Down-Shifting and Anti-Reflection Effect of CsPbBr3 Quantum Dots/Multicrystalline Silicon Hybrid Structures for Enhanced Photovoltaic Properties.

Over the past couple of decades, extensive research has been conducted on silicon (Si) based solar cells, whose power conversion efficiency (PCE) still has limitations because of a mismatched solar spectrum. Recently, a down-shifting effect has provided a new way to improve cell performances by converting ultraviolet (UV) photons to visible light. In this work, caesium lead bromide perovskite quantum dots (CsPbBr3 QDs) are synthesized with a uniform size of 10 nm. Exhibiting strong absorption of near UV light and intense photoluminescence (PL) peak at 515 nm, CsPbBr3 QDs show a potential application of the down-shifting effect. CsPbBr3 QDs/multicrystalline silicon (mc-Si) hybrid structured solar cells are fabricated and systematically studied. Compared with mc-Si solar cells, CsPbBr3 QDs/mc-Si solar cells have obvious improvement in external quantum efficiency (EQE) within the wavelength ranges of both 300 to 500 nm and 700 to 1100 nm, which can be attributed to the down-shifting effect and the anti-reflection property of CsPbBr3 QDs through the formation of CsPbBr3 QDs/mc-Si structures. Furthermore, a detailed discussion of contact resistance and interface defects is provided. As a result, the coated CsPbBr3 QDs are optimized to be two layers and the solar cell exhibits a highest PCE of 14.52%.


Introduction
For the past few years, silicon (Si) based solar cells have become the most commonly-used materials of photovoltaic devices because of its abundant and non-polluting properties with a mature production process [1][2][3]. By virtue of its high efficiency and low cost, multicrystalline Si (mc-Si) solar cells are produced most extensively among various solar cells [4]. However, crystalline Si solar cells are limited in power conversion efficiency (PCE), as high-energy photons cannot fully be utilized and photons whose energy is inferior to the bandgap of Si have transmission loss [5]. In order to obtain better spectral response, one possible solution is to use luminescent materials converting ultraviolet (UV) photons to visible light by means of a down-shifting effect [6,7]. Recently, multiple reports have demonstrated that the down-shifting mechanism of nanomaterials can improve the PCE of solar cells [8][9][10][11][12]. For example, van Sark et al. calculated in theory that Cd-based quantum dots (QDs), which had an emission at 603 nm, led to an increase of around 10% in the short-circuit current of mc-Si solar cells [13]. Pi et al. fabricated Si QDs on the surface of mc-Si solar cells via the inkjet printing method and found that solar cell exhibited a relative rise of 2% in PCE because of better spectral response within a short wavelength range of 300 nm to 400 nm [14]. On one hand, however, conventional CdS or CdSe QDs are faced with the problems of severe aggregation and photoluminescence (PL) quenching in the process of film fabrication [15]. On the other hand, Si QDs fail to achieve high PL quantum yield (QY) due to their indirect Si bandgap [16][17][18].
With a potential application in light emitting diodes [19][20][21], lasers [22][23][24], photodetectors [25][26][27] and other optoelectronic devices, all inorganic lead halide perovskite QDs (IPQDs) could become alternative materials for the down-shifting effect and photovoltaic applications due to their low cost synthesis method, long-time stability, high optical absorption coefficient, as well as controllable and high intensity PL [28][29][30]. Compared with a relatively low PL QY (<50%) in Si QDs [31,32], IPQDs have PL QYs of 80%, 95%, 70%, for red, green, and blue emissions [33]. It has been reported that the spectral response with near UV light range of 300-390 nm of a Cu(In,Ga)Se 2 (CIGS) thin film solar cell was improved by taking advantage of the down-shifting effect of IPQDs [34]. In the present work, a colloidal approach is introduced to synthesize caesium lead bromide perovskite quantum dots (CsPbBr 3 QDs) that are cubic shaped with a mean size of 10 nm and whose room temperature PL peak is observed at 515 nm. The colloidal CsPbBr 3 QDs solution is then spin-coated onto the surface of commercially produced mc-Si solar cells in order to obtain CsPbBr 3 QDs/mc-Si hybrid structured solar cells. It is found that CsPbBr 3 QDs/mc-Si hybrid structured solar cells have an increase in external quantum efficiency (EQE) within the wavelength ranges of both 300 to 500 nm and 700 to 1100 nm compared with solar cells without CsPbBr 3 QDs, demonstrating that the photovoltaic performances of solar cells can be improved by the down-shifting effect and the anti-reflection property of CsPbBr 3 QDs/mc-Si hybrid structures.

