Manganese Dioxide (MnO2) Nanoparticles Passivated Perovskite Solar Cell for Improved Power Conversion Efficiency

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Manganese Dioxide (MnO₂) Nanoparticles Passivated Perovskite Solar Cell for Improved Power Conversion Efficiency

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Solar Forecasting and Smart Photovoltaic Systems

Submitted:

05 May 2024

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07 May 2024

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Abstract

Passivating the grain boundaries is completely very crucial in the enhancement of the performance of halide perovskite solar cells (PSCs). Here, a novel organolead halide perovskite (CH₃NH₃PbI₃) was synthesized using solution processes-based method to sensitize 1D titanium dioxide (TiO₂) and reduced graphene oxide (RGO) nanoparticles for all-solid-state halide perovskite solar cells. TiO₂ and RGO were synthesized via sol-gel and Hummers’ methods, respectively, and incorporated at the electron transport layer (ETL) in planar PSCs. Additionally, MnO₂was prepared by chemical method, and used to enhance graphite counter electrode. ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr and ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ planar PSCs were fabricated via spin coating method. ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ film achieved a power conversion efficiency (PCE) of 10.79%, short circuit current (Jsc) of 19.0 mAcm^-2and fill factor (FF) of 51.53% compared to PCE of 8.64%, Jsc of 16.25 mAcm^-2and FF of 47.48% achieved for ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr film. The enhancement value of 22.85% was achieved from J-V curves after exposing the ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr and ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ films to Keithley 2400 sourcemeter (Keithley Instrument Inc.) under AM 1.5G (100 mWcm^-2) (Newport) solar illumination in order to test their photovoltaic performance. This study shows that MnO₂ nanoparticle has a proven capability to improve the photovoltaic performance of PSCs.

Keywords:

Subject: Physical Sciences - Applied Physics

1. Introduction

PSC has a strong possibility for future commercialization owing to its high photoconversion efficiency. The current record for a single-junction perovskite solar cell has now reached 23.7% PCE surpassing the mainstream silicon solar cell. Nonetheless, structural defects such as dangling bonds and vacancies are formed at the GBs due to preparation via solution-based process and crystallization at low temperatures (<100 ^oC) (Han et al., 2018). Dangling bond provide highways for the migration of ionic and molecular species, and also act as charge recombination centres, leading to recombination, hindering charge mobility and extraction, decreasing photovoltaic performance (Shao et al., 2016). Perovskite films are liable to attack from moisture within GBs, leading to decomposition and poor device stability (Jiang et al., 2016). Because of this, many efforts have been sought to passivate GBs and interfaces to modify the efficiency of PSCs (Yang et al., 2018).

Reports have shown that self-passivation using excess PbI₂ and CH₃NH₃I reduced recombination loss at GBs (Son et al., 2016). But then, these self-passivation methods are sensitive to the preparation conditions, resulting in difficulties associated with reproducibility (Yang et al., 2019). Other studies showed that excess PbI₂ are detrimental to the overall PCE (Tumen-Ulzii et al., 2020). Many other passivation agents have been developed to improve the performance. Organic Lewis acids and bases such as buckminsterfullerene (

C_{60}

) (Wang et al., 2014), (6,6)-phenyl-

C_{61}

-butyric acid and methyl ester (PCBM) (Shao et al., 2014) have efficiently reduced the recombination centres in perovskite films leading to increased enhancement in photovoltaic performance. Also, inorganic transition oxide materials such as NiO

x

, Cr₂O₄, ZrO₂, Ag and MnO₂ have a proven passivation capabilities owing to their astonishing structural modularity, straightforward application methods and versatile passivation influences (Gao et al., 2022). MnO₂ has an attractive renewed interest as a promising material owing its high energy density, high theoretical capacitance and completely astonishing structural modularity (Markus et al., 2023). Here, combining graphite and MnO₂ nanoparticle can improve the photovoltaic performance of PSCs

2. Theoretical Consideration

The band gap of perovskite film is calculated by Tauc’s plot (Awodugba et al., 2011) which is expressed as:

{(\propto h ν)}^{\frac{1}{n}} ═ (h ν ─ E_{g})

(1)

α = \frac{A}{d}

(2)

The grain size of the perovskite was calculated using intercept technique, given as (Cheng et al., 2018):

g = \frac{b}{a}

(3)

where a is the number of intersection, and b is the actual length of the line. However, actual length is the ratio of the measured length by the magnification

For the determination of interplanar distance Bragg’s law was used

n λ = 2 d s i n Ɵ

(4)

Here

Ɵ

is the one half of peak diffraction angle or Bragg’s angle, d is the interplanar distance,

λ

represents the Cu K(α) wavelength, which in our case is 1.5418 A and n is the mode of vibration.

