Sn-Based Perovskite Solar Cells towards High Stability and Performance

Recent years have witnessed rapid development in the field of tin-based perovskite solar cells (TPSCs) due to their environmental friendliness and tremendous potential in the photovoltaic field. Most of the high-performance PSCs are based on lead as the light-absorber material. However, the toxicity of lead and the commercialization raise concerns about potential health and environmental hazards. TPSCs can maintain all the optoelectronic properties of lead PSCs, as well as feature a favorable smaller bandgap. However, TPSCs tend to undergo rapid oxidation, crystallization, and charge recombination, which make it difficult to unlock the full potential of such perovskites. Here, we shed light on the most critical features and mechanisms affecting the growth, oxidation, crystallization, morphology, energy levels, stability, and performance of TPSCs. We also investigate the recent strategies, such as interfaces and bulk additives, built-in electric field, and alternative charge transport materials that are used to enhance the performance of the TPSCs. More importantly, we have summarized most of the recent best-performing lead-free and lead-mixed TPSCs. This review aims to help future research in TPSCs to produce highly stable and efficient solar cells.


Introduction
Nowadays, perovskites solar cells (PSCs) are considered as one of the most promising clean and renewable energy technologies. PSCs have achieved a high power conversion energy (PCE) up to about 26% [1,2], making it one of the most compelling research fields. Additionally, PSCs have enormous potential and versatile applications starting from solar plants for daily use electricity up to being utilized in space applications due to their appealing properties (light weight, low cost, flexibility, high PCE, and radiation tolerance) [3]. The ideal crystal structure of perovskites is cubic and based on the formula ABX 3 . The cation 'A' (organic or inorganic such as methylammonium (MA), formamidinium (FA), or Cs) occupies the vertices of the cubic lattice. The 'X' anions (oxygen or halogen (Cl − , Br − , or I − )) are located at the faces. The 'B' cation (Cu +2 , Sn +2 , or Pb +2 ) occupies the octahedral site. Perovskites containing halides were introduced for the first time in 1978 [4]. However, the first PSC with halides was reported in 2009 [5].
Currently, all high-performance PSCs contain Pb in the light absorber since it is proven to provide superior opto-electronic properties, such as high absorption coefficient [6] and excellent transport capability [7]. However, lead toxicity and the correlated need for large-scale commercialization of PSCs raise concerns about the hazards that Pb may cause to humans and the environment [8]. Pb can rapidly enter the human bodies through inhalation, causing dangerous effects on the organs of the body even a on molecular level [9]. Therefore, there is an urgent need to replace the toxic lead with elements that have less toxicity or none. Some of the suggested alternatives are Sn, Sb, Bi, or Ge [10][11][12][13][14][15]. Between these fundamental elements, Sn presents itself as one of the most promising options [16][17][18][19][20][21][22]. Sn is a group 14 element in the periodic table, and it has a similar ionic radius (115 pm) to Pb (119 pm), allowing for ASnX 3 perovskites to develop [19]. In comparison to the Pb-based

High Conductivity and Metallic Behavior
A very important insight about the electronic properties of Sn-based perovskites goes back to the work reported by Yamada et al. [39] in 1990. They investigated a set of different ASnI 3 perovskites (A = K, NH 4 , Rb, Cs, or MA). Both of the investigated Cs and MA -SnI 3 perovskites exhibited high conductivity at room temperature (Figure 1a), which was found to be in the range of 10 2 -10 3 S cm −1 [39]. However, in the case of CsSnI 3, this conductivity that is similar to metallic materials was only observed after heating, where the films were observed to undergo structural transformation at 425 K. This structural change was not observed in the case of MASnI 3 . The heating treatment increased the conductivity of CsSnI 3 by about 4 orders of magnitude and at the same time the materials' color was observed to change from greenish to black with a metallic luster. Additionally, the conductivity of the Cs-based sample was observed to increase with decreasing temperature in a similar trend, which is usually observed for metals [39].
In 2013, Stoumpos et al. [40] calculated the electronic properties of the of different Sn perovskites using the Seebeck coefficient and Hall effect measurements. An exceptionally high electron mobility of MASnI 3 was calculated, up to 2320 cm 2 V −1 ·s −1 . In 2016, Ma et al., reported that MASnI 3 may have opto-electronic properties that are better than those of CH 3 NH 3 PbI 3 [26]. They reported long carrier diffusion lengths of about 300 nm for electrons and 200 nm for holes (and can increase 10 times when the SnF 2 reducing agent was used), which were recorded using time-resolved fluorescence spectroscopy [26]. On the other hand, an interesting slow relaxation of the hot carriers (0.5 ps) was observed for the same samples [26]. Fang et al. [41] also found that the hot carriers in FASnPbI 3 have lifetimes of a few seconds, which can be utilized to design solar cells with PCEs that can exceed the Shockley-Queisser limit [27]. Additionally, with increased excitation source power, they observed a 75 meV blue shift of the optical bandgap at room temperature, which is due to the filling of band edge states [41]. However, the electronic properties are very dependent on the preparation method, which may directly affect the material quality and stoichiometry [40,42]. exceed the Shockley-Queisser limit [27]. Additionally, with increased excitation source power, they observed a 75 meV blue shift of the optical bandgap at room temperature, which is due to the filling of band edge states [41]. However, the electronic properties are very dependent on the preparation method, which may directly affect the material quality and stoichiometry [40,42].
(a) (b) Figure 1. (a) Electrical conductivity as a function of temperature of CsSnI3 and MASnI3. Reproduced with permission [39]. Copyright 1990, De Gruyter, and (b) schematic representation of BA incorporation in perovskite materials with n = 2, 3, and ∞, reproduced with permission [43]. Copyright 1995, Nature publishing group.