Materials and Methods
CsPbBr 3 QDs were synthesized with a colloidal approach. First, Cs 2 CO 3 (99.9%, 2.5 mmol, Sigma-Aldrich, St. Louis, MO, USA) was added to 40 mL of octadecene (ODE, 90%, Acros, Geel, Belgium) with 2.5 mL of oleic acid (OA, 90%, Sigma-Aldrich) at 130 • C under N 2 atmosphere for 30 min. The solution after reaction was naturally cooled to ambient temperature to obtain the Cs-oleate solution. Second, PbBr 2 (99.999%, 0.188 mmol, Sigma-Aldrich), 5 mL of ODE, 0.5 mL of OA, and 0.5 mL of oleylamine (OLA, 90%, Acros) were mixed and dried at 120 • C under vacuum for 60 min. After complete dissolution of PbBr 2 , the solution saw a rise of 150 • C in temperature under N 2 atmosphere and a quick injection of 0.4 mL of the prepared Cs-oleate solution. The mixture after reaction was placed at this temperature for 5 s and cooled by an ice-water bath to ambient temperature. Finally, the reaction solution was used to purify CsPbBr 3 QDs by centrifugation at 12,000 rpm for 10 min and then re-dispersed in n-hexane (99%, Sigma-Aldrich) to obtain a long-time stable colloidal solution.
The microstructures of CsPbBr 3 QDs were characterized by means of transmission electron microscopy (TEM) and X-ray diffraction (XRD) (MXP-III, Bruker, Inc., Leipzig, Germany). The diluted and highly dispersed CsPbBr 3 QDs solution was dropped onto a carbon-coated Cu grid and dried at room temperature. TEM images were performed by Tecnai G2 operated at 200 kV. A UV-3600 spectrophotometer produced by Shimadzu was applied to measure the optical absorbance of CsPbBr 3 QDs. Equipped with a synapse photomultiplier tube (PMT) detector, a system made by HORIBA Jobin Yvon was used to measure PL spectra. The absorbance and PL spectra were measured at room temperature in a fused silica cuvette using diluted solution of CsPbBr 3 QDs in n-hexane.
In this work, commercially produced mc-Si solar cells with texturized surface were fabricated by Hareonsolar (Wuxi, China), including acid texturization, high temperature diffusion, SiN x film deposition, and metal grid screen-printing. The mc-Si substrate was p-type (1~3 Ω·cm) with a thickness of 200 ± 20 µm and the texturized surface had an average roughness of 0.8~1.6 µm. The surface of mc-Si solar cells was spin-coated with the CsPbBr 3 QDs/n-hexane solution at 2000 rpm for 1 min in a glovebox. CsPbBr 3 QDs have a concentration of 5 mg/mL and mc-Si solar cells have an active area of 4 cm 2 .
