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Article

Enhancement of Perovskite Photodetector Using MAPbI3 with Formamidinium Bromide

by
Dong Jae Shin
and
Hyung Wook Choi
*
Department of Electrical Engineering, Gachon University, Seongnam 13120, Republic of Korea
*
Author to whom correspondence should be addressed.
Energies 2024, 17(9), 2183; https://doi.org/10.3390/en17092183
Submission received: 28 March 2024 / Revised: 22 April 2024 / Accepted: 29 April 2024 / Published: 2 May 2024
(This article belongs to the Section D1: Advanced Energy Materials)
Browse Figures
Versions Notes

Abstract

:
In this study, a perovskite-based mixed cation/anion ultraviolet photodetector with an added halide material is fabricated using perovskite combined with an ABX_3 structure. Mixed cation/anion perovskite thin films of MAPbI3/FABr are manufactured through a relatively simple solution process and employed as light-absorption layers. In the produced thin film, SnO2–sodium dodecylbenzenesulfonate acts as an electron transport layer and spiro-OMeTAD acts as a hole injection layer. Compared to a single cation/anion perovskite, the fabricated device exhibits phase stability and optoelectronic properties, and demonstrates a responsivity of 72.2 mA/W and a detectability of 4.67 × 1013 Jones. In addition, the films show an external quantum efficiency of 56%. This suggests that mixed cation/anion films can replace single cation/anion perovskite films. Thus, photodetectors based on lead halides that can be applied in various fields have recently been manufactured.

1. Introduction

In recent years, ultraviolet (UV) photodetectors have received considerable attention from researchers owing to their use in various fields such as covert communication, photo detecting, environmental analysis, astronomy, and medicine [1,2,3]. Generally, UV rays are divided into three areas according to wavelength range: UVA (~400–320 nm), UVB (~320–280 nm), and UVC (~280–100 nm) [1]. Most UVC rays are absorbed by the ozone layer and atmosphere and have no effect on Earth [4]. However, some UVC rays are radiated from technical light sources, like UV germicidal bulbs and mercury lamps [5]. UVC is harmful to human cells and can cause erythema and blindness [6,7]. Therefore, research on photodetectors that can detect UVC regions by converting incident optical signals into electrical signals is required.
Several types of inorganic materials such as Ga2O3, GaN, ZnGa2O4, and MoS2/Si have been used for UV detection. However, processes that use inorganic semiconductor materials require sophisticated processing at high temperatures [8,9,10]. By contrast, the application of low-temperature solution processing using perovskite materials is increasing compared to that of other semiconductors [11,12,13,14].
At present, perovskites are considered as good materials for fabricating photodetectors owing to their ease of manufacturing and low operating voltage [15]. Additionally, hybrid organic–inorganic perovskites demonstrate advantages such as a large optical absorption coefficient, high carrier mobility, controlled band gap, and long diffusion length; consequently, the reported photodetectors based on halide perovskites can function in wide detection regions with a fast response speed [16].
Early research on optical devices using perovskites used methylammonium lead iodide (CH3NH3PbI3, MAPbI3), which was prepared using only MA+ monovalent A cations as the light absorber. However, problems such as photostability and thermal stability occur because of the low crystallization energy and phase transition between the tetragonal and cubic phases at ~320 K [17,18,19]. Therefore, the focus of research has shifted to engineering optimal perovskite configurations [20]. In this regard, formamidinium lead iodide (CH(NH2)2PbI3, FAPbI3) has been studied, owing to its higher decomposition temperature, longer diffusion length, excellent thermal stability, and narrow bandgap compared with MAPbI3 [21]. However, FAPbI3 has a trigonal structure (perovskite phase, black, and α-phase-FAPbI3) or a hexagonal structure (non-perovskite phase, yellow, and δ-phase-FAPbI3) depending on the synthesis temperature [22]. Because α-phase-FAPbI3 is stable at high temperatures (above 160 °C), it can change into the more stable δ-phase-FAPbI3 at room temperature [20]. This phase change degrades the performance of optical devices that use the fabricated perovskite film as a light-absorption layer. Therefore, to prevent this phase change and improve the performance of optical devices, research is being conducted to improve stability using a mixture of monovalent cations such as MA+, FA+, and CS+, or by adding halides such as Cl− and Br− [23,24].
In this study, mixed cation/anion perovskite films of MAPbI3/FABr were produced as light-absorption layers to enhance the performance of perovskite deep-UV photodetectors. A more stable perovskite photodetector can be produced by adding a halide material (Br−) to the anti-solvent. When Br− ions are added, the Pb–Br bond length is relatively short, which reduces the lattice constant and improves the photogeneration and carrier transport characteristics. Additionally, because the ionic radius of the Br atom is smaller than that of I and the electronegativity of Br (2.96) is higher than that of I (2.66), the electronic charge distribution around the Br atom is much stronger, which can address the phase transition problem. Moreover, by adding Br ions, the bonding density of the perovskite can be increased, which can improve the efficiency of the film. Consequently, the prepared perovskite-based photodetector showed a photocurrent generation of 108.3 µA and a reactivity of 72.2 mA/W when FABr 20 was added to MAPbI3. In addition, the photodetector exhibited a detection degree of 4.67 × 1013 Jones.