Metallic to Semiconducting by Incorporation of Different Organic Cations
In 1994, looking for new classes of superconductors, the insertion of organic chains of n-butylammonium (BA) into MASnI3 was performed and investigated by Mitzi et al. [43]. The incorporation of BA in the MASnI3 yielded a semiconducting behavior. With a general formula, BA2MA(n−1) Sn(n)I(3n+1). When n = ∞, the film only consists of MASnI3 and was observed to be also more of metallic. With n = 2, the formula becomes BAMASnI3 and the measured resistivity was observed to be 10 Ω cm at room temperature. With more BA incorporated (smaller n values), a more nonmetallic behavior was observed, (i.e., n = 3) along with a trend of resistivity decrease up to a temperature of 75 K followed by a slow upturn in resistivity with higher temperatures.
Similarly, an FA cation was also incorporated in the same way as BA [44]. Based on the formula [NH2C(I)=NH2]2(CH3NH3)m Snm I3m+2, with higher m values a metallic behavior was observed (Figure 1b). When n, m ⟹ ∞, the material is just MASnI3 [43,44]. Mitzi et al. [45] further investigated the observed metallic behavior of MASnI3. They also observed a low carrier density (p-type metallic behavior) with a hall carrier density of 2 × 10 19 cm −3 . The resistivity was also observed to decrease with decreased temperature, which is in line with the metallic behavior, with a resistivity at room temperature of about 7 mΩ cm [45]. Moreover, Mitzi et al. [45] also reported that the prepared MASnI3 material has free carrier IR (infra-red) reflectivity with a plasma edge, which confirms the metallic nature of the prepared materials.
After that, in 1997, the same previous group reported that the resistivity of MASnI3 at room temperature in the pure FASnI3 is about three orders of magnitude higher than previously reported [46]. The resistivity at room temperature of FASnI3 was found to be ~ Figure 1. (a) Electrical conductivity as a function of temperature of CsSnI 3 and MASnI 3 . Reproduced with permission [39]. Copyright 1990, De Gruyter, and (b) schematic representation of BA incorporation in perovskite materials with n = 2, 3, and ∞, reproduced with permission [43]. Copyright 1995, Nature publishing group.

Metallic to Semiconducting by Incorporation of Different Organic Cations
In 1994, looking for new classes of superconductors, the insertion of organic chains of n-butylammonium (BA) into MASnI 3 was performed and investigated by Mitzi et al. [43]. The incorporation of BA in the MASnI 3 yielded a semiconducting behavior. With a general formula, BA 2 MA (n−1) Sn (n) I (3n+1) . When n = ∞, the film only consists of MASnI 3 and was observed to be also more of metallic. With n = 2, the formula becomes BAMASnI 3 and the measured resistivity was observed to be 10 Ω cm at room temperature. With more BA incorporated (smaller n values), a more nonmetallic behavior was observed, (i.e., n = 3) along with a trend of resistivity decrease up to a temperature of 75 K followed by a slow upturn in resistivity with higher temperatures.
Similarly, an FA cation was also incorporated in the same way as BA [44]. Based on the formula [NH 2 C(I)=NH 2 ] 2 (CH 3 NH 3 ) m Sn m I 3m+2 , with higher m values a metallic behavior was observed (Figure 1b). When n, m ⇒ ∞, the material is just MASnI 3 [43,44]. Mitzi et al. [45] further investigated the observed metallic behavior of MASnI 3 . They also observed a low carrier density (p-type metallic behavior) with a hall carrier density of 2 × 10 19 cm −3 . The resistivity was also observed to decrease with decreased temperature, which is in line with the metallic behavior, with a resistivity at room temperature of about 7 mΩ cm [45]. Moreover, Mitzi et al. [45] also reported that the prepared MASnI 3 material has free carrier IR (infra-red) reflectivity with a plasma edge, which confirms the metallic nature of the prepared materials.
After that, in 1997, the same previous group reported that the resistivity of MASnI 3 at room temperature in the pure FASnI 3 is about three orders of magnitude higher than previously reported [46]. The resistivity at room temperature of FASnI 3 was found to bẽ 7 Ω cm compared to 3 Ω cm in the case of MASnI 3 . The use of FA resulted in lattice expansion, which was speculated to have an effect on the formation of defects, which would readily produce a shift in the energy levels and affect transport properties [46]. Additionally, FA has an extra NH 2 group compared to MA, which provides an extra site to form an additional hydrogen bond that can contribute to better ordering. In general, the FAMA system was also observed to add additional freedom to tailor the electronic properties of such materials by changing the ratio from MA to FA [46].

Importance of Preparation Method
Several comparative studies of CsSnI 3 's electrical behavior and a detailed investigation of MA and FA compared to Cs-based -SnI 3 perovskites were reported [24,42,47]. However, the preparation method and post-treatment can majorly alter the film electronic nature up to even an n-type semiconductor [40]. Two of three methods used to prepare Cs, FA, and MA-SnI 3 perovskites (single crystals from solution, and compressed pellets from sealed tubes dry reaction) exhibited high resistivity trends that are consistent with semiconductor behavior [40]. However, similar samples prepared using the third method (dry in an open tube) were found to behave as a p-type metal. The single crystals from the solution method of FA and MA-SnI 3 were found to be n-type semiconductors with a low level of electron carriers in the temperature range from 300 to 400 K. However, pressed pellets from the dry method with no annealing were found to be p-type semiconductors. When high-quality ingots of CsSnI 3 were prepared, superior performance with lifetimes approaching 6.6 ns and diffusion length approaching 1µm compared to only 54 ps and 16 nm for the lower quality polycrystalline ones were observed [25]. For these ingots, no reducing agents such as SnF 2 were used. Based on the extracted lifetimes and diffusion lengths of these high-quality CsSnI 3 crystals, a PCE of 23% was estimated [25]. It was shown that the significant factor for electrical properties of the Sn perovskites is the easy oxidization of Sn +2 and the formation of the more stable Sn +4 . Consequently, p-type metal character and low resistivity are increased, contributing to the self-doping mechanism. Sn has two active electrons on the 5-S orbital, which causes the easy oxidization from Sn +2 to Sn +4 . It tends to lose these two electrons because the fully occupied 4d orbital electrons are less effective as electromagnetic shields [48].

Defect Physics of Sn Perovskites
Tin-based perovskites have a direct bandgap, meaning that the momentum of the VB maximum and the CB minimum is the same [10]. This results in a high absorption coefficient. However, it is reported to be an order of magnitude less than Pb-based perovskites [10,26,49]. Even though Sn perovskites have a direct bandgap, their energy bands are higher than those of Pb-based perovskites ( Figure 2a). As a result, the Sn-I bond can be broken easily, allowing for I − and Sn +2 to react with H 2 O and O 2 , respectively; therefore, the Sn perovskites may easily become poor in crystal quality and photovoltaic performance and the properties may be easily altered.
In Sn +2 states, the 5P orbital's high energy causes Lewis acidity [50], which leads to the unwanted and uncontrolled rapid crystallization of perovskites. This leads to a substantial amount of physical defects in crystal lattice, which may be the reason for the often observed discrepancy of Sn perovskite properties, such as the energy levels measured and reported values of Sn perovskite films (Figure 2b). LaMer's classic crystal growth theory states that small crystal grains could form due to fast crystallization [51]. These grains significantly affect the optoelectronic properties of Sn-based perovskites since it helps to ease the losses of Sn ions [52]. On the other hand, the oxidization from Sn +2 to Sn +4 leads to the formation of Sn vacancies (V Sn ) and act as high p-doping. Finally, these defects result in hole carriers with high concentrations, which operate as recombination centers for charge carriers. Consequently, tin-based perovskite systems perform sub-optimally.  [53], (ii) [54], (iii) [55], (iv) [56], and (v) [57].