Here, layer-by-layer spin-coating process was used to fabricate CsPbBr 3 QDs/mc-Si hybrid structured solar cells. The layer number of CsPbBr 3 QDs varied from one to four. A 610C electrometer made by Keithley (Cleveland, OH, USA) was utilized to measure the current density-voltage (J-V) characteristics of solar cells under the AM 1.5 (100 mW/cm 2 ) illumination. A QEX10 quantum efficiency/spectral response measurement system produced by PV Measurements (Point Roberts, WA, USA) was adopted to measure the EQE spectra of mc-Si solar cells inclusive and exclusive of CsPbBr 3 QDs within the spectral range of 300 to 1100 nm. A standard Si solar cell was used for calibrating both J-V and EQE measurements. Hall Effect was measured at room temperature by LakeShore 8400 with the use of a coplanar van der Pauw (VDP) geometry and films with vacuum-evaporated Al electrodes. A liquid He-cooled spectrometer produced by Bruker EMX (Karlsruhe, Germany) was utilized to obtain low-temperature X-band electron spin resonance (ESR) spectra CsPbBr 3 QD films. Figure 1a shows that CsPbBr 3 QDs prepared in the current experiment present cubic shapes with a uniform size. The high-resolution TEM (HRTEM) image of one CsPbBr 3 QD is presented in Figure 1b. The prepared CsPbBr 3 QDs have a crystalline interplanar spacing of 0.29 nm relative to the (200) crystalline planes of cubic CsPbBr 3 . The distribution of CsPbBr 3 QDs sizes is demonstrated in Figure 1c. The quantum confinement effect of CsPbBr 3 QDs is expectable since their mean size (about 10 nm) approaches the Bohr diameter (7 nm) that was predicted by the Wannier-Mott excitons of bulk CsPbBr 3 perovskites [35]. The pattern of XRD presented in Figure 1d

Optical Properties of CsPbBr 3 QDs
It can be seen in Figure 2 that CsPbBr 3 QDs have quite high absorbance in the region of short wavelength and the absorption edge locates at 520 nm (2.38 eV), suggesting that the blue-shift of the bandgap corresponds to bulk CsPbBr 3 with 2.25 eV [36], which accords with the quantum confinement effect. In addition, the PL spectrum of CsPbBr 3 QDs excited by a He-Cd laser of 325 nm is also presented in Figure 2, showing an intense peak at 515 nm with width as narrow as 20 nm at half height. The observed high intensity and color purity PL can be attributed to the uniform size distribution of CsPbBr 3 QDs, as identified by TEM measurements. Moreover, the PL QY is measured to be as high as 80%, by using standard fluorescence dye as a reference. It is demonstrated that CsPbBr 3 QDs can strongly absorb the near UV photons and then efficiently emit visible light, indicating their suitable down-shifting applications.

Optical Properties of CsPbBr3 QDs
It can be seen in Figure 2 that CsPbBr3 QDs have quite high absorbance in the region of short wavelength and the absorption edge locates at 520 nm (2.38 eV), suggesting that the blue-shift of the bandgap corresponds to bulk CsPbBr3 with 2.25 eV [36], which accords with the quantum confinement effect. In addition, the PL spectrum of CsPbBr3 QDs excited by a He-Cd laser of 325 nm is also presented in Figure 2, showing an intense peak at 515 nm with width as narrow as 20 nm at half height. The observed high intensity and color purity PL can be attributed to the uniform size distribution of CsPbBr3 QDs, as identified by TEM measurements. Moreover, the PL QY is measured to be as high as 80%, by using standard fluorescence dye as a reference. It is demonstrated that CsPbBr3 QDs can strongly absorb the near UV photons and then efficiently emit visible light, indicating their suitable down-shifting applications.

