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. 2023 Feb 13;13(8):5428–5436. doi: 10.1039/d3ra00279a

Citric acid tuned negative thermal quenching of all inorganic copper-based perovskites†

Lu Yao a, Hong Meng a, Ming Liu a,✉
PMCID: PMC9923819  PMID: 36793305

Abstract

Copper-based perovskites, with lower electronic dimensions and high photoluminescence quantum yields (PLQY), which are non-toxic and thermally stable, have been reported since 2019 and have immediately attracted great attention. So far, only a few studies have researched the temperature-dependent photoluminescence properties, posing a challenge in ensuring the stability of the material. In this paper, the temperature-dependent photoluminescence properties have been investigated in detail, and a negative thermal quenching of all-inorganic CsCu2I3 perovskites has been studied. Moreover, the negative thermal quenching property can be tuned with the assistance of citric acid, which has not been reported before. The Huang–Rhys factors are calculated to be 46.32/38.31, which is higher than for many semiconductors and perovskites.

Citric acid increase induces structure and better crystallinity and more surface defects of copper-based perovskite, resulting in higher luminescence and more surface energy states, which leads to enhanced thermal stability.graphic file with name d3ra00279a-ga.jpg

1. Introduction

For luminescent materials, their photoluminescence (PL) intensity always decreases with an increase in temperature, which has been called thermal quenching.1,2 However, a negative thermal quenching phenomenon has been found in some special luminescent materials, first discovered in doped GaAs and ZnS semiconductors.3–6 This same phenomenon has then been found in pure ZnO material, GaInP, and carbon nanodots.7–11 The reason for the negative thermal quenching is mostly attributed to electrons at defect energy states, which couple with phonons and can be easily activated by thermal energy.3–11

Perovskites, which were discovered in 1839, have received great attention in recent years due to the emergence of halide perovskites.12–14 Significant developments have been made in light emitting, photodetector, and solar cell technologies concerning lead-halide perovskites.15–19 However, these devices are severely affected by lead toxicity and poor thermal and air stability.20–23 Copper-based perovskites, with lower electronic dimensions and high photoluminescence quantum yields (PLQY), which are non-toxic and thermally stable, were reported in 2019 and have received great attention immediately.24–28 For instance, the all-inorganic Cs3Cu2Br5−xIx, which possess a 0D electronic structure, showed improved stability compared to that of Pb- and Sn-based halides.29,30 CsCu2X3, which has a 1D electronic structure and multiple excitons, exhibits yellow light and has great potential for light emission.25,31 Especially for CsCu2I3, the single crystal of this material displays a high PLQY; the nanowire of it shows an intrinsic anisotropy due to its asymmetric structure and external morphology anisotropy, and exhibits polarization-sensitive photoconductive detection performance.31–33 These materials are not only thermally stable in terms of their phase and structure, but also thermally stable in terms of their photoluminescence property.32

Chelating agents, such as polyvinylpyrrolidone, oleic acid, ethylene diamine tetraacetic acid, and citric acid, have been widely used to control particle size and crystal growth orientation in nanocrystal synthesis. In many reports, it has been shown that adding a chelating agent can significantly alter the crystallization and morphology of the nanocrystal, as well as its luminescence properties.34–37 Herein, we report the negative thermal quenching phenomenon of the all-inorganic perovskite CsCu2I3, and we found that the negative thermal quenching property can be tuned by the chelating agent citric acid. In Roccanova et al.'s report, they also found a negative thermal quenching of CsCu2X3 structure, which they attributed to the “electron–phonon” coupling. However, in our experiment, we found the negative quenching not only attributed to electron–phonon coupling, but also highly related to the crystallinity and surface defects. To the best of our knowledge, this is the first report of chelating agents-tuned negative thermal quenching in perovskites, which provides a new strategy to enhance the luminescence and stability of perovskites.

2. Methods

2.1. Chemicals

All reagents were used without further purification, unless otherwise stated. Cesium iodide (CsI, Xi'an Polymer Light Technology Corp. 99.9%), copper iodide (CuI, Aladdin, 99.9%), dimethyl sulfoxide (DMSO, Alfa Aesar, 99.9%), dimethyl formamide (DMF, S-A, 99.9%), citric acid (Cit, energy chemical, 99%), olic acid (OA, energy chemical, 99%) and methyl alcohol (Aladdin, 99%) are the original reagents.