Stability of Sn Perovskites
The low environmental stability of Sn perovskites has been long recognized as a sig nificant issue, and it has been blamed for their inability to achieve performance compara ble to Pb-based PSCs. Perovskite layers tend to oxidize rapidly with oxygen in ambien conditions [58,59]. As a result, short carrier lifetimes and a high nonradiative carrier re combination rate are often observed and detrimental to their photovoltaic performanc There are several factors leading to the well-known poor stability of the Sn-based perov skites, including extrinsic and intrinsic factors. We will discuss specifically the followin factors: oxygen, moisture, illumination, and ion migration.

Moisture Effect
Moisture is considered to be the most prominent factor that causes the degradatio of the Sn-based perovskites, leading to the oxidation of Sn [60]. In the presence of mois ture, the perovskites are expected to degrade to form metal iodides (i.e., SnI2). Simultane ously, in the case of MA cations (CH3NH3I), they form HI acid under H2O environment Even though minimal moisture is necessary to decompose the organic part, an excess needed to break down the HI and CH3NH2 derivatives for the degradation to progress.
In addition to MA cations, FA cations also have a hygroscopic nature [61,62]. FA an MA cations also react with H2O in distinct binding mechanisms [63]. FA and H2O form stronger hydrogen bonds (than MA + ), increasing the size of the perovskite lattice and re ducing the stability of the crystal structure. However, this may reduce the H2O interactio with SnI2. Furthermore, the changes that happen to the electronic properties of FASnI3 an MASnI3 in the presence of moisture air include the fact that the resistivity decreases at th beginning of air exposure for both films and then increases over time [63]. After 40 min o air exposure with 60% humidity, the MA perovskite displays a drop in order of magn tude. On the other hand, the FA perovskite displays a 10% drop under similar condition (Figure 3a,b).

Stability of Sn Perovskites
The low environmental stability of Sn perovskites has been long recognized as a significant issue, and it has been blamed for their inability to achieve performance comparable to Pb-based PSCs. Perovskite layers tend to oxidize rapidly with oxygen in ambient conditions [58,59]. As a result, short carrier lifetimes and a high nonradiative carrier recombination rate are often observed and detrimental to their photovoltaic performance. There are several factors leading to the well-known poor stability of the Sn-based perovskites, including extrinsic and intrinsic factors. We will discuss specifically the following factors: oxygen, moisture, illumination, and ion migration.

Moisture Effect
Moisture is considered to be the most prominent factor that causes the degradation of the Sn-based perovskites, leading to the oxidation of Sn [60]. In the presence of moisture, the perovskites are expected to degrade to form metal iodides (i.e., SnI 2 ). Simultaneously, in the case of MA cations (CH 3 NH 3 I), they form HI acid under H 2 O environments. Even though minimal moisture is necessary to decompose the organic part, an excess is needed to break down the HI and CH 3 NH 2 derivatives for the degradation to progress.
In addition to MA cations, FA cations also have a hygroscopic nature [61,62]. FA and MA cations also react with H 2 O in distinct binding mechanisms [63]. FA and H 2 O form stronger hydrogen bonds (than MA + ), increasing the size of the perovskite lattice and reducing the stability of the crystal structure. However, this may reduce the H 2 O interaction with SnI 2 . Furthermore, the changes that happen to the electronic properties of FASnI 3 and MASnI 3 in the presence of moisture air include the fact that the resistivity decreases at the beginning of air exposure for both films and then increases over time [63]. After 40 min of air exposure with 60% humidity, the MA perovskite displays a drop in order of magnitude. On the other hand, the FA perovskite displays a 10% drop under similar conditions (Figure 3a,b).
When TPSCs are tested in nitrogen-filled gloveboxes with H 2 O~1 ppm, the performance of FASnI 3 devices is more stable and they display good reproducibility ( Figure 3c). Therefore, it may be possible to produce better TPSCs by carefully selecting the organic cation, which reduces moisture ingress [64].

Oxygen Effect
Oxygen damages the charge neutrality of the perovskite structure and causes it to disintegrate into oxides or hydroxides of Sn and MAI or FAI, and as a result the electron-hole recombination increases [10]. The organic cations (i.e., FA and MA) have a significant im-pact on the O 2 -induced degradation of Sn-based perovskites, as well as affecting the optical and electronic properties of the materials such as charge mobility, band alignment, and diffusion length [63]. Lanzetta et al. [65] defined the mechanisms underlying the degradation of different dimensional tin-perovskite films based on phenethylamine (PEA) 0.2 (FA) 0.8 SnI 3 . As a result of moisture and oxygen, SnI 4 and SnO 2 were formed and resulted in the formation of molecular iodine, which is detrimental to the perovskites' performance. Iodine is a hyper aggressive compound that can further oxidize the perovskite, resulting in a cyclic degradation ( Figure 4a) [65,66].