The crystallite size (L) was determined from the Scherrer equation

L = \frac{K λ}{β c o s Ɵ}

(5)

where K is the Scherrer constant (0.9),

λ

is the wavelength and

β

is the full width (in radians) of the peak at the half maximum (FWHM) intensity and

Ɵ

is the one half of peak diffraction angle or Bragg’s angle.

Lattice stain (ɛ) of the materials was calculated by the relation

ɛ = \frac{β c o s Ɵ}{4}

(6)

Ɵ

is the one half of peak diffraction angle or Bragg’s angle and ɛ is the lattice strain.

The dislocation density δ was calculated using the relation

δ = \frac{1}{L^{2}}

(7)

where δ is the dislocation density and L is the crystallite size

The number of reduced graphene oxide layer was calculated using the relation

N_{G P} = \frac{L_{002}}{d_{002}}

(8)

where

d_{002}

is the d-spacing,

N_{G P}

is the number of reduced graphene oxide layer and

L_{002}

is the crystallite size.

To measure the efficiency of a solar cell, the current density of a device is obtained as a function of applied voltage. Such a curve provides the parameters required to calculate efficiency (Walton, Wynne (2018))

η ═ \frac{p_{o u t}}{p_{i n}} ═ \frac{J_{s c} V_{O C} F F}{p_{i n}}

(9)

where ƞ is efficiency, P_out is the output power of a device, P_in the input power of the incident light, J_sc is the short-circuit current density.

V_oc is the open-circuit voltage, and FF is a fill factor

F F ═ \frac{J_{m p V_{m p}}}{J_{s c} V_{o c}}

(10)

where J_mp, and V_mp are the current density and voltage of the device at its maximum power point, where the value of J × V is at its maximum in the JV curve. Therefore, to design a high-efficiency solar cell, one may aim to improve the J_sc, V_oc, or FF.

3. Materials and Methods

3.1. Materials

Lead (II) iodide (PbI₂) 98% purity, titanium isopropoxide (C₁₂H₂₈O₄Ti) 96% purity, methyl ammonium iodide (CH₃NH₃I) 98% purity, graphite, potassium per manganese (KMnO₄) 96% purity, dimethyl formamide (DMF) 97% purity, isopropanol (CH₃CH(OH)CH₃) 99% purity, ethanol (CH₃CH₂OH) 99% purity, hydrochloric acid (HCl) 97% purity, hydrogen tetraoxosulphate (VI) acid (H₂SO₄) 97% purity indium doped tin oxide (ITO) glass and detergent were purchased from commercial suppliers (Fisher Scientific or Sigma-Aldrich).

3.2. Experimental Method

3.2.1. Synthesis of Methyl Ammonium Lead Triiodide (CH₃NH₃PbI₃)

Lead (II) iodide (PbI₂) was preheated for 10 minutes at 100 ^oC to evaporate possible humidity within. First, in a process to dissolve PbI₂, 578 mg of it and 200 mg of methyl ammonium iodide (CH₃NH₃I) were mixed with 1 mL of DMF in a test tube and heated 250 ^oC. This temperature was maintained until PbI₂ completely dissolved. The solution was stirred to prevent crystallization of PbI₂. Face mask would be used as safety precaution to prevent the harmful hazard of lead. The perovskite solution was prepared prior to its used because CH₃NH₃I is extremely sensitive to moisture.

CH₃NH₃I + PbI₂ →CH₃NH₃PbI₃

(11)

3.2.2. Synthesis of Titanium Dioxide (TiO₂)Nanoparticles

0.4M of Titanium Isopropoxide was mixed with 1.4M of acetyl acetone and stirred manually for 5 minutes.0.2M of ethanol was then be added to the mixture, and stirred for another 5 minutes. Acetyl acetonate served as stabilizer.