2.2. Preparation

Synthesis of CsCu2I3 films

CuI (12.5 × 10−4 mol, 0.1187 g) and CsI (6.25 × 10−4 mol, 0.2436 g) with different amounts of Cit (0 mmol, 1 mmol, 2 mmol) were dissolved in 2.5 ml of a DMF : DMSO mixture (4 : 1, typically 2 ml DMF and 0.5 ml DMSO) and stirred at 60 °C in a nitrogen atmosphere until completely dissolved. The solutions were then filtered with a 0.22 μm nylon66 syringe and spin-coated onto quartz glass substrates. Each layer was deposited at 4000 rpm for 30 s and preheated at 100 °C for 1 h.

Synthesis of CsCu2I3 powders with Cit assistance

The residual precursor from the synthesis of CsCu2I3 films was then transferred to certain mount anti-solvent (methyl alcohol), forming a white powder in the process. The products were collected, separated by centrifugation, and dried at 60 °C in an atmosphere.

Synthesis of CsCu2I3 powders with OA assistance

CuI (12.5 × 10−4 mol, 0.1187 g) and CsI (6.25 × 10−4 mol, 0.2436 g) and different amounts of oleic acid (OA) (0 μl, 200 μl, 400 μl, 800 μl) were dissolved in 2.5 ml of a DMF : DMSO mixture (4 : 1, typically 2 ml DMF and 0.5 ml DMSO) and stirred at 60 °C in a nitrogen atmosphere until complete dissolution. The solution was then transferred to 2.5 ml of an anti-solvent (methyl alcohol), forming a white powder in the process. The products were collected, separated by centrifugation, and dried at 60 °C in an atmosphere.

2.3. Characterization

The structural characterization of the CsCu2I3 films was carried out using an X-Ray Diffractometer (Bruker D8 Advance diffractometer with a Cu Kα (0.15418) X-ray source, operating at 80 KV and 40 mA). The measurements were taken from 2θ of 10° to 50°. The morphological characterization was conducted using a thermal field scanning electron microscope (ZeissSupra 55) operated at 5 kV and Atom force microscope (Bruker). Photoluminescence excitation and emission spectra were recorded with a photoluminescence spectrometer (HORIBA Fluorolog-3) equipped with a temperature control device. Absorption spectra were performed using a PerkinElmer lambda 950 spectrophotometer. Fourier transform infrared spectra were performed by a Fourier Transform Infrared Spectrometer (INVENIO-R).

3. Experiments and discussion

3.1. Structural and morphological studies

Structural characterization

To fully characterize the structure of the CsCu2I3 films, the X-ray diffraction (XRD) spectra of the three samples (Fig. 1(a)) were measured. For the samples with Cit amount of 0 mmol and 1 mmol, the phase are pure CsCu2I3 phase (PDF#45-0076) with a CmCm (63) space group. With further increasing the Cit amount to 2 mmol, the dynamic equilibrium of Cu+ and Cs+ in precursor might be changed, a few impure phase Cs3Cu2I5 (PDF#45-0077) with a Pbnm (62) space group can be observed, which are shown by a star symbol. As the amount of Cit increased, the XRD intensity become higher, implying a higher degree of crystallinity or a larger grain size. However, larger grain sizes can not be observed from the scanning electron microscopy (SEM) images (Fig. 1(b–d)). With Cit 0 mmol, a grain size of about 74 nm is obtained, and with Cit 1 mmol, it is hard to seen the grain boundary. The same results can also be obtained from AFM images (Fig S5†). Usually, Cit introduction leads to the orientation growth of crystals, but it is hard to identify the orientation growth from the films. Therefore, the micro-crystals have been synthesized by an anti-solvent method. The SEM images are shown in Fig. 2, and an obvious orientation growth can be observed with Cit added to the precursor. When there is no Cit in the precursor, the micro-crystals are 15 μm and there are lots of irregularly shaped powders. With Cit added to the precursor, the micro-crystals are 53 μm and the irregularly shaped powders has disappeared. From the analysis above, it can be concluded that the reason for the increasing XRD intensity might be due to better crystallinity and the orientation growth of the crystal.

Fig. 1. (a) X-Ray diffraction patterns, and SEM images of the CsCu2I3 films with different Cit amounts (b) 0 mmol, (c) 1 mmol (d) 2 mmol.

Fig. 1

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Fig. 2. SEM images of the CsCu2I3 micro-crystals with different Cit amounts (a) 0 mmol, (b) 1 mmol. (c) Schematic orientation growth of the CsCu2I3 micro-crystals with assistance of Cit.