2. Materials and Methods

2.1. Reagents and Materials

All the materials and reagents were used without additional purification. Indium tin oxide (ITO) was coated on a quartz glass substrate (TMA, Seoul, Republic of Korea). A SnO2 colloidal solution (15 wt% in water; Alfa Aesar, Haveril, MA, USA) was prepared. Furthermore, Pb(II) iodide (PbI2; 99.999%), 1-butyl alcohol (99%,), sodium dodecylbenzenesulfonate (SDBS), acetonitrile (99.93%), ethyl alcohol (≥99.5%), dimethyl sulfoxide (DMSO; ≥99.9%), N,N-dimethylformamide (DMF; 99.8%), 2,2,7,7-tetrakis[N,N-di(4-methoxyphenyl)amino]-9,9-spirobifluorene (spiro-OMeTAD; 99%), 2-propanol (IPA; 75 wt%), bis(trifluoromethane)sulfonimide lithium salt (Li-TSFI; ≥99.0%), toluene (99.9%), and 4-tertbutylpyridine (98%) were all purchased from Sigma Aldrich, St. Louis, MO, USA. In addition, methylammonium iodide (MAI) and formamidanium bromide (FABr) were obtained from GreatCell SolarKorea, Seohyun, Republic of Korea.

2.2. Fabrication of MAPbI3-Based Perovskite Photodetector

The ITO-deposited quartz substrates (8 Wm/sq) were purified to remove organic matter. Then, the substrates were sequentially cleaned using an ultrasonic bath with a neutral detergent, IPA, acetone, and purified water for 15 min each. Subsequently, the films were dried with UV ozone to remove any foreign substances. After diluting 1.2 mL of the SnO2 colloidal solution with 5.2 mL of deionized water, 1 mg of SDBS was dissolved in the SnO2 solution to make a SnO2–SDBS mixed solution. To form the electron transport layer of the film, the SnO2–SDBS mixed solution was spin-coated on an ITO substrate at 3000 rpm for 30 s and annealed at 150 °C for 30 min. The films were dried with UV ozone for 20 min to completely remove any moisture prior to the deposition of perovskite. The MAPbI3 perovskite precursor solution was prepared by mixing PbI2 (1.4 mol) and MAI (1.4 mol) in a mixture of DMF and DMSO (10:1, v/v). Next, IPA was stirred with FABr (0, 5, 10, 15, 20, and 25 mg) for 1 h to prepare the solution for FABr post-processing. The MAPbI3 perovskite layer was spin-coated onto the SnO2–SDBS layer at 4000 rpm for 25 s. Subsequently, 250 μL of toluene was added dropwise 15 s before the end of the spin-coating to form an anti-solvent. The prepared post-processing solution was then spin-coated onto the MAPbI3 layer at 4000 rpm for 25 s. The perovskite films were then annealed at 140 °C for 15 min on a hot plate. After cooling to room temperature, a spiro-OMeTAD solution [1 mL chlorobenzene containing 72.3 mg spiro-OMeTAD, 28.8 μL 4-tert-butyl pyridine, and 17.5 μL Li-TFSI solution (ACN in 1 mL of 520 mg Li-TSFI)] was coated onto the perovskite layer at 2000 rpm for 35 s. Finally, Au was thermally evaporated through an electrode using an e-beam evaporator in a high vacuum (2 × 106 Torr). Figure 1a shows the vertical structure of the fabricated photodetector and Figure 1b shows the preparation method.