C₁₂H₂₈O₄Ti + CH₃CH₂OH →Ti(OC₅H₁₁)₄ + 4H₂O →Ti(OH)₄ + C₅H₁₁OH (Hydrolysis)
Ti(OH)₄→TiO₂+TiO₂.2H₂O+2H₂O (Polymerization)

(12)

3.2.3. Synthesis of RGO Nanoparticles

At first, the mixture of 5g of graphite and 15g of potassium per manganese was added slowly to 400mL of 0.5 M hydrogen tetraoxosulphate (VI) acid solution in a three neck flask. The mixture was simultaneously stirred and heated at 50 ^oC for 2 hours using a magnetic stirrer hot plate (modl 78-1). After complete mixing of the solution, 3mL of hydrogen peroxide and 200g of ice was added to the solution to stop the reaction. Thereafter, the mixture was filtered using a filter paper. The residue was then washed with 200mL of distilled water to neutralize the pH and 200mL of 3.2 M hydrochloric acid to remove metal ions. Afterward, 200 mL of ethanol was added to dry the RGO nanoparticles.

3.2.4. Synthesis of MnO₂ Nanoparticles

12 mL of ethanol (CH₃CH₂OH) 99% purity, was added slowly to 12 mL of distilled water in a three neck flask, and the mixture was added to 6 mL of 0.5 M potassium permanganate (KmnO₄) solution. The mixture was stirred for 5 minutes using a magnetic stirrer. Thereafter, 3mL of hydrogen peroxide was added as reducing agent and stirred for another 5 minutes to prevent agglomeration. Thereafter, the mixture was filtered using a filter paper. The residue was then washed with 100 mL of ethanol was added to dry the MnO₂ nanoparticles.

3.2.5. Glass/ITO/RGO/TiO₂/CH₃NH₃I₃/Graphite- MnO₂ Device Fabrication

The ITO glass slides was cleaned using standard glass cleaning agents in base bath (cleaning agents: deionized water, 1:20), followed by rinsing with deionized water, propanol and ethanol. The glass slides were then dried in an ovum. 2.00 M TiO₂ solution was be prepared in ethanol. One layer of TiO₂ was deposited on the ITO slide glass through spin-coating process (2000 rpm for 30 s) and annealed at 400^oC for 1 hr.1.00 M of RGO was prepared in ethanol. One layer of TiO₂ was spin-coated at 2000 rpm for 30 s and annealed at 400^oC for 1 hr. A solution of 578 mg of PbI₂ and 200 mg of CH₃NH₃I in 1 mL of DMF was prepared, heated at 250^oC, and deposited via spin coating steps (2000 rpm for 20 s, 2000 rpm for 10 s). The CH₃NH₃I₃ was allowed to dry for 1 hr. 1.00 M of MnO₂ was prepared in ethanol and 1mL of it was mixed with 5 mL of a solution of 0.006g graphite in 0.04g of ethanol. Afterward enhanced graphite was deposited by spin coating (2000 rpm for 30 s).

3.2.6. Glass/ITO/RGO/TiO₂/CH₃NH₃I₃/Graphite Device Fabrication

The ITO glass slides was cleaned using standard glass cleaning agents in base bath (cleaning agents: deionized water, 1:20), followed by rinsing with deionized water, propanol and ethanol. The glass slides were then dried in an ovum. 2.00 M TiO₂ solution was be prepared in ethanol. One layer of TiO₂ was deposited on the ITO slide glass through spin-coating process (2000 rpm for 30 s) and annealed at 400^oC for 1 hr.1.00 M of RGO was prepared in ethanol. One layer of TiO₂ was spin-coated at 2000 rpm for 30 s and annealed at 400^oC for 1 hr. A solution of 578 mg of PbI₂ and 200 mg of CH₃NH₃I in 1 mL of DMF was prepared, heated at 250^oC, and deposited via spin coating steps (2000 rpm for 20 s, 2000 rpm for 10 s). The CH₃NH₃I₃ was allowed to dry for 1 hr. Afterward enhanced graphite was deposited by spin coating (2000 rpm for 30 s) from a solution of 0.006g graphite in 0.04g of ethanol.