Photovoltaic Properties of CsPbBr3 QDs/mc-Si Hybrid Structured Solar Cells
CsPbBr3 QDs/mc-Si hybrid structured solar cells were fabricated after spin-coating the colloidal CsPbBr3 QDs solution onto the surface of mc-Si solar cells. Measurements were carried out for the J-V characteristics of solar cells under the AM 1.5 illumination. Figure   In general, cell performances strongly depend on the layer number of CsPbBr3 QDs. As shown in Figure 3b, CsPbBr3 QDs/mc-Si hybrid structured solar cells have higher Jsc compared with ref_mc-Si solar cell when the layer number of CsPbBr3 QDs is one to three. In particular, Jsc increases from 36.14 mA/cm 2 to 37.48 mA/cm 2 when the layer number is two, which is considered to result from better spectral utilization. However, the Jsc of 4_L_mc-Si cell drops to 33.76 mA/cm 2 , even below that of mc-Si solar cell without CsPbBr3 QDs. In principle, the significant reduction of Jsc can be explained by the following two reasons. The first reason should be the induced contact resistance in CsPbBr3 QDs layers. As we know, undoped CsPbBr3 QDs have poor electrical conductivity. Through the room temperature Hall Effect measurement, the CsPbBr3 QDs film has a dark conductivity of about 3.6 × 10 −7 S/cm, which is very low in the order of magnitude according to the previous reports of metal halide perovskite materials [37][38][39]. In this study, Jsc drops off due to the increase of contact resistance, which deteriorates the carrier collection efficiency. The other reason is the defect in hybrid structures which acts as a non-radiative recombination center and results in thermal energy loss. In order to confirm the existence and study the behavior of defects in hybrid structures, a liquid He-cooled spectrometer of Bruker EMX 10/12+ whose center field is 3342.5 G is used to obtain the lowtemperature X-band ESR spectrum of CsPbBr3 QDs/mc-Si structure, as shown in Figure 4. The Xband ESR spectrum at 4 K shows an ESR signal with g = 2.006. In previous works, this signal was usually observed in disordered materials and corresponding to the dangling bond defects derived In general, cell performances strongly depend on the layer number of CsPbBr 3 QDs. As shown in Figure 3b, CsPbBr 3 QDs/mc-Si hybrid structured solar cells have higher J sc compared with ref_mc-Si solar cell when the layer number of CsPbBr 3 QDs is one to three. In particular, J sc increases from 36.14 mA/cm 2 to 37.48 mA/cm 2 when the layer number is two, which is considered to result from better spectral utilization. However, the J sc of 4_L_mc-Si cell drops to 33.76 mA/cm 2 , even below that of mc-Si solar cell without CsPbBr 3 QDs. In principle, the significant reduction of J sc can be explained by the following two reasons. The first reason should be the induced contact resistance in CsPbBr 3 QDs layers. As we know, undoped CsPbBr 3 QDs have poor electrical conductivity. Through the room temperature Hall Effect measurement, the CsPbBr 3 QDs film has a dark conductivity of about 3.6 × 10 −7 S/cm, which is very low in the order of magnitude according to the previous reports of metal halide perovskite materials [37][38][39]. In this study, J sc drops off due to the increase of contact resistance, which deteriorates the carrier collection efficiency. The other reason is the defect in hybrid structures which acts as a non-radiative recombination center and results in thermal energy loss. In order to confirm the existence and study the behavior of defects in hybrid structures, a liquid He-cooled spectrometer of Bruker EMX 10/12+ whose center field is 3342.5 G is used to obtain the low-temperature X-band ESR spectrum of CsPbBr 3 QDs/mc-Si structure, as shown in Figure 4. The X-band ESR spectrum at 4 K shows an ESR signal with g = 2.006. In previous works, this signal was usually observed in disordered materials and corresponding to the dangling bond defects derived from the chemical synthesis and spin-coating process, and poor adhesion of coating films on substrates [40][41][42]. It is worth noting that no ESR signal can be detected in the ref_mc-Si solar cell. As a result, the ESR signal here results from the lone-pair electrons (like dangling bonds defects) on the surface and interfaces of CsPbBr 3 QDs layers. The density of induced surface and interface defects increases with the increasing layer number of CsPbBr 3 QDs, indicating a decline in the J sc of solar cells because of the enhanced carrier recombination. Nanomaterials 2020, 10, x FOR PEER REVIEW 7 of 13 from the chemical synthesis and spin-coating process, and poor adhesion of coating films on substrates [40][41][42]. It is worth noting that no ESR signal can be detected in the ref_mc-Si solar cell. As a result, the ESR signal here results from the lone-pair electrons (like dangling bonds defects) on the surface and interfaces of CsPbBr3 QDs layers. The density of induced surface and interface defects increases with the increasing layer number of CsPbBr3 QDs, indicating a decline in the Jsc of solar cells because of the enhanced carrier recombination. As shown in Figure 3c, the change of Voc with the layer number of CsPbBr3 QDs tends to be linear. When the layer number increases, Voc decreases slightly from 612.1 to 608.5 mV because of