2.3. Device Characterization

To investigate the crystal structure of the fabricated film, XRD (SmartLab, Rigaku, Tokyo, Japan) analysis was performed using Cu Kα radiation (λ = 1.542 Å). Field-emission SEM (Hitachi, S-4700, Tokyo, Japan) was used to analyze the surface and cross-sectional morphologies of the perovskite layers. The light absorptivity of the device was measured by UV-vis spectroscopy (UV-vis 8453, Agilent, Santa Clara, CA, USA). A combined source and measurement meter (Source Measure Unit, Keithley, 2400, Cleveland, OH, USA) was used to measure the electrical response of the perovskite photodetector. A UV lamp (6 W, 254 nm) (VL-6. LC, Vilber, VL6.LC, Seine-et-Marne, France) was used to provide 254 nm irradiation.

3. Results

Characteristics of the Prepared Perovskite Film

The perovskite films fabricated in this process are denoted as FABr 0, 5, 10, 15, 20, and 25, according to the amount of FABr added. Figure 2 shows the X-ray diffraction (XRD) patterns as a function of the amount of FABr added. The patterns indicate the crystal formation of the thin film after post-treatment with FABr. Figure 2a shows that the crystallinity of the films gradually enhanced as the FABr content increased. The reduced peak intensity in FABr 25 indicated that the high density of FABr caused grain shrinkage, which has a negative effect on film crystallization. The highest crystallinity was observed for FABr 20, and the intensity of the XRD peak was approximately 2.43 times that of the film without FABr. The growth of crystal grains owing to the addition of FABr leads to an increase in the extinction coefficient, which indicates the improved performance of the photodetector [25]. Figure 2b exhibits that with the addition of FABr, the main peak of MAPbI3 shifts from 14.2° to 14.0°, which matches the main peak of FAPbI3. This peak shift suggests the formation of an FAXMA1−XPbI3 perovskite thin film [26,27]. The lattice constant calculated by Bragg’s law is 3.14 Å at a diffraction angle of 14.2°, and increases to 3.184 Å at 14.0°, which suggests that adding br-ions to the produced film increases mobility, allowing better current flow. It can be seen that the crystal size calculated using the Debye–Scherrer equation increases from 36.37 nm for FABr 0 to 39.98 nm for FABr 20. As a result, the produced FAXMA1−X PbI3 film has high crystallinity. First, MAI and PbI2 were dissolved in DMSO and DMF and filtered using a syringe filter. Subsequently, the prepared precursor solution was spin-coated on the ITO substrate on which SnO2 was deposited. In the intermediate step, the film was concentrated by solvent evaporation, and the spatial steric hindrance of FABr and DMSO prevented the conversion of layered PbI2 into tetragonal perovskite. Subsequently, perovskite nucleation was accelerated through an anti-solvent process to crystallize the perovskite film with rapid solvent extraction. Finally, FABr was converted into the FAXMA1−XPbI3-DMSO phase via ion exchange. A highly crystalline perovskite film was formed through annealing [28].