3.3. Characterization of the Films

The Ultraviolet-visible spectrophotometer (Lambda 950) was used to study the optical properties such as intensity and wavelength of the absorption spectral of the formed films. X-ray diffraction patterns were obtained with Rigaku D/Max-lllC X-ray diffractometer developed by the Rigaku Int. Corp. Tokyo, Japan, and set to produce diffractions at scanning rate of 2 ^o/min in the 2 to 50^o at room temperature with a CuKa radiation set at 40kV and 20mA. Scanning electron microscopy (SEM) images were acquired using a JEOL JSM-6010LV microscope at an accelerating voltage of 15 KV, and a working distance of 11 mm. All spectra were recorded from 4000 to 400 cm-1 using the Pelkin Elmer 3000 MX spectrometer. Scans were 32 per spectrum with a resolution of 4 cm¹.The IR spectra were analysed using the spectroscopic software Win-IR Pro Version 3.0 with a peak sensitivity of 2 cm^-1.

4. Results

4.1.1. Optical Characterization of CH₃NH₃PbI₃

Figure 1a shows absorbance-wavelength plot of CH₃NH₃PbI₃ with its distinct absorption edges. It is clear that the absorption onset systemically located at 652 nm. Besides, the graph reveals another absorbance peaks corresponding to 722 nm. This shows that CH₃NH₃PbI₃ absorbs within the visible region with longer wavelength range of between 395-800 nm. Transmittance-wavelength plot in Figure 1b clearly shows the transmittance onset at 485 nm. The plot shows gradual increase in transmittance between the wavelength range of 485 nm -650 nm, and transmits steadily within the visible region of solar spectrum with longer wavelength range between 500 - 800 nm. The bandgap of the synthesized CH₃NH₃PbI₃ film in Figure 1c is 1.67 eV. The bandgap value of 1.67 eV for perovskite is within the acceptable range 1.6 - 1.9 eV (Masclocene et al., 2021)

Figure 1. (a)Absorbance-wavelength plot of CH₃NH₃PbI₃ (b) Transmittance-wavelength plot of CH₃NH₃PbI₃ (c) (αhv)²-Eg plots of CH₃NH₃PbI_3.

4.1.2. FTIR Characterization of CH₃NH₃PbI₃ Film

Several molecular vibration frequencies are identified which include

{C H_{3} N H}_{3}^{+}

(

V_{{C H_{3} N H}_{3}^{+}}

,1029.00 cm^-1), C=N (V_C=N, 1742.77 cm^-1), C-C (V_C-C, 726.26 cm^-1), C-H (V_C-H, 2924.00 and 2857.00 cm^-1), C-O-C (V_C-O-C, 1165.00 cm^-1), NH₂ (

V_{N H 2}, 3305.00

cm^-1) and O-H (V_C-OH,3455.00 cm^-1). These functional groups are in keeping with cubic phase of CH₃NH₃PbI₃ halide perovskite.

Table 1. Summary of bondtypes and wavenumbers in CH₃NH₃PbI₃ FTIR spectrum.

Figure 2. FTIR spectra of CH₃NH₃PbI₃ film showing bond type and wavenumber.

4.1.3. XRD Characterization of CH₃NH₃PbI₃ Halide Perovskite Film

XRD measurements were performed and results are shown in Figure 3. The most prominent perovskite peak is at the (101) reflection, observed at 2θ =28.8^o compatible with a single- crystalline phase. Three other strong diffraction peaks are located at 32.0^o, 45.4^o and 56.1^o corresponding to the (100), (200) and (220) crystal planes of cubic phase CH₃NH₃PbI₃ halide perovskite respectively. Additionally, the presence of peaks at 28.8^o and 45.4^o indicates presence of CH₃NH₃I crystallization in perovskite films, supporting the conversion of the precursor materials into CH₃NH₃PbI₃ films, and the appearance of the diffraction angles 28.8^o.confirmed cubic phase CH₃NH₃PbI₃ halide perovskite. From the data in Table 2, the average crystallite size and d-spacing were calculated to be ̴ 7.86 nm and ̴ 1.79 Å respectively.