Oxygen Effect
Oxygen damages the charge neutrality of the perovskite structure and causes it to disintegrate into oxides or hydroxides of Sn and MAI or FAI, and as a result the electronhole recombination increases [10]. The organic cations (i.e., FA and MA) have a significant impact on the O2-induced degradation of Sn-based perovskites, as well as affecting the optical and electronic properties of the materials such as charge mobility, band alignment, and diffusion length [63]. Lanzetta et al. [65] defined the mechanisms underlying the degradation of different dimensional tin-perovskite films based on phenethylamine (PEA)0.2(FA)0.8SnI3. As a result of moisture and oxygen, SnI4 and SnO2 were formed and resulted in the formation of molecular iodine, which is detrimental to the perovskites' performance. Iodine is a hyper aggressive compound that can further oxidize the perovskite, resulting in a cyclic degradation ( Figure 4a) [65,66]. presence of humid air in which reaction 1 is the oxidation of ASnI3 By O2, reaction 2 is the solid-state formation of A2SnI6, reaction 3 is the hydrolysis of SnI4 by H2O, reaction 4 is the oxidation of HI By O2, and reaction 5 is the oxidation of perovskite by I2. Reproduced under terms of CC-BY [65]. Copyright 2021, Nature publishing group. (b) Proposed ultraviolet light degradation process when photo-generated holes are applied externally with oxygen, after which they react with oxygen radicals adsorbed on the surface of oxygen vacancies, as seen in (i,ii). As a result of the oxygen, deep surface traps remain unfilled, and each trap has a free electron. (iii) As a result of the sensitizer's photoexcitation, electrons flow into the conduction band, where they are deeply trapped, or directly into the deep surface traps, and as a result of that the electrons are strongly trapped and they easily recombine with holes in the spiro-

Oxygen Effect
Oxygen damages the charge neutrality of the perovskite structure and causes it to disintegrate into oxides or hydroxides of Sn and MAI or FAI, and as a result the electronhole recombination increases [10]. The organic cations (i.e., FA and MA) have a significant impact on the O2-induced degradation of Sn-based perovskites, as well as affecting the optical and electronic properties of the materials such as charge mobility, band alignment, and diffusion length [63]. Lanzetta et al. [65] defined the mechanisms underlying the degradation of different dimensional tin-perovskite films based on phenethylamine (PEA)0.2(FA)0.8SnI3. As a result of moisture and oxygen, SnI4 and SnO2 were formed and resulted in the formation of molecular iodine, which is detrimental to the perovskites' performance. Iodine is a hyper aggressive compound that can further oxidize the perovskite, resulting in a cyclic degradation (Figure 4a) [65,66]. presence of humid air in which reaction 1 is the oxidation of ASnI3 By O2, reaction 2 is the solid-state formation of A2SnI6, reaction 3 is the hydrolysis of SnI4 by H2O, reaction 4 is the oxidation of HI By O2, and reaction 5 is the oxidation of perovskite by I2. Reproduced under terms of CC-BY [65]. Copyright 2021, Nature publishing group. (b) Proposed ultraviolet light degradation process when photo-generated holes are applied externally with oxygen, after which they react with oxygen radicals adsorbed on the surface of oxygen vacancies, as seen in (i,ii). As a result of the oxygen, deep surface traps remain unfilled, and each trap has a free electron. (iii) As a result of the sensitizer's photoexcitation, electrons flow into the conduction band, where they are deeply trapped, or directly into the deep surface traps, and as a result of that the electrons are strongly trapped and they easily recombine with holes in the spiro-OMeTAD (2,2',7,7'-Tetrakis[N,N-di(4-methoxyphenyl)amino]-9,9'-spirobifluorene) hole transporter layer (iv). Reproduced with permission [67]. Copyright 2013, Nature publishing group. Reproduced under terms of CC-BY [65]. Copyright 2021, Nature publishing group. (b) Proposed ultraviolet light degradation process when photo-generated holes are applied externally with oxygen, after which they react with oxygen radicals adsorbed on the surface of oxygen vacancies, as seen in (i,ii). As a result of the oxygen, deep surface traps remain unfilled, and each trap has a free electron. (iii) As a result of the sensitizer's photoexcitation, electrons flow into the conduction band, where they are deeply trapped, or directly into the deep surface traps, and as a result of that the electrons are strongly trapped and they easily recombine with holes in the spiro-OMeTAD (2,2',7,7'-Tetrakis[N,N-di(4-methoxyphenyl)amino]-9,9'-spirobifluorene) hole transporter layer (iv). Reproduced with permission [67]. Copyright 2013, Nature publishing group.

Illumination
In general, TiO 2 is one of the most common electron transport materials (ETMs) for n-i-p PSCs. Specifically, under UV-illumination, TiO 2 molecules are a typical photo-catalyst that can accelerate the degradation of perovskite materials [67]. TiO 2 has many several oxygen vacancies as it is an n-type material. In the presence of oxygen, it adsorbs these vacancy cites due to the reaction with the deep electrons that lie in the vacancies. Through UV-illumination, an electron-hole pair was formed in TiO 2 . As a result, the electron in the vacancy, which lies before the CB by~1 eV, will interact with holes in the VB. This operation leads to free electrons in the CB and empty oxygen vacancies with a positive charge, which will act as traps for electrons generated from perovskite material. Additionally, in the common n-i-p structure, spiro-OMeTAD hole transport material (HTM) is used as a heavily p-doped material that will allow for recombination with these free electrons in the CB (Figure 4b(ii-iv)). Lee et al. [68] mitigated this problem in PSCs replacing mesoporous TiO 2 with a thin layer of insulating Al 2 O 3 . However, with this UV-related problem and with the aforementioned TiO 2 -related problems, the p-i-n structure is more commonly used for TPSCs.
One of the popular methods to improve the illumination stability of Sn perovskites is with 'X' site (ABX 3 perovskites) doping, which is unfortunately more susceptible to illumination degradation due to phase separation under illumination [69]. Additionally, the 'A' organic cations, especially MA + (best for highest PCEs), are very prone to decomposition under illumination [70,71]. Therefore, 'A' site manipulation or additives are the most popular methods to enhance the Sn perovskites' stability under illumination [72].

Ion Migration
Ion migration is a well-known and an undesirable phenomenon in PSCs. This is also related to the hysteresis in current density-voltage (J-V) characteristics curve [73]. Due to the dissociation of the charged ions, the diffusion of the ions results in unbalanced charge transport [74]. It also has an impact on the cell's long-term stability and performance, as well as its photoelectronic properties. Defects/ions such as iodide vacancies can migrate across the contact during PSC operation, producing interfacial deterioration, compromising device function, and even triggering device failure. The activation barrier of hybrid perovskites is low. Thus, the ions, such as iodide, are induced to migrate through perovskite devices under applied bias or irradiation [73]. The ions of the iodide (I − ) easily move to defects in perovskites under an external electric field [75]. Additionally, excess iodide may accumulate at the interface between the perovskite, charge transport materials, and electrodes. As a result, the solar cells perform poorly and degrade rapidly [76].
One common method to restrict the ion migration is using additives. For example, the addition of polyvinyl alcohol (PVA) polymer to the FASnI 3 solution was shown to improve hydrogen-bonding interactions. Therefore, the PVA-inhibited transport of iodide ions prevented the formation of iodide vacancies, and lowered ionic conductivity, preventing ion migration and preserving the long-term stability of tin-based PSCs [77]. More examples of the recent development of enhanced stability are presented in a later section.