Figure 3 shows the degree of surface formation of each fabricated perovskite film as observed using scanning electron microscopy (SEM). Figure 3a shows an SEM image of pure MAPbI3. It can be observed that the surface of FABr 0 has an irregular thin film. In addition, the particle sizes are relatively small. With the addition of the postprocessing solution, the size of the particles on the thin films also increased. In addition, the surface formation of the film improved, and a change in particle formation occurred. This implies improved photoelectric properties such as longer carrier life and better absorbance [29,30]. Figure 3e shows the most stable grain growth and uniform surface formation for FABr 20. However, Figure 3f shows that the grain size decreased and the number of pinholes increased in FABr 25. In addition, residues of PbI2 are observed. This can be attributed to the de-wetting phenomenon caused by the addition of excessive FA cations [31]. Excessive FABr content may affect the quality of the film by microcrystallizing the remaining fine pattern material. Thus, the crystal grains become smaller and gaps appear throughout the thin film, which ultimately has a negative effect on the performance of the perovskite films. Therefore, the addition of more FABr than is necessary prevents the proper formation of the perovskite and causes a decrease in the performance. Consequently, changes in the grain size and surface shape depending on the concentration of added FABr suggest that the added FABr has a significant impact on the microstructural changes in the perovskite [32].
The UV-visible absorption spectra in Figure 4a show the absorbance of the fabricated film. With an increase in the amount of FABr solution during the post-treatment process, the absorption spectrum showed a relative improvement. The films post-processed with FABr exhibited better optical properties than that of FABr 0. Furthermore, FABr 20 exhibited the highest absorbance, and the decrease in the absorbance of FABr-25 was affected by grain shrinkage owing to the excessive addition of FABr. In addition, adding an optimal amount of Br improved the binding density of the particles, which is expected to improve the characteristics of the film, as shown in the absorbance measurement results [33].
Optoelectronic properties such as the resistivity, mobility, and carrier concentration of perovskite films are important characteristics of photodetector materials [34]. The photoelectric properties of the films with different concentrations of FABr were analyzed through a Hall measurement system, and the results are shown in Figure 4b. The resistivity in FABr 0 is 0.7704 Ω∙cm, and the perovskite films with added FABr show resistivities of 0.2519, 0.2975, 0.2249, 0.2077, and 0.8474 Ω∙cm. The pure film (FABr 0) exhibits a mobility of 5.01 cm2/V∙s, whereas FABr 20 exhibits a mobility of 25.48 cm2/V∙s, which is the highest value obtained among the samples tested. The mobility is correlated with the Pb–Br structure. As the Pb–Br bond is relatively short, the lattice constant and distance between the atoms are reduced. Additionally, the electronegativity of the Br atom (2.96) is higher than that of I (2.66); therefore, heavy Pb hardly interacted with Br [35]. The decrease in the mobility of FABr 25 can be attributed to the excessive amount of FABr added. The higher the mobility, the greater the photocurrent generated [36]. The parameter values of Resistivity, Mobility, and Carrier Concentration are shown in Table 1.
The performance of the PD with respect to the amount of FABr added can be investigated by irradiating a 254 nm light with an output of 0.774 mW/cm2 in dark conditions and analyzing the current–voltage (I–V) correlation from −2 to +2 V. Figure 5 shows the amount of photocurrent generated as a function of the amount of FABr added. The generation of a photocurrent is affected by the intensity and bias voltage of the irradiated light. At a voltage of 2 V, the amounts of generated photocurrents were 31.8, 51.6, 70.1, 85.2, 108.3, and 75.3 μA, respectively. The smallest amount of photocurrent was generated in FABr 0, and as the amount of added FABr increased, the amount of generated photocurrent also increased; consequently, the largest amount of photocurrent was generated in FABr 20. This is because the added FABr increased the particle size and crystal grains, thereby increasing the extinction coefficient, as shown in the SEM image and absorbance results.
