Dayu
Huang
ab,
Ziyong
Cheng
ab,
Qiuyun
Ouyang
*a,
Hongzhou
Lian
*ab and
Jun
Lin
*ab
aKey Laboratory of In-Fiber Integrated Optics, Ministry Education of China, and College of Physics and Opotoelectronic Engineering, Harbin Engineering University, Harbin 150001, China. E-mail: qyouyang@hrbeu.edu.cn; hzlian@ciac.ac.cn; jlin@ciac.ac.cn
bState Key Laboratory of Rare Earth Resource Utilization, Changchun Institute of Applied Chemistry, Chinese Academy of Sciences, Changchun 130022, P. R. China
First published on 17th April 2023
The lattice defects that occur in material preparation processes are closely related to carrier migration. The carrier migration can be regulated by artificially modulating the defects to improve the luminescence performance, which is important for the development and application of luminescent materials. Here, we achieved a 3.29-fold increase in the high-temperature luminescence intensity by introducing Mn2+ to generate Cl vacancy defects in Cs2CdCl4. Due to thermally induced electron de-trapping, Cs2CdCl4:Mn2+ also displays anti-thermal quenching (ATQ) behavior and good thermal quenching resistance (329% at 175 °C). The increase in the photoionization effect and de-trapping of the captured electrons from shallow trap states were appropriately attributed to this exceptional phenomenon, based on thermoluminescence (TL) analysis. Based on comprehensive optical characterization, thermoluminescence and temperature-dependent X-ray diffraction (XRD), we reveal that the Cl vacancy trap state generated by Mn doping is the reason for the enhanced PL in air. The discovery of these materials helps to better understand the optical properties of all-inorganic perovskites.
In this work, we studied the relationship between radiative exciton recombination and carrier trapping on the surface of the Cs2CdCl4:Mn2+ perovskite crystal via high temperature spectra. It is found that the photoluminescence (PL) intensity of the Cs2CdCl4:Mn2+ crystal can be increased 3.29 fold by increasing the temperature from room temperature to 175 °C. Based on comprehensive steady-state and dynamic optical characterizations, we attribute the enhanced PL with increasing temperature to the reduced density of states associated with Cl vacancies near the crystal surface. We found that the carriers trapped by Cl vacancies are activated at high temperature, contributing to the PL intensity. Therefore, we speculate that the trap density of the Cs2CdCl4:Mn2+ crystal is more than that of the Cs2CdCl4 crystal. It is worth noting that high temperature is detrimental to the performance of perovskite LEDs. Our results provide a new means of improving the stability of devices based on all-inorganic perovskites, and highlight the interesting photoelectric properties of Cs2CdCl4:Mn2+ crystals due to high temperature.
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Fig. 1 (a) X-ray diffraction pattern of the Cs2CdCl4:Mn2+ perovskite crystal, showing the I4/m space group that coincides well with CCDC 2235089 (a = b = 5.2464 Å, c = 16.854 Å, α = β = γ = 90°). (b) Crystal structure of Cs2CdCl4. (c) XPS spectra corresponding to Cs2CdCl4, Cs, Cd, Mn, C and Cl. (d) EPR spectrum of Cs2CdCl4:Mn2+. |
Structural parameter | Cs2CdCl4:Mn2+ |
---|---|
a | 5.2464 Å |
b | 5.2464 Å |
c | 16.854 Å |
Volume | 463.9 Å3 |
Space group | I4/m |
Z | 4 |
h | 7 |
k | 7 |
l max | 23 |
R (reflections) | 0.0663 |
wR2 (reflections) | 0.1851 |
CCDC | 2235089 |
Fig. 2a displays the UV/Vis diffuse reflectance (DR) spectrum of Cs2CdCl4:Mn2+. Here, Cs2CdCl4:Mn2+ exhibits several absorption sites and an indirect bandgap (Fig. 2b). Indeed, under observation with the naked eye, Cs2CdCl4:Mn2+ exhibited yellow emission under UV irradiation, which is clearly brighter than that of pristine Cs2CdCl4. The host's own luminescence is very weak or even invisible to the naked eye (Fig. 2c). After Mn2+ doping, the Mn2+ d–d emission corresponding to the spin-forbidden 4T1 → 6A1 transition can be observed as a broadband yellow emission peak at around 585 nm with excitation at 417 nm (Fig. 2d). The emission bands of these samples share many solitary excitation bands at 250–325, 325–375, 417, and 475–550 nm, which perhaps belong to a charge transfer band and electronic transitions from 6A1g(S) to the excited state. The corresponding excitation spectrum is shown in Fig. 2d. The distinct transitions show different excitation peaks. The excitation peak at 250–325 nm belongs to the charge transfer band of the host. The excitation peak at 325–375 nm is attributed to the 4Eg(4D)/4T2g(4D)–6A1 transition. The 4E2g(4G)/4T2g(4G)/4A1(4G)–6A1 transition is responsible for the excitation peak at 417 nm. Moreover, the 4T1(4G)–6A1 transition is involved in the excitation peak at 475–550 nm.
Fig. 2e and f present photographs of the luminescence of the samples under visible light and ultraviolet light, respectively. The size and the yellow emission of the Cs2CdCl4:Mn2+ are clearly shown. In addition, grinding the single crystal into powder does not affect the luminescence intensity of the sample. The PLQY of the material can reach 90%.
In order to study the temperature dependence of the photoluminescence of the Cs2CdCl4:Mn2+ crystal, we monitored the crystal luminescence at high temperature. Fig. 3a shows the PL spectra of the Cs2CdCl4:Mn2+ crystal excited at 275 nm at different temperatures. Surprisingly, as shown in Fig. 3c, the PL intensity at high temperature increases by 3.29 fold (I(175°C) = 3.29I