Basic Structure and Charge Transport Materials for Tin-Based Perovskite Solar Cells
A typical PSC consists of five main individual layers deposited consecutively on a glass or flexible substrate. Based on the order of the deposited layers on the transparent conductive electrode (TCE), it can be a normal or an inverted structure. The normal structure is TCE/ETM/perovskite absorber (PVSK)/HTM/top electrode (n-i-p stack). The inverted structure is TCE/HTM/PVSK/ETM/top electrode (p-i-n stack).
One of the first TPSCs with the n-i-p structure was reported by Hao et al. [11] with a standard architecture of fluorinated tin oxide (FTO)/compact TiO 2 /MASnI 3 /spiro-OMeTAD/Au and achieved a PCE of 5.7%. The first TPSC with a p-i-n structure was reported with indium tin oxide (ITO)/poly(3,4-ethylenedioxythiophene):polystyrene sulfonate (PEDOT:PSS)/FASnI 3 /fullerene (C 60 )/2,9-dimethyl-4,7-diphenyl-1,10-phenanthroline (BCP)/Ag with PCE of 6.22% ( Figure 5) [53]. These structures had low efficiencies with many problems and challenges, such as poor and uncontrolled quality of Sn perovskites as well as poor interfacial contact resulting in instability problems, mismatch of energy levels, insufficient charge extraction, and hysteresis effect. However, inverted (p-i-n) TPCSs exhibited a slightly better performance, stability, lower cost, as well as ease of fabrication, which made them more reliable to fabricate. sulfonate (PEDOT:PSS)/FASnI3/fullerene (C60)/2,9-dimethyl-4,7-diphenyl-1,10-phenanthroline (BCP)/Ag with PCE of 6.22% ( Figure 5) [53]. These structures had low efficiencies with many problems and challenges, such as poor and uncontrolled quality of Sn perovskites as well as poor interfacial contact resulting in instability problems, mismatch of energy levels, insufficient charge extraction, and hysteresis effect. However, inverted (p-i-n) TPCSs exhibited a slightly better performance, stability, lower cost, as well as ease of fabrication, which made them more reliable to fabricate.

Electron Transport Layer (ETL)
The ETL is necessary to transport photo-generated electrons from the perovskite layer towards the anode. One of the most common ETLs is the compact blocking layer of TiO2, which is usually deposited using spray pyrolysis and it has a good chemical stability, electrical properties, and is non-toxic [78]. However, TiO2 implies high-temperature processing, low durability due to brittle nature, and is a photocatalyst that tends to adsorb oxygen, which results in the degradation of perovskites upon UV intake. Due to this problem, researchers attempt to find alternatives for TiO2. One of the possible alternatives is ZnO, which exhibits a suitable bandgap, similar to TiO2 (3.2 eV). It also has a high electron mobility equal to ~200 cm 2 V −1 s −1 [79]. However, ZnO has a poor stability and is hygroscopic, which makes it less suitable due to its degradation and fast reaction with air [80]. Another rising alternative is SnO2, which has a high electron mobility (250 cm 2 V −1 s −1 , which is higher than that for TiO2 and ZnO) [79]. Its bandgap is wider (3.8 eV), which is more suitable for matching with the perovskite materials' bandgap [80,81]. In addition, it is less hygroscopic, which results in lower photocatalytic activity and therefore stable performance [82][83][84]. An example from 2018, SnO2 with a thin layer of C60 as ETM in n-i-p TPSCs with the architecture of ITO/SnO2/C60/FASnI3/spiro-OMeTAD/Ag was able to achieve 4.34% without noticeable problems [85].
The most common ETM material used in inverted devices is C60 and [6,6]-phenyl-C61-butyric acid methyl ester (PCBM). Fullerenes show a good band alignment with perovskite materials, leading to lower charge recombination since it transfers smoothly to the perovskite [86,87]. It also has a good energy alignment with the CB of the FASnI3 perovskites. Furthermore, using C60 as ETM exhibits low hysterias in the J-V curve, leading to a high PCE [88].

Electron Transport Layer (ETL)
The ETL is necessary to transport photo-generated electrons from the perovskite layer towards the anode. One of the most common ETLs is the compact blocking layer of TiO 2 , which is usually deposited using spray pyrolysis and it has a good chemical stability, electrical properties, and is non-toxic [78]. However, TiO 2 implies high-temperature processing, low durability due to brittle nature, and is a photocatalyst that tends to adsorb oxygen, which results in the degradation of perovskites upon UV intake. Due to this problem, researchers attempt to find alternatives for TiO 2 . One of the possible alternatives is ZnO, which exhibits a suitable bandgap, similar to TiO 2 (3.2 eV). It also has a high electron mobility equal to~200 cm 2 V −1 s −1 [79]. However, ZnO has a poor stability and is hygroscopic, which makes it less suitable due to its degradation and fast reaction with air [80]. Another rising alternative is SnO 2 , which has a high electron mobility (250 cm 2 V −1 s −1 , which is higher than that for TiO 2 and ZnO) [79]. Its bandgap is wider (3.8 eV), which is more suitable for matching with the perovskite materials' bandgap [80,81]. In addition, it is less hygroscopic, which results in lower photocatalytic activity and therefore stable performance [82][83][84]. An example from 2018, SnO 2 with a thin layer of C 60 as ETM in n-i-p TPSCs with the architecture of ITO/SnO 2 /C 60 /FASnI 3 /spiro-OMeTAD/Ag was able to achieve 4.34% without noticeable problems [85].
The most common ETM material used in inverted devices is C 60 and [6,6]-phenyl-C61-butyric acid methyl ester (PCBM). Fullerenes show a good band alignment with perovskite materials, leading to lower charge recombination since it transfers smoothly to the perovskite [86,87]. It also has a good energy alignment with the CB of the FASnI 3 perovskites. Furthermore, using C 60 as ETM exhibits low hysterias in the J-V curve, leading to a high PCE [88].