Table 2. Structural parameters of in CH₃NH₃PbI₃ film.

Figure 3. XRD pattern of CH₃NH₃PbI₃ film.

4.1.4. SEM Analysis of CH₃NH₃PbI₃ Film

Figure 4 a,b show the SEM images of CH₃NH₃PbI₃ film at 7000 and 8000 magnifications. The Figure 4 shows high film coverage, compact structure, uniform morphology and smooth surface with apparent grain boundries typical of CH₃NH₃PbI₃ films prepared by solution process in one step. No cracks were observed. In perovskite films, the smoothness of each layer is crucial for interface contact. The smooth surface of perovskite thin films lead to the reduced interface resistance of the perovskite, and reduce charge recombination loss at the interface of perovskites. It was reported that the smoothness of perovskite film is necessary to obtain high quality interfaces and high photoconversion efficiency.

Figure 4. SEM images of CH₃NH₃PbI₃ film.

4.2.1. FTIR Characterization of TiO₂, RGO and MnO₂ Nanoparticles

As seen in Figure 4a, several molecular vibration frequencies are identified which include OH (

V_{O H}

3380.00 cm^-1,1619.00 cm^-1), C-H (V_C-H, 2355.00 cm^-1) and Ti-O-Ti (V _Ti-O-Ti, 560.00 cm^-1, 460.00 cm^-1). As see Figure 4b, the hydroxyl compound functional group (–OH) formed at the peak with a wavenumber of 3438.51 cm ^{– 1}, the aromatic carbon functional group (C=C) formed at the peak with a wavenumber of 1665.02 cm ^{– 1}, and the epoxy functional group (–CO) formed at the peak with a wavenumber of 1216.14 cm ^{– 1}. Additionally, alkoxy functional group(–C–O) is located at the peak with a wavenumber 1028.88 cm ^{– 1} and the absorption peak with a wavenumber of 2886.00 cm^{– 1} signifying the existence –C-H stretching mode (Konios et al., 2014). Figure 4c represents the FTIR spectrum of MnO₂ nanoparticles. Two broad bands appear at 3400.00 cm^-1 and 1650.00 cm^-1. Both bands are the characteristic and specific bands for O–H group representing stretching and bending vibration respectively for surface-adsorbed hydroxyl groups in water (Suriyavathana et al., 2015). The absorption peak with a wavenumber of 2886.00 cm^{– 1} signifying the existence –C-H stretching mode (Konios et al., 2014). Besides, the transmission peaks 765.00 cm^-1 and 528.00 cm^-1 represent the stretching vibration of Mn-O bonds, and characteristic stretching of O–Mn–O.

Table 3. Summary of bond types and wavenumber in TiO₂, RGO and MnO_2.

Figure 4. (a)FTIR spectrum of TiO₂ nanoparticles (b)FTIR spectrum of RGO nanoparticles(a)FTIRspectrum of MnO₂ nanoparticles.

4.2.2. XRD Characterization of TiO₂, RGO and MnO₂ Nanoparticles

Figure 5a shows the TiO₂ film XRD patterns. The presence of a sharp peak which corresponds to plane(110) at 2θ = 27.59˚ referring to the rutile phase having tetragonal structure. The diffraction peaks for planes (001), (201), (101), (110), (101), (111) and (211) at 2θ=7.60˚, 2θ=14.89˚, 2θ=29.75˚, 2θ=27.50˚, 2θ=37.10˚, 2θ=42.50˚ and 2θ= 54.60˚ reflect the tetragonal structure of TiO₂ nanoparticles. As seen in Table 4, the average crystallite size of 59.78 nm, lattice strain of 0.032 % and dislocation density of 0.00030 nm^-2 were also calculated. The diffraction patterns for MnO₂ are given in Figure 5b. The presence of diffraction peaks for planes (110), (200), (310), (311) and (410) at 2θ=18.27˚, 2θ=24.80˚ and 2θ=28.75˚, 2θ=42.50˚ and 51.20˚ reveal the alpha phase having pattern of tetragonal structure conformity with (JCPDS Card No.44-0141) having the lattice constants of (a = b = 9.78475 Å, c = 2.86302 Å) and (α = β = γ = 90˚). As seen in Table 5, the average crystallite size of 53.87 nm, lattice strain of 0.040 % and dislocation density of 0.00039 nm^-2 were also calculated. The XRD pattern of the synthesized RGO as shown in Figure 6 demonstrated peaks at 2θ=22.10˚ and 2θ =28.20˚ which is the characteristics of carbonaceous material. The most prominent peak located at 2θ=22.10˚ and other strong diffraction peak at 2θ=22.10˚ correspond to (002) and (200) basal planes respectively. Additionally, the d-spacing of film decreases as the diffraction tends towards larger angle with average d-spacing value of ~ 4.095 Å compared to ~ 7.37 Å obtained for graphene oxide by Mohamed et al, 2015.

