
135]. To control the shape of NCs and the unit cell number, the reaction temperature was modified. When the reaction temperature decreased from 150 ° to 90 °, the shape of CsPbBr
3 NCs changed from nanocubes to nanoplatelets [
136]. The tunable shapes (nanocubes, nanowires, and nanoplatelets) of CH
3NH
3PbX
3 (X = Br or I) NCs was achieved by varying the ratio of OM to OA [
137]. In general, OM controls the size of formed NCs, whereas oleic acid suppresses aggregation effects. Low reaction temperatures and high ligand concentrations always favor anisotropic growth, mainly producing nanoplatelets [
138].
In ligand-assisted re-precipitation (LARP) method, the perovskite precursors with OM and OA in a good solvent (e.g., DMF or
γ-butyrolactone) was injected into a bad solvent (e.g., toluene or acetone) [
139,
140]. By tuning the amounts of OM and OA, the shapes of CsPbBr
3 NCs changed from lamellar-structured 0D quantum dots to face-to-face stacking 2D nanoplatelets and flat-lying 2D nanosheets as shown in Fig. 6(a) [
141]. Similarly, MAPbBr
3 nanoplatelets were synthesized by LARP method, with tunable atomic layer numbers obtained by adding different amount of octylammonium bromide [
142]. Besides ratio of OM and OA, the shape of nanostructure could also be modified by applying different types of organic acid and amine ligands [
143]. When OM and OA were adding in the bad solvent (i.e., toluene) instead of precursor solution, MAPbBr
3 nanoplatelets were also formed with atomic layer controlled by the amount of OM and OA [
44].
Apart from the shape control of nanostructure by direct synthesis, the perovskite nanoplatelets can also be obtained by diluting microcrystals solution in toluene with octylamine [
144,
145]. The thickness of the nanoplatelets can be controlled both by the dilution level and by the ligand concentration as shown in Fig. 6(b). The shape change from large NCs to nanoplatelet was explained by osmotic swelling of large NCs along with the quick passivation of organic ligands as shown in Fig. 6(c) [
145].
8 Prospects
In conclusion, atomic structure and crystal control of 2D perovskite were reviewed. Despite the excellent works done to control the formation of 2D perovskites for optoelectronic device, some open questions still remain and new strategies continue to emerge. First, exploring multifunctional long-chain cations for RP perovskite may pave another way for developing high efficient optoelectronic device. For example, long cations with high dipole moment might promote separation of photo-generated electron–hole pairs and suppress nonradiative recombination by reducing exciton binding energy, which resulted in an improved PCE of perovskite solar cells. Applying cations with better hydrophobic property might further improve the stability of RP perovskite against humidity. Second, a clear understanding of the mechanism about OP orientation would benefit developing RP perovskite solar cells with higher efficiency. Up to now, the PCEs of RP perovskite solar cells still lagged behind the 3D perovskite solar cells. One of the reasons lies in the misalignment of vertically packed quantum wells. Therefore, better crystallization along OP direction would favor charge transport and improve the performance of RP perovskite solar cells. Third, since single crystals with less traps would enable a high charge mobility, devices based on RP perovskite single crystals might show a better performance than the devices based on polycrystalline film. However, except single-crystalline PEA2PbI4 perovskite membrane was fabricated, reports on large-size RP single crystals is still sparse.
Higher Education Press and Springer-Verlag GmbH Germany, part of Springer Nature 2019