Hole Transport Layer (HTL)
The most common hole transport layers (HTLs) that are used in high-performance PSCs are spiro-OMeTAD [89], poly[bis(4-phenyl)(2,4,6-trimethylphenyl)amine] (PTAA) [90,91], PEDOT:PSS [90,92,93], and some metal oxides as well as small molecules [90,94]. HTM plays a significant role in the hole transport and stability of the perovskite layer [95]; however, pure spiro-OMeTAD exhibits low conductivity [96]. Different small molecules are often added as p-dopants, such as lithium salt Lithium bis(trifluoromethanesulfonyl)imide (Li-TFSI) and 4-tert-Butylpyridine (tBP) [97]. Adding these molecules improves the hole mobility, and as a result, high open-circuit voltage (V OC ) and PCE were achieved [98,99]. However, due to high moisture sensitivity of Li-TFSI and tBP, the combination results in degradation; additionally, tBP can dissolve perovskites [89]. In order to solve these issues, researchers introduced a set of alternatives such as PEDOT:PSS [100], which is more common in inverted devices. However, PEDOT:PSS is sensitive to moisture, leading to stability problems. One of the alternatives investigated by Cao et al. [101] was copper thiocyanate (CuSCN), with which a PCE of 7.34% was achieved. Nickel oxide (NiO) is also a common HTM and has the advantage of more stability than another alternatives. On the other hand, it has a wide bandgap and good energy alignment with the Sn perovskite [102].

Thin Films of Sn Perovskites towards High Efficiency and Stability
Compared to Pb-based PSCs, TPSCs exhibit a much lower PCE, mainly due to the poor film quality, correlated degradation, and detrimental effects. Perovskite films are often fabricated from solutions due to ease of fabrication. In order to create a high-performance tinbased PSC, it is imperative to form dense, compact, well-crystalline perovskite films [103]. Many ways have been proposed to resolve the instabilities of tin-based perovskites. The first step to enhance the stability of the device is to gain a deeper understanding of the degradation mechanisms. Earlier, we briefly pointed out the effects of moisture, oxygen, illumination, ion migration, and chemical reactions which are the most common causes of degradation in perovskite halides. In this section, we go over the most effective ways for increasing the performance and stability of Sn-based perovskite halides that have been reported.

Tin Perovskites with Additives/Reducing Agents
A defect is often induced by the fast oxidation of Sn +2 due to its fast kinetics of nucleation and growth in perovskites; therefore, additives that often reduce the fast oxidation and improve the film morphology (compactness) are required. Sn halides (SnF 2 , SnCl 2 , SnBr 2 , and SnI 2 ) and several organic molecules have been shown to prevent oxidation and enhance the performance of TPSCs. Furthermore, Sn halide additives are able to compensate for Sn vacancies in the films, improving the film morphology, reducing the likelihood of vacancy formation, and reducing the background hole density [104].

SnF 2 Additive
One of the first reports of reducing agents was implemented in 2012 by Chung et al. [24] using CsSnI 3 Sn perovskites as an HTM by doping with SnF 2 in dye-sensitized solar cells, which helped in producing a V OC of 0.42 V and an overall PCE of 0.9%. Following this, in 2014 Kumar et al. [105] found that incorporating SnF 2 into CsSnI 3 reduces the formation energy of Sn vacancies, leading to less conductivity in CsSnI 3 , and as a result, the TPSCs gained a high current density (J SC ) of 22 mA cm −2 . The impacts of SnF 2 doping in FASnI 3 with 20% mole were confirmed with X-ray diffraction (XRD) data that indicated a reduced amount of Sn +4 [42]. This helped the current density to increase by 10 mA cm −2 . In 2018, Xiao et al. [106] were able to achieve homogeneous crystal growth and uniform film coverage. They demonstrated that SnF 2 can reduce Sn vacancy (V Sn ) concentrations by boosting their formation energy. Following that, Hartmann et al. [107] studied the electronic structure of CsSnBr 3 and observed that Sn oxidation was inhibited by the addition of 20% mole SnF 2 . In 2016, Ma et al. [26] showed that SnF 2 had the effect of a distinguishable increase in carriers' lifetime from 0.7 ns to 6 ns. Additionally, hole diffusion length was estimated to increase substantially, as a result of the addition of SnF 2 , whereas the electron diffusion length remained unchanged. SnF 2 is commonly used in most tin-based photovoltaic systems for easy optimization of Sn perovskites.

SnCl 2 Additive
An additional reducing agent commonly used in Sn perovskites is SnCl 2 [108]. It was used to increase the stability of the Sn-based devices in an HTM free structure. Using X-ray photoemission spectroscopy (XPS) analysis on CsSnI 3 perovskite samples treated with the addition of 10 mol% of SnCl 2 , they found that SnCl 2 was present at the perovskites' surfaces, and that the SnCl 2 layer could act as a dryer to improve the stability of CsSnI 3 . Interestingly, after 5 months of storage under a nitrogen environment, the PCE was observed to increase, along with the V OC and FF. This improvement in the performance over time can be explained by the SnCl 2 doping on the electron-transport layer of the used ETM (i.e., PCBM). In addition, they evaluated different tin halide additives (SnCl 2 , SnBr 2 , SnI 2, and SnF 2 ) to see how they could affect HTM-free TPSCs (ITO/CsSnI 3 /PC 61 BM/BCP/Al). Among the tested devices, with the SnCl 2 additive, a PCE of 3.56% was the best, and SnCl 2 resulted in the highest film stability. Performance improvements may be attributable to the enhancement of PCBM ETM crystallization under light illumination.

Hydrazine Additive
Hydrazine has long been used in chemical synthesis to prevent oxidation (reducing agent). Additionally, hydrazine's highly volatile nature makes it an easy agent to be introduced as a reducing atmosphere. Song et al. [60] introduced hydrazine vapor atmosphere prior to the spin-coating process of the perovskite precursor. The films were formed in hydrazine atmosphere resulting in reduced defects, oxidation, and therefore better performance. Similarly, Kayesh et al. [109] were able to minimize the concentration of Sn +4 by 20% and significantly suppress carrier recombination during the fabrication of FASnI 3 perovskite films, by incorporating hydrazinium chloride (N 2 H 5 Cl) into a single precursor solvent system. A high PCE with significantly enhanced V OC and pinhole-free FASnI 3 perovskite films were achieved. Li et al. [110] reported a solution-deposition method for the fabrication of MASnI 3 that included hydrazinium iodide (N 2 H 5 I) with SnI 2 precursor. A mesoporous TPSC with a PCE of 7.13% was achieved.