Table 4. Structural parameters of TiO₂ film.

Table 5. Structural parameters of RGO film.

Table 6. Structural parameters of MnO₂ film.

Figure 5. (a) XRD pattern of TiO₂ nanoparticles (b) XRD pattern of RGO nanoparticles (c) XRD pattern of MnO₂ nanoparticles.

Figure 6. (a) SEM image of TiO₂ nanoparticles (b) SEM image of RGO nanoparticles (c) SEM image of MnO₂ nanoparticles.

4.2.3. SEM Characterization of TiO₂, RGO and MnO₂ Nanoparticles

The SEM image of TiO₂ in Figure 6a demonstrated properly-aligned structures of oval shapes constructed by nearly homogenous grains. Additionally, the surface was smooth and presents the crystalline nature of the produced film. SEM image of RGO is shown in Figure 6b. The morphology of multilayer RGOs revealed rough surface, flake-like shape, not crumpled and corrugated together with non-uniform of particle size. High film coverage was also observed. The aggregation or coalescence of flakes were large and ubiquitous. The agglomeration of the flakes was owing to catalytic oxidation of graphite by surphuric acid (Bhatti et al., 2016). As seen in Figure 6c, the morphology study results of MnO₂ nanoparticle film exhibit high-quality nanocomposites having different micrometers average length. The particle size was elongated and nearly spherical.

3.3.1. Optical Characterization of ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr and ITO/RGO/ TiO₂/CH₃NH₃PbI₃/Gr- MnO₂ Films

Figure 7a shows the UV-vis absorption spectra of the ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr and ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ films. the modification showed increases the intensity of absorption (hyperchromic effect) due to the increase in the number of delocalized electrons leading to a quasi-fermi level. This high absorbance intensity is attributed to the presence of simple un-conjugated chromophore with lone pair electrons in the MnO₂ and ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr. As a result, there was a high energy transition from an occupied molecular orbital (a non-bonding 𝜋 orbital) to an unoccupied molecular orbital (σ* orbital) of greater potential energy. i.e., 𝜋→σ* (Subodh, 2006). The (αhv)²-Eg plots of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr and ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ film is shown in Figure 7b. The band gap of fabricated ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr solar cell was extrapolated to be 1.75 eV, and that of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ reduced to 1.66 eV.

Figure 7. (a) Absorbance-wavelength plots of ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr and ITO/RGO/ TiO₂/CH₃NH₃PbI₃/Gr- MnO₂ films (b) (αhv)²-Eg plots of ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr and ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr- MnO₂ films.

4.3.2. FTIR Characterization of ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr and ITO/RGO/ TiO₂/CH₃NH₃PbI₃/Gr- MnO₂ Films

FTIR analysis was carried out to investigate the interaction between MnO₂ and ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr and results shown in Figure 8. In the fingerprint region of MnO₂ FTIR spectrum, two absorption peaks 528.00 cm^-1 and 765.00 cm^-1 which could be assigned to Mn-O-Mn and Mn-O. These two peaks present in ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr FTIR spectrum which confirmed incorporation of MnO₂ within the ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr specie. The peaks of Mn-O-Mn and Mn-O were located at 528.00 cm^-1 and 765.00 cm^-1 in MnO₂ film, while these peaks red shift to 556.00 cm^-1 and 825.00 cm^-1. Besides, the asymmetric

{N H}_{3}^{+}

bend, symmetric

{N H}_{3}^{+}

bend and CH₃

{N H}_{3}^{+}

stretch located at 2886.00 cm^-1, 1445.00 cm^-1 and 976.00 cm^-1 in ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr film blue shift to 2880.00 cm^-1, 1442.00 cm^-1 and 975.00 cm^-1. The blue shift of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr film peak and red shift of MnO₂ peak confirmed that there was strong coordination interaction between the functional groups of MnO₂ and Pb defects of the grain boundaries and interfaces of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr film.