Fig. 2

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3.2. Optical characterization

The absorption spectra of two samples with no Cit and 1 mmol Cit were measured and showed similar absorption performances, with a deep UV absorption less than 330 nm wavelength. The PL excitation spectrum (measuring emission at 550 nm) has two peaks at 314 nm (3.95 eV) and 323 nm (3.83 eV), with a peak spacing of 0.12 eV, which is close to the spin orbit splitting of copper d electrons. Previous reports have calculated the valence band (VB) and conduction band (CB) of CsCu2I3, with the results showing that the VB is mainly composed of Cu 3d orbitals and the CB derived from Cu 4 s orbitals. A VB splitting of 0.18 eV has also been reported before,25 which is consistent with our results. The optical band gap (Eg) of CsCu2I3 thin films was calculated by the classical Tauc formula.38αhv = A(hv − Eg)1/2where A, h, ν, Eg, and α are constants, the Planck constant, light frequency, optical band gap, and absorption coefficient, respectively. The (αhν)2versus hν plots of CsCu2I3 films with different Cit amounts are shown in Fig. 3(b). The Eg can be obtained from the tangent line of the plots of Fig. 3(b). The Eg of CsCu2I3 films with no Cit and 1 mmol Cit are 3.7 eV, consistent with the previous reports of 3.93 eV, which have been calculated by hybrid PBE0 DFT calculations.25,31 When the Cit amount increases to 2 mmol, the band gap is 3.43 eV, which shows a decrease due to the disturbance of the impure phase.

Fig. 3. (a) UV-visible absorption spectra (b) and the (αhν)2versus hν plots of CsCu2I3 films with different Cit amount.

Fig. 3

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The PL spectra of CsCu2I3 films with different amounts of Cit were measured. All of the three samples shows a broad emission between 400 nm to 800 nm with an incident light of 325 nm. The broad emission peak indicates that the electrons at the self-trapped states are coupling with the phonons.

The lifetime of the samples can be described by the equation:393.2.

∑AR is the radiative transition rate of the samples, ∑AnR is the nonradiative transition rate of the samples. Fig. 4(b) shows the time-resolved PL of the as-prepared samples, from which the decay profile can be obtained by fitting with a two-exponential function. The sample with Cit 1 mmol shows the longest lifetime, which is 79 ns. The lifetimes of the samples with Cit 0 mmol and Cit 2 mmol are 67 ns and 60 ns, respectively. It is worth noting that with the addition of Cit to the precursor, the emission intensity has increased, indicating an increase in the radiative rate ∑AR. However, the lifetime has increased, implying a decrease of narrative rate ∑AnR. Therefore, we can conclude that the nonradiative rate has been efficiently suppressed due to the increasing crystallinity of the films, which has reduced localized disordered defects and limited the internal nonradiative pathway. However, with the Cit add into the precursor, there is as increase concentration of surface defects, which can be identified from the FTIR spectra (Fig. S7†). Even though the surface defects have increased, which would cause an increase of ∑AnR, the combination of these two effects has ultimately caused a decrease of ∑AnR and an the increase of PL lifetime. With increasing Cit amount to 2 mmol, the lifetime shows a decrease, which may be attributed to the increased nonradiative rate of the impure phase Cs3Cu2I5. The lifetime of the impure phase Cs3Cu2I5 has also been measured, which is about 383 ns (Fig. S8†).

Fig. 4. (a) Photo luminescence (PL) spectra and (b) time resolved photo luminescence decay curves of CsCu2I3 films with different Cit amount (excited at 325 nm, emission at 550 nm).

Fig. 4

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3.3. Temperature-dependents upconversion luminescence properties

The intensity of all CsCu2I3 samples first increases with temperature and then decreases at higher temperatures (Fig. 5(a and b)). For the CsCu2I3 sample with Cit 0 mmol, the highest PL integrated intensity is obtained at 200 K; for the CsCu2I3 sample with Cit 1 mmol, the highest PL integrated intensity is obtained at 250 K. From the structural and morphology analysis, it can be observed that the samples with Cit 1 mmol have better crystallinity and more surface defects. Better crystallinity implies fewer defects in the crystal lattice. Usually, the PL integrated intensity decreases with temperature, which is called “positive thermal quenching”. In this experiment, the PL integrated intensity first increases with temperature, and then quenches with temperature, which is called “negative thermal quenching”. This phenomenon has been observed in some semiconductors and metal halides, which is attributed to the detrapping of electrons in defect states with increasing temperature.

Fig. 5. (a and b) Temperature-dependent PL spectra of CsCu2I3 under 325 nm excitation. Thermal evolution of (c) integrated intensity, (d) peak position, (e and f) peak separation of PL peaks of CsCu2I3 with different Cit concentration.