Acidic Additives
Hypophosphorous acid (HPA). In the synthesis of tin-based perovskites, HPA has long been used as a common reducing agent. In most circumstances, HPA is utilized as an assisting reducing agent in antioxidation when powerful agents such as hydroiodic acid (HI) or SnF 2 are present, eventually stabilizing the process. Researchers used HPA as a coordinating agent in the CsSnIBr 2 production process, which allowed them to speed nucleation while restricting Sn +2 oxidation. Charge carrier density and Sn vacancy levels were lowered as a result of the HPA integration [111].
2,2,2-trifluoroethylamine hydrochloride (TFEACl). In combination with SnF 2 , 5 mol% of TFEACl was found to improve and enhance FASnI 3 solar cells [100]. The work function of perovskite films may be adjusted by adding Cl. Therefore, the perovskite films are better aligned with the charge transport layers. In addition, light soaking stability was found to be improved, which all resulted in improved device performance and charge collection.
Gallic acid (GA).Wang et al. [112] used the antioxidant GA as an additive together with excess SnCl 2 . GA was found capable to form a complex with SnCl 2 that is evenly distributed on perovskite grains. The characteristics of the GA can be derived from the aromatic ring's hydroxyl groups (-OH), which can donate electrons and absorb oxygen by hydrogen atoms. The SnCl 2 layers present atop perovskite grains were expected to result in a wider bandgap compared to the bulk. After 1000 h of air exposure, unencapsulated GA-based devices preserved more than 80% of their initial PCE, which is one of the highest reports. Moreover, the solar cells with GA exhibited a high PCE of 9.03%.
Ascorbic acid (AA). It is a simple but effective additive that inhibits the oxidation of Sn +2 also regulates its film crystallization and creation, and can be utilized to build polymer-stabilized Pb/Sn binary PSCs [113], enhancing the optoelectronic quality of dual, perovskite films greatly. The resulting MA 0.5 FA 0.5 Pb 0.5 Sn 0.5 I 3 film's photogenerated carrier lifetime (183 ns) demonstrates this. As a result, MA 0.5 FA 0.5 Pb 0.5 Sn 0.5 I 3 treated with AA achieved a high PCE of 14.01% and a higher stability than the control device employing the SnF 2 additive, outperforming it. This research proposes a novel method for improving the performance and obtaining more stable Pb/Sn-PSCs.

Surface Modifiers
There are many surface modifiers for TPSCs that are applied using different methods and can be applied before or after the perovskite layer deposition. Controlling the surface terminations can majorly affect the stability and morphology [59,114,115]. [116]. The C=O group in such modifier was observed to interact with Sn +2 and promote the formation of largely oriented perovskites. Additionally, it was found that FBH results in the reduction in Sn +4 by the hydrazide group. According to the performed density functional theory calculation, the oxygen absorption barrier is increased after the FBH modification, resulting in a delay in the oxidation process. As a result of such, the interface modifier (capping layer) in the PCE increased from 8.34% to 9.47%.

One of the common examples is the introduction of antioxidant-carrying 4-fluorobenzohydrazide (FBH) on top of FASnI 3 perovskite films
Similarly, a dense layer of Al 2 O 3 as a buffer layer separating perovskites and HTL can prevent degradation from moisture [117]. Cetyltrimethylammoniu bromide (CTAB) doped zirconium oxide (ZrO x ) can also act in a similar manner [118]. In general, the switch from Pb to Sn affects the morphology severely due to the higher Lewis acidity of Sn +2 compared to Pb +2 [50]. Therefore, one of the major goals when making Sn films is to achieve compact and pinhole-free thin films.

Cation Engineering
Cations play a major role in Sn halide perovskites thin films in regard to lattice strain engineering. Nishimura et al. [119] investigated the relationship between lattice strain in tin-based perovskite films and TPSCs efficiency. They prepared tin-based Q x (FA 0.75 MA 0.25 ) 1−x SnI 3 perovskites, where Q is various cations with different ionic radii such as Na + , K + , Cs + , BA + , and ethylammonium (EA + ). The link between actual measured lattice strain and solar performance was explored. As the tolerance factor approached unity, the lattice strain decreased (measured by the Williamson hall plot of XRD data). As the lattice strain decreased, the performance of the Sn perovskites was enhanced. EA 0.1 (FA 0.75 MA 0.25 ) 0.9 SnI 3 with the lowest lattice strain yielded the best performance, because carrier mobility increased as lattice strain decreased. These lattice strains would disrupt carrier mobility and reduce solar cell performance [119]. The lowest lattice strains were found for Cs-0.1 and EA-0.1 and provided the highest mobility of about 43 cm 2 V −1 ·s −1 ; however, in the case of Na-0.1, the lattice strain was found to be higher and therefore the mobility was down to 4.6 cm 2 V −1 ·s −1 .
Sun et al. [120] added a bi-linkable reductive cation (i.e., formamide (FM)), into FASnI 3 to function as molecular glue for improving the stability and performance of TPSCs by the formyl group (-CHO) and amine group (−NH 2 ). They revealed that the NH 2 and C=O groups in FM are capable of interacting with FA + and Sn +2 through hydrogen bonds and Lewis acid-base coordination, respectively. This resulted in a greater grain size, preferred orientation, lower defect density, and better film stability. The TPSC device based on 10% of FMI resulted in a 40% increased PCE from 5.51% to 7.71% with notable enhanced stability, retaining its initial PCE after one year in N 2 without encapsulation.
Jokar et al. [17] used guanidinium cations (GA + ) as an additive with at least 1% of ethylenediammonium diiodide (EDAI 2 ) to form a FASnI 3 films, and this resulted in the remarkably improved performance of TPSCs. A high PCE of 8.5% was achieved and increased to 9.6% after 2000 h of storage in a glove box. Additionally, the resulting perovskite operated for almost an hour under continuous illumination and for six days in air without encapsulation [17].