Table 7. Summary of bond types and wavenumber in MnO₂, ITO/RGO/TiO₂/MAPbI₃/Gr and ITO/RGO/TiO₂/MAPbI₃/Gr.

Figure 8. FTIR spectrum of MnO₂, ITO/RGO/TiO₂/MAPbI₃/Gr and ITO/RGO/TiO₂/MAPbI₃/Gr.

3.3.3. XRD Characterization of ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr and ITO/RGO/ TiO₂/CH₃NH₃PbI₃/Gr- MnO₂ Films

In order to investigate the effect of MnO₂ on the crystallinity of ITO/RGO/TiO₂/CH₃NH₃PbI₃Br/Gr film. XRD measurements were performed and the results are shown in Figure 9. Five XRD peaks at 2θ= 19.20^o, 27.90^o, 29.80^o, 38.90^o and 59.20^o were observed in the two perovskite films which correspond to (101), (111), (210), (200) and (310) crystal plane of cubic phase CH₃NH₃PbI₃halide perovskite. The XRD results confirmed that MnO₂ has no remarkable influence on the crystal phase of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr film by the addition of MnO₂ (Xu et al., 2018). The intensities of 19.20^o, 27.90^o, 38.90^o and 59.20^o XRD peaks of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ film were higher than those of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr film, and the narrowed widths of these diffraction angles indicating that MnO₂ incorporation enhanced the crystallinity of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr film consistent with reports of other additives used in perovskites (Chavan et al., 2020).

Table 8. Summary of structural parameter MnO₂, ITO/RGO/TiO₂/MAPbI₃/Gr and ITO/RGO/TiO₂/MAPbI₃/Gr.

Figure 9. XRD patterns of ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr and ITO/RGO/ TiO₂/CH₃NH₃PbI₃/Gr- MnO₂ films.

4.3.4. SEM Characterization of ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr and ITO/RGO/ TiO₂/CH₃NH₃PbI₃/Gr- MnO₂ Films

The reference film without MnO₂ showed high film coverage, uniform morphology with apparent grain boundaries (Figure 9a) typical of perovskite films synthesized using the solution processed in one step method (Yang et al., 2019, He et al., 2020, Chiang et al., 2017). There was an evidence of compositional uniformity, and thus the grain boundaries were ubiquitous. No cracks were observed throughout the films (Figure 10a).Interesting, ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr film modified with MnO₂ exhibited a more uniform and compact structure compared to the reference film (Figure 9b). As seen in Figure 9b, there was evidence of more smooth surface which confirmed crystallinity enhancement. The average grain size(s) calculated for ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr and ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ films were ̴ 620 nm and ̴ 696 nm using intercept technique. This result confirms the morphology improvement of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr modified with MnO₂.

Figure 10. SEM images of ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr and ITO/RGO/ TiO₂/CH₃NH₃PbI₃/Gr- MnO₂ films.

4.3.5. Photovoltaic Performance of ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr and ITO/RGO/ TiO₂/CH₃NH₃PbI₃/Gr- MnO₂ Films

The photovoltaic performance parameters (such as Jsc, Voc, FF, and PCE) are shown in the Figure 11 As seen in Table 9, the incorporation of MnO₂ into the second device produced an increased in the value of Jsc from 16.25 mAcm^-2 to 19.00 mAcm^-2. This is due to the improved charge extraction and transfer ability induced in the second device by modification with MnO₂.nanoparticles. FF also increased from 47.48 % to 51.53 %. This indicates that the incorporation of MnO₂ enhanced the grain size of the perovskite absorber and the crystallinity of the absorber at the interface between the absorber and the ETL. As the grain size increases, the grain boundary reduces, thereby eliminating the charge trapping regions within the perovskite structure. However, the variation in the values of Voc in both devices could be as a result of hysteresis effect (Ihly et al, 2016). From the obtained photovoltaic parameters, the PCE increased from 8.64% to 10.79% with an enhancement value of 21.79%. This is due to tailored functionality of MnO₂ in the generation of functional group that act as conducting bridge in reducing the contact resistance between individual nanoparticle.