the surface and interface defects induced by CsPbBr3 QDs layers. As shown in Figure 3d, FF declines obviously when the layer number increases to four, which may be owing to an increase in series resistance (Rs). A negative correlation is found between FF and Rs. Equation (1) below displays the relationship between the voltage and current density of a single-diode model: wherein, J0 and Jp are saturation current density and photocurrent density, respectively, Rs represents series resistance, Rsh represents shunt resistance, n refers to ideality factor, q is electron charge, kB is Boltzmann constant and T is temperature. The Rs values of ref_mc-Si and 4_L_mc-Si cells extracted by a fit to the illuminated J-V curves are 1.2 and 2.8 Ω, respectively. As discussed before, contact resistance increases with the increasing layer number of CsPbBr3 QDs, which in turn give rise to an obvious decline in FF. Finally, the optimal mc-Si solar cell coated with two layers of CsPbBr3 QDs leads to the best PCE of 14.52%, as shown in Figure 3e. The EQE spectra of mc-Si solar cells inclusive and exclusive of CsPbBr3 QDs layers were measured to further study the down-shifting mechanism of CsPbBr3 QDs/mc-Si hybrid structured solar cells. As observed in Figure 5, the EQE of CsPbBr3 QDs/mc-Si hybrid structured solar cells has a great increase within the spectral range of 300 to 500 nm when the layer number of CsPbBr3 QDs is 1 to 3, which should be attributed to the formation of CsPbBr3 QDs, as discussed before. It suggests that CsPbBr3 QDs are capable of absorbing the near UV light and emitting photons in the region of visible light, which could enhance the spectral response in the region of short wavelength through the re-absorption of mc-Si substrates. When the layer number increases to 4, nevertheless, EQE decreases obviously almost in the whole spectral range, even below that of ref_mc-Si cell, which agrees with the J-V results. Another interesting finding is that the EQE of CsPbBr3 QDs/mc-Si hybrid structured solar cells also increases within the spectral range of 700 to 1100 nm, which will be As shown in Figure 3c, the change of V oc with the layer number of CsPbBr 3 QDs tends to be linear. When the layer number increases, V oc decreases slightly from 612.1 to 608.5 mV because of the surface and interface defects induced by CsPbBr 3 QDs layers. As shown in Figure 3d, FF declines obviously when the layer number increases to four, which may be owing to an increase in series resistance (R s ). A negative correlation is found between FF and R s . Equation (1) below displays the relationship between the voltage and current density of a single-diode model: wherein, J 0 and J p are saturation current density and photocurrent density, respectively, R s represents series resistance, R sh represents shunt resistance, n refers to ideality factor, q is electron charge, k B is Boltzmann constant and T is temperature. The R s values of ref_mc-Si and 4_L_mc-Si cells extracted by a fit to the illuminated J-V curves are 1.2 and 2.8 Ω, respectively. As discussed before, contact resistance increases with the increasing layer number of CsPbBr 3 QDs, which in turn give rise to an obvious decline in FF. Finally, the optimal mc-Si solar cell coated with two layers of CsPbBr 3 QDs leads to the best PCE of 14.52%, as shown in Figure 3e. The EQE spectra of mc-Si solar cells inclusive and exclusive of CsPbBr 3 QDs layers were measured to further study the down-shifting mechanism of CsPbBr 3 QDs/mc-Si hybrid structured solar cells. As observed in Figure 5, the EQE of CsPbBr 3 QDs/mc-Si hybrid structured solar cells has a great increase within the spectral range of 300 to 500 nm when the layer number of CsPbBr 3 QDs is 1 to 3, which should be attributed to the formation of CsPbBr 3 QDs, as discussed before. It suggests that CsPbBr 3 QDs are capable of absorbing the near UV light and emitting photons in the region of visible light, which could enhance the spectral response in the region of short wavelength through the re-absorption of mc-Si substrates. When the layer number increases to 4, nevertheless, EQE decreases obviously almost in the whole spectral range, even below that of ref_mc-Si cell, which agrees with the J-V results. Another interesting finding is that the EQE of CsPbBr 3 QDs/mc-Si hybrid structured solar cells also increases within the spectral range of 700 to 1100 nm, which will be discussed below. Based on EQE results, J sc contributed from the spectral response of solar cells in different wavelength ranges can be calculated according to Equation (2) as follows: wherein, F(λ) and E(λ) are incident light flux and energy of photons with the wavelength of λ, respectively. Compared with ref_mc-Si cell, the J sc of 2_L_mc-Si cell contributed from spectral response within spectral range of 300 to 500 nm and 700 to 1100 nm increases from 5.98 mA/cm 2 to 6.79 mA/cm 2 and 14.15 mA/cm 2 to 14.52 mA/cm 2 , respectively. As reported by the work of Pi et al., the anti-reflection of prepared porous Si QDs films improved the efficiency of crystalline Si (c-Si) solar cells [43]. In this study, the reflection characteristics of mc-Si solar cells inclusive and exclusive of CsPbBr 3 QDs layers must be taken into consideration.