Fig. 5

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The negative thermal quenching mechanism is illustrated by Fig. 6. The PL process can be described by the following path. First, the electrons at the valence band are activated to become hot-free electrons, and then the hot-free electrons turn into cooling-free electrons by carrier optical-phonon scattering. The cooling-free excitons then overcome the trap barrier by carrier acoustic phonon scattering and turn into self-trapped excitons. The self-trapped excitons couple with phonons by phonon scattering and phonon absorption, which form a broad emission band. Finally, the self-trapped excitons relax by nonradiative and radiative pathways. The nonradiative recombination is derived from the electrons at the defect energy state. The radiative recombination comes from the self-trapped excitons returning to the ground state directly. In the process, there are two different ways that account for the negative thermal quenching. First, the electrons at the surface defect energy state might be activated to the conduction band by increasing temperature. Second, the electrons at other defect energy states might be thermally activated to the self-trapped energy state.

Fig. 6. Configurational coordinate diagram illustrating the origin of negative thermal quenching of as-prepared CsCu2I3 films.

Fig. 6

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The change in negative thermal quenching with different Cit amounts suggests that the negative thermal quenching of CsCu2I3 is mainly due to surface defects that have been thermally activated to the luminescence energy. To verify this conclusion, we synthesized micro-crystals by anti-solvent precipitation with the chelate agent OA. Due to the large size of the powder crystal, the surface-to-volume ratio becomes small, which will lead to low surface defect concentration, the temperature of the strongest luminescence intensity is lower than that of the CsCu2I3 films, which is around 150 K (Fig. S3†).

It also can be observed in Fig. 5(d–f) that there is a blue shift of the emission peak. It has been reported by Du’s research that there is three self-trapped excitons in CsCu2I3 system. Two of them are at about 2.5–2.6 eV (blue emission). The other one at about 2.8 eV (green emission). Therefore, with the increasing temperature, there might be more electrons in defect energy detrapped to the self-trapped energy state with blue emission (Fig. 7).

Fig. 7. (a and b) FWHM of CsCu2I3 with different Cit concentration.

Fig. 7

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The full width at half maximum (FWHM) are enlarged with increasing temperature, which implies electrons distributed to more self-trapped energy states as well, which is consistent with the blue shift results. In principle, the Huang–Rhys factor (S) reflects how strongly electrons couple to phonons, which can be obtained by fitting the temperature-dependent full-width at half-maxima (FWHM) of emission peaks using the equation as following;3.3.where hωphonon is the phonon frequency. For CsCu2I3 with no Cit, S and hωphonon are calculated as 46.32 and 13.07 meV, respectively, For CsCu2I3 with Cit 1 mmol, S and hωphonon are calculated as 38.31 and 18.29 meV, respectively. The Huang–Rhys factor is larger than that of conventional emitters like CdSe, ZnSe and CsPbBr3 perovskites, indicating the easy formation of STEs in CsCu2I3. However, the Huang–Rhys factor of CsCu2I3 are lower than many other perovskites, such as Cs3Sb2I9, Cs3Bi2I9 and Rb3Sb2I9. It is comparable to a reported high quantum efficiency perovskite Cs2AgInCl6, of which the Huang–Rhys factor is 38.7, which means the photoluminescence performance of CsCu2I3 also can be good. But unfortunately the emission peak (400–700 nm) is at the dual frequency peak of the excitation peak (328 nm), it hard to measure the QE of CsCu2I3 films (Table 1).

Huang–Rhys factors of different compounds.

Compounds Huang–Rhys factor Ref.
CdSe 1 40
ZnSe 0.3 41
CsPbBr3 3.2 42
Cs2AgInCl6 38.7 43
CsCu2I3 46.32/38.31 This work
Cs3Bi2I9 79.5 44
Rb3Sb2I9 50.4 44
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4. Conclusion

Cit tuned negative thermal quenching photoluminescence performance has been found in the CsCu2I3, which has been derived from the increase of surface defect concentration. This enhanced negative thermal quenching performance improves the luminescence stability of CsCu2I3. This strategy provides a potential method to improve the luminescence stability of perovskites. The Huang–Rhys factor of CsCu2I3 films is higher than conventional emitters but lower than many perovskites, which is an appropriate value and implies that the CsCu2I3 films have good luminescence properties and potential applications in lighting and scintillator.

Conflicts of interest

There are no conflicts to declare.

Supplementary Material

RA-013-D3RA00279A-s001

Acknowledgments

This work was supported by Key-Area Research and Development Program of Guangdong Province (No. 2020B010178001), Shenzhen Hong Kong Innovation Circle Joint R&D Project (SGDX20190918105201704), Shenzhen Fundamental Research Program (No. GXWD20201231165807007-20200810113811001).

†

Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d3ra00279a

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