Table 9. Summary of Photovoltaic parameter of ITO/RGO/TiO₂/MAPbI₃/Gr and ITO/RGO/TiO₂/MAPbI₃/Gr.

Figure 11. J-V curves of ITO/RGO/ TiO₂/CH ₃NH₃PbI₃/Gr and ITO/RGO/ TiO₂/CH₃NH₃PbI₃/Gr- MnO₂ films

4. Conclusion

In this work, ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr and ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ were fabricated on ITO glass slide using solution process-based spin coating method, and their properties were studied. The bandgaps of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ compared to ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr decreased from 1.75 to 1.65 eV. Besides, the XRD patterns showed variation in the intensity of diffraction angles. The average crystallite size and d-spacing of 657.37 nm and 5.797Å were calculated for ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ compared to 576.05 nm and 5.956 Å calculated for ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr film. J-V curves of ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr and ITO/RGO/TiO₂/CH₃NH₃PbI₃/Gr-MnO₂ showed that the PCE increased from 8.64% to 10.79%. The Jsc and FF also increased from 16.25 Acm^-2-19.00 Acm^-2 and 47.48%-51.53% respectively. The enhancement value of 21.79% was achieved with MnO₂ passivation.

Acknowledgments

The authors profoundly acknowledge technical supports of the Material Science and Engineering Laboratory, KWASU, Molete and Industrial Laboratory, Pure and Applied Chemistry Department, LAUTECH, Ogbomoso.

Conflicts of Interest

The authors declare no conflicts of interest.

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Manganese Dioxide (MnO2) Nanoparticles Passivated Perovskite Solar Cell for Improved Power Conversion Efficiency

Abstract

1. Introduction

2. Theoretical Consideration

3. Materials and Methods

3.1. Materials

3.2. Experimental Method

3.2.1. Synthesis of Methyl Ammonium Lead Triiodide (CH3NH3PbI3)

3.2.2. Synthesis of Titanium Dioxide (TiO2)Nanoparticles

3.2.3. Synthesis of RGO Nanoparticles

3.2.4. Synthesis of MnO2 Nanoparticles

3.2.5. Glass/ITO/RGO/TiO2/CH3NH3I3/Graphite- MnO2 Device Fabrication

3.2.6. Glass/ITO/RGO/TiO2/CH3NH3I3/Graphite Device Fabrication

3.3. Characterization of the Films

4. Results

4.1.1. Optical Characterization of CH3NH3PbI3

4.1.2. FTIR Characterization of CH3NH3PbI3 Film

4.1.3. XRD Characterization of CH3NH3PbI3 Halide Perovskite Film

4.1.4. SEM Analysis of CH3NH3PbI3 Film

4.2.1. FTIR Characterization of TiO2, RGO and MnO2 Nanoparticles

4.2.2. XRD Characterization of TiO2, RGO and MnO2 Nanoparticles

4.2.3. SEM Characterization of TiO2, RGO and MnO2 Nanoparticles

3.3.1. Optical Characterization of ITO/RGO/ TiO2/CH 3NH3PbI3/Gr and ITO/RGO/ TiO2/CH3NH3PbI3/Gr- MnO2 Films

4.3.2. FTIR Characterization of ITO/RGO/ TiO2/CH 3NH3PbI3/Gr and ITO/RGO/ TiO2/CH3NH3PbI3/Gr- MnO2 Films

3.3.3. XRD Characterization of ITO/RGO/ TiO2/CH 3NH3PbI3/Gr and ITO/RGO/ TiO2/CH3NH3PbI3/Gr- MnO2 Films

4.3.4. SEM Characterization of ITO/RGO/ TiO2/CH 3NH3PbI3/Gr and ITO/RGO/ TiO2/CH3NH3PbI3/Gr- MnO2 Films

4.3.5. Photovoltaic Performance of ITO/RGO/ TiO2/CH 3NH3PbI3/Gr and ITO/RGO/ TiO2/CH3NH3PbI3/Gr- MnO2 Films