Figure 6a shows the responsivity (R) and detectability (D*) values of each thin film; R indicates the responsivity efficiency of the fabricated photodetector to the irradiated light. R is defined as the output photocurrent divided by the incident light power in the active area of the photodetector. It is determined by R = (Ilight − Idark)/APop (Ilight is the output current under 254 nm UV light, Idark is the dark current, A is the active area of the PD, and Pop is the incident light power intensity). As the amount of FABr increased, the R values increased to 21.1, 34.4, 46.7, 56.8, and 72.2 mA/W. However, for FABr 25, the R value decreased to 50.2 mA/W. Furthermore, D* is an important performance parameter indicating whether a PD region can be detected; D* is related to the R value and the noise of the device, and can be confirmed through these characteristics. It is defined as D* = (AΔf)1/2ΔR/in (A is the effective area of the PD, Δf is the electrical bandwidth, and in is the current noise). Generally, it is calculated as D* = R/2qJdark. In this equation, q is the amount of charge and Jdark is the dark current density. R and D* are proportional; as R increases, D* also increases. The D* value of the fabricated film increased to 1.74 × 1012, 4.98 × 1012, 2.38 × 1013, 2.89 × 1013, and 4.67 × 1013 Jones. However, in FABr 25, it decreased to 2.44 × 1013 Jones.
Figure 6b shows the external quantum efficiency (EQE) of the photodetector as a function of the amount of added FABr. The EQE is defined as the ratio of the number of photons emitted to the number of electrons injected, and shows the conversion degree of the PD; a high EQE indicates an excellent conversion efficiency of the photodetector. With an increase in the amount of added FABr, the EQE value at 2 V increased to 16, 27, 36, 44, and 56%; however, the EQE value decreased to 39% for FABr-25. This indicates that the mixed cation/anion perovskite film has better optoelectric properties than the single film. The R, D*, and EQE values of the produced films are shown in Table 2.
Figure 7a shows the time-dependent optical response of the photodetector observed at a bias voltage of 1 V and an output light intensity of 0.774 mW/cm2. When the physical value input to the photodetector changes over time, the output of the UV PD cannot fluctuate immediately and there is a delay depending on the response time. Response speed refers to how quickly a sensor’s output can fluctuate in response to input. This is one of the main parameters indicating the performance of the photodetector. The rise and fall times of the photodetector were measured to be 148 ms/164 ms, 164 s/171 ms, 224 ms/227 ms, 228 ms/231 ms, 227 ms/276 ms, and 228 ms/265 ms by increasing the amount of FABr added. This change occurs when numerous traps in the active layer briefly capture photocarriers before they are emitted, contributing to the circuit current and extending the fall time. Figure 7b shows the optical stability of the photodetector. Light stability can be checked by repeating ON/OFF 200 times at 3 s intervals. The optical current of 2.12 μA in the first iteration was 2.18 μA after 200 iterations. This section shows the improved stability of the photodetector.