Solvent Engineering
Solvents and secondary solvents can play a major role in the formation of pinholes in thin films, especially thin films that contain organic materials [121]. One common way to produce a compact Sn film is by different solvents, such as dimethylformamide (DMF) or dimethyl sulfoxide (DMSO) [122,123]. Post-treatment with antisolvents also plays a crucial role in the quality of tin-based perovskite films [123,124].
It was reported that when perovskite films are formed without any anti-solvent dripping, the precursor is far from supersaturated until the solvent totally evaporates and, as a result, the nucleation site density is rather low, resulting in a flower-like film with limited surface coverage [123]. Therefore, different antisolvents (diethyl ether (DE), toluene (TL), and chlorobenzene (ClB)) were tested. The size of pinholes in the FA 0.75 MA 0.25 SnI 3 films dripped by DE is less than that of pinholes in the film dripped by TL, but the quantity of pinholes is greater. In the case of ClB, the film has a uniform surface with full coverage and clear grain features. One reason for this could be related to its high boiling point of 131 • C, which has a slower evaporation rate, which extends the crystal development period during the thermal annealing process.
Hao et al. [42] investigated the DMSO function as a the Lewis base solvent to adjust the crystallization rate of MASnI 3 perovskite by Lewis acid-base interaction. When DMSO molecules react with Lewis acid SnI 2 , they form the SnI 2 -3DMSO intermediate adduct, which effectively slows down the interaction between MAI and SnI 2 , resulting in an enhanced MASnI 3 film. Similarly, the generation and orientation of FASnI 3 perovskites was controlled when poly-ethylene-co-vinyl acetate (PEVA) was introduced into the anti-solvent [125]. At the grain boundaries, the C=O groups of PEVA molecules cause a complexation between Lewis acid-base interaction and Sn +2 . This results in larger grains and lowered surface defects of FASnI 3 , leading to enhanced devices' performance.

Low-Dimensional Perovskites
In fact, using different solvents incorporated with different additives as well as cations with different radii often has a direct influence on the dimensionality of the perovskite films, which is on its own is a major research and development direction. Lower dimension perovskites seem to be more stable than three-dimensional ones, so these are expected to improve tin-based perovskites' stability [126]. The three-dimensional structure of perovskites could be decreased to two-or one-dimensional by substituting the bulky organic ammonium ions at the A-site in the perovskite lattice or by inserting 2D materials in the precursor solution [127,128]. 2D perovskites seems to have exceptional optoelectronic properties and therefore may make them excellent photovoltaic materials [129]. 2D perovskite reduces moisture as well as oxygen from going inside the film [130,131]. It also can reduce defects, resulting in a low amount unwanted self-doping [132]. Many researchers are currently investigating 2D TPSCs to increase their stability based on the benefits of lower dimension perovskites.
Similarly, low-dimensional Sn perovskites have become a topic of interest in TPSCs due to their ability to improve device performance and stability. In 2017, Liao et al. [133] incorporated phenylethylammonium (PEA) into FASnI 3 perovskites and they achieved perpendicularly oriented, low-dimensional Sn perovskite films with remarkably enhanced stability and a PCE of 5.9%. In 2020, a report by Liang et al. [134] utilizing indene-C 60 bisadduct (ICBA) as an ETM found that their Sn-based perovskite (PEA x FA 1−x SnI 3 ) with PEA incorporation formed a low-dimensional perovskite with reduced defect concentrations, which resulted in a high V OC of 0.94, a record PCE of 12.4%, and better stability (shelf stability of 3800 h).

Variety of Very Recent Perovskite Additives, Surface/interface Modifiers in TPSCs with Noticeable Performance
There are many additives that were reported in recent years to enhance the performance of TPSCs [55,72,[135][136][137]. However, here (Table 1) we summarize most of the very recent and noticeable additives and correlated outstanding device performance of lead-free TPSCs that were reported during the last two years. Table 2 provides a list of the most recent and highly performing surface/interface modifiers that were applied in lead-free TPSCs. Table 3 provides a list of most recent highly performing mixed Pb-Sn perovskites with Pb ≤ 50% and it includes devices with both perovskite additives and surface/interface modifiers. The table also provides structure and reported stability.      It is noteworthy to mention that the reasons behind the enhancement of the performance of the devices listed in the tables are often related to the same reasons. Here, we briefly list the reasons behind the enhancement in general, which is important for further future consideration and development to achieve even higher performance: (i) oxidation, (ii) reduced defects, (iii) controlled crystallization, (iv) morphology (compactness and pinholes, strain relaxation), (v) charge diffusion and extraction (mobility, carriers density, energy levels, recombination), (vi) built-in electric field (gradient vertical perovskite growth), (vii) better choice of cations (reduced or eliminated MA + ) (iix) hydrophobicity, and (ix) passivation of the acidic and hygroscopic surface of the commonly used PEDOT:PSS HTL (or alternative or HTL or SAMs).

Conclusions and Prospects
Currently, there is a significant amount of research that is being carried out on the enhancement of TPSCs. The PCE of lead-free as well as lead-mixed TPSCs is approaching 15% and 24%, respectively. Similarly, the stability of TPSCs is rapidly improving. It may be true that the PCEs and the stability of TPSCs are still behind lead PSCs; however, TPSCs have a wider range of applications, especially due to the lesser toxicity and narrower bandgap of Sn perovskites.
The development of new and improved synthetic methods for Sn-based perovskite materials can help to further boost the efficiency, stability, and scalability of TPSCs. Further investigation of new device structures can lead to further improvements in efficiency and stability. Investigating the use of new interfaces and interlayers can help to improve the stability and efficiency of Sn-based perovskite solar cells. Improving the stability of Snbased perovskite solar cells is still a crucial direction for future research. Strategies such as passivation of defects, encapsulation, and material engineering can help to improve their long-term stability.
It is important to emphasize that Sn-based perovskites exhibit both metallic and semiconducting behavior depending on the preparation method. This is attributed to the presence of metallic Sn phases in the perovskite film at different levels. Therefore, different properties can be observed across the film (bottom surface, bulk, and top surface). This behavior can result in a built-in electric field. In general, this varying conducting nature may result in a trade-off between electrical conductivity and photoelectric performance. As discussed, various strategies have been proposed to reduce the metallic Sn content, and recently, there have been several good attempts to control such problem and to use it to make a controlled built-in field and surfaces. In general, there are several challenges facing TPSCs and manifested in the poor stability of Sn. Additionally, the control of crystallization dynamics (growth and gradient), self-doping, morphology, strains, defects density, oxidation, ion migration, and charge transport and extraction all hinder the performance of TPSCs. However, many successful efforts have been made to resolve these issues, such as the use of various additives, surface/interface modifiers, solvents engineering, crystal dimensionality, and compositional engineering, which are all moving forward in the enhancement of the overall PV performance and stability of TPSCs.
This review summarizes some milestones in the development and the up-to-date progress of tin perovskites and TPSCs. The crystal structure and electrical properties of tin perovskite materials, as well as the cause of their chemical instability, were discussed. Furthermore, the main factors affecting the stability and resulting degradation, such as moisture, oxygen, ion migration, and UV-illumination, were summarized.
Funding: This research received no external funding.