Nanomaterials 2020, 10, x FOR PEER REVIEW 8 of 13 discussed below. Based on EQE results, Jsc contributed from the spectral response of solar cells in different wavelength ranges can be calculated according to Equation (2) as follows: wherein, ( ) and ( ) are incident light flux and energy of photons with the wavelength of , respectively. Compared with ref_mc-Si cell, the Jsc of 2_L_mc-Si cell contributed from spectral response within spectral range of 300 to 500 nm and 700 to 1100 nm increases from 5.98 mA/cm 2 to 6.79 mA/cm 2 and 14.15 mA/cm 2 to 14.52 mA/cm 2 , respectively. As reported by the work of Pi et al., the anti-reflection of prepared porous Si QDs films improved the efficiency of crystalline Si (c-Si) solar cells [43]. In this study, the reflection characteristics of mc-Si solar cells inclusive and exclusive of CsPbBr3 QDs layers must be taken into consideration.  Figure 6 shows the optical reflection (R) spectra of mc-Si solar cells and CsPbBr3 QDs/mc-Si hybrid structured solar cells. Obviously, CsPbBr3 QDs layers lead to the decrease of reflection within the spectral ranges of both 300 to 500 nm and 700 to 1100 nm. The reduction of reflection in long wavelength region is mainly induced by the nanostructure of CsPbBr3 QDs layers. Meanwhile, a greater decline in reflection in short wavelength region should be ascribed to the anti-reflection property of nanostructures and the absorption of CsPbBr3 QDs themselves, as shown in Figure 2.  Figure 6 shows the optical reflection (R) spectra of mc-Si solar cells and CsPbBr 3 QDs/mc-Si hybrid structured solar cells. Obviously, CsPbBr 3 QDs layers lead to the decrease of reflection within the spectral ranges of both 300 to 500 nm and 700 to 1100 nm. The reduction of reflection in long wavelength region is mainly induced by the nanostructure of CsPbBr 3 QDs layers. Meanwhile, a greater decline in reflection in short wavelength region should be ascribed to the anti-reflection property of nanostructures and the absorption of CsPbBr 3 QDs themselves, as shown in Figure 2.
In order to evaluate the contributions from the down-shifting and anti-reflection effect, an enhancement factor (EF) is defined for both the EQE and absorption results: wherein, A is the optical absorption of hybrid structures, which can be deduced by A = 1 − R. Figure 7 shows the EF of 2_L_mc-Si cell as a function of wavelength. It can be clearly seen that the decrease of reflection (which means the enhancement of absorption) improves EQE within the wavelength range of 700 to 1100 nm. However, in wavelength range of 300 to 450 nm, the anti-reflection effect cannot overlap with all the enhancement of EQE result. For example, at 320 nm, the EQE enhancement is 27% while the absorption enhancement is only 4%, which indicates that the down-shifting effect of CsPbBr 3 QDs dominates the improving spectral response in the short wavelength region. In contrast, at 480 nm, the CsPbBr 3 QDs/mc-Si structures show the strongest anti-reflection property. The enhancements of EQE and absorption are almost the same. Hence, the EQE enhancement is mainly due to the anti-reflection of hybrid structures. In a word, we conclude that the improved photovoltaic performances can be attributed both to the down-shifting effect and the anti-reflection property of CsPbBr 3 QDs by forming CsPbBr 3 QDs/mc-Si hybrid structures. Furthermore, for future photovoltaic application, in order to avoid the environmental pollution caused by lead, a protected layer will be introduced into the hybrid structures to reduce the lead leakage [44,45]. In order to evaluate the contributions from the down-shifting and anti-reflection effect, an enhancement factor (EF) is defined for both the EQE and absorption results: wherein, A is the optical absorption of hybrid structures, which can be deduced by A = 1 − R. Figure  7 shows the EF of 2_L_mc-Si cell as a function of wavelength. It can be clearly seen that the decrease of reflection (which means the enhancement of absorption) improves EQE within the wavelength range of 700 to 1100 nm. However, in wavelength range of 300 to 450 nm, the anti-reflection effect cannot overlap with all the enhancement of EQE result. For example, at 320 nm, the EQE enhancement is 27% while the absorption enhancement is only 4%, which indicates that the downshifting effect of CsPbBr3 QDs dominates the improving spectral response in the short wavelength region. In contrast, at 480 nm, the CsPbBr3 QDs/mc-Si structures show the strongest anti-reflection property. The enhancements of EQE and absorption are almost the same. Hence, the EQE enhancement is mainly due to the anti-reflection of hybrid structures. In a word, we conclude that the improved photovoltaic performances can be attributed both to the down-shifting effect and the anti-reflection property of CsPbBr3 QDs by forming CsPbBr3 QDs/mc-Si hybrid structures. Furthermore, for future photovoltaic application, in order to avoid the environmental pollution caused by lead, a protected layer will be introduced into the hybrid structures to reduce the lead leakage [44,45].

Conclusions
In conclusion, CsPbBr3 QDs are fabricated with a colloidal synthesis approach. TEM and XRD measurements reveal that cubic CsPbBr3 QDs are formed with an average size of 10 nm. It is observed that CsPbBr3 QDs can strongly absorb the near UV light and present a room temperature PL peak at 515 nm, suggesting their typical down-shifting mechanism. Moreover, CsPbBr3 QDs/mc-Si hybrid

Conclusions
In conclusion, CsPbBr 3 QDs are fabricated with a colloidal synthesis approach. TEM and XRD measurements reveal that cubic CsPbBr 3 QDs are formed with an average size of 10 nm. It is observed that CsPbBr 3 QDs can strongly absorb the near UV light and present a room temperature PL peak at 515 nm, suggesting their typical down-shifting mechanism. Moreover, CsPbBr 3 QDs/mc-Si hybrid structured solar cells containing CsPbBr 3 QDs of different layers are fabricated. According to the findings, the EQE of CsPbBr 3 QDs/mc-Si hybrid structured solar cells is increased within the wavelength ranges of both 300 to 500 nm and 700 to 1100 nm compared with mc-Si solar cells without CsPbBr 3 QDs, which should be attributed to the broadband anti-reflection characteristics of nanostructures and the additionally improved down-shifting effect of CsPbBr 3 QDs. However, the higher contact resistance and density of surface and interface defects resulting from the increasing layer number of CsPbBr 3 QDs deteriorate cell performances due to the reduction of carrier collection efficiency. As a result, the optimal mc-Si solar cell coated with two layers of CsPbBr 3 QDs contributes to achieving the best PCE of 14.52%. It is worth noting that all inorganic CsPbBr 3 QDs have better stability than the organic-inorganic (MAPbBr 3 ) perovskite materials. Our experimental results indicate a promising way to exploit CsPbBr 3 QDs for future photovoltaic devices.