4. Discussion and Conclusions

In summary, a mixed cation/anion perovskite UVC photodetector is manufactured by adding FABr to MAPbI3 perovskite. When a halide material (Br−) was added to the anti-solvent, a more stable perovskite photodetector was obtained. The fabricated thin film showed better photoelectric properties under a 254 nm deep-UV light source, and FABr 20 in particular showed the best photoelectric properties. This suggests that an optimal PD operation can be realized with the addition of an appropriate amount of FABr. Therefore, these findings are expected to be useful in various fields.

Author Contributions

Sample fabrication and original draft preparation: D.J.S.; Supervision and editing: H.W.C. All authors have read and agreed to the published version of the manuscript.

Funding

The Authors have received research support from the Ministry of Education and Gachon University Research Grant.

Data Availability Statement

Data is unavailable due to privacy.

Acknowledgments

This research was supported by the Basic Science Research Capacity Enhancement Project through the Korea Basic Science Institute (National Research Facilities and Equipment Center) grant funded by the Ministry of Education (2019R1A6C1010016), and by the 2023 Gachon University Research Grant (GCU-202300810001).

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. (a) Schematic diagram and (b) manufacturing process of MAPbI3-based deep-UV PD.
Figure 1. (a) Schematic diagram and (b) manufacturing process of MAPbI3-based deep-UV PD.
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Figure 2. XRD patterns of FAXMA1−XPbI3 films with different amounts of FABr added. (a) XRD patterns for different composition ratio and (b) expanded XRD patterns of the peaks from 13.0° to 15.0°.
Figure 2. XRD patterns of FAXMA1−XPbI3 films with different amounts of FABr added. (a) XRD patterns for different composition ratio and (b) expanded XRD patterns of the peaks from 13.0° to 15.0°.
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Figure 3. SEM images of FAXMA1−XPbI3 films: (a) FABr 0, (b) FABr 5, (c) FABr 10, (d) FABr 15, (e) FABr 20, and (f) FABr 25. (g) Cross-section of a device with individual layers shown in different colors.
Figure 3. SEM images of FAXMA1−XPbI3 films: (a) FABr 0, (b) FABr 5, (c) FABr 10, (d) FABr 15, (e) FABr 20, and (f) FABr 25. (g) Cross-section of a device with individual layers shown in different colors.
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Figure 4. Characteristics of perovskite films: (a) UV-vis absorption spectra and (b) photoelectric characteristics.
Figure 4. Characteristics of perovskite films: (a) UV-vis absorption spectra and (b) photoelectric characteristics.
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Figure 5. I–V curves of the UVC detector in a dark environment under 254 nm irradiation: (a) FABr 0, (b) FABr 5, (c) FABr 10, (d) FABr 15, (e) FABr 20, and (f) FABr 25.
Figure 5. I–V curves of the UVC detector in a dark environment under 254 nm irradiation: (a) FABr 0, (b) FABr 5, (c) FABr 10, (d) FABr 15, (e) FABr 20, and (f) FABr 25.
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Figure 6. (a) Calculated R as a function of voltage and D*; (b) EQE.
Figure 6. (a) Calculated R as a function of voltage and D*; (b) EQE.
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Figure 7. (a) Current-time characteristics of the photodetector according to the amount of FABr added; (b) photostability.
Figure 7. (a) Current-time characteristics of the photodetector according to the amount of FABr added; (b) photostability.
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Table 1. Parameters of resistivity, mobility, and carrier concentration for all films.
Table 1. Parameters of resistivity, mobility, and carrier concentration for all films.
SampleResistivity
(Ω∙cm)		Mobility
(cm2/V∙s)		Carrier Concentration
(cm−3)
FABr 00.77045.012.506 × 1013
FABr 50.251911.472.821 × 1013
FABr 100.297512.643.564 × 1013
FABr 150.224914.295.358 × 1013
FABr 200.207725.485.469 × 1013
FABr 250.847417.484.242 × 1013
Table 2. Performance parameters of PD according to the amount of FABr added.
Table 2. Performance parameters of PD according to the amount of FABr added.
SampleResponsivity
(mA/W)		Detectivity (Jones)EQE (%)
FABr 021.11.74 × 101216
FABr 534.44.98 × 101227
FABr 1046.72.38 × 101336
FABr 1556.82.89 × 101344
FABr 2072.24.67 × 101356
FABr 2550.22.44 × 101339
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Shin, D.J.; Choi, H.W. Enhancement of Perovskite Photodetector Using MAPbI3 with Formamidinium Bromide. Energies 2024, 17, 2183. https://doi.org/10.3390/en17092183

AMA Style

Shin DJ, Choi HW. Enhancement of Perovskite Photodetector Using MAPbI3 with Formamidinium Bromide. Energies. 2024; 17(9):2183. https://doi.org/10.3390/en17092183

Chicago/Turabian Style

Shin, Dong Jae, and Hyung Wook Choi. 2024. "Enhancement of Perovskite Photodetector Using MAPbI3 with Formamidinium Bromide" Energies 17, no. 9: 2183. https://doi.org/10.3390/en17092183

APA Style

Shin, D. J., & Choi, H. W. (2024). Enhancement of Perovskite Photodetector Using MAPbI3 with Formamidinium Bromide. Energies, 17(9), 2183. https://doi.org/10.3390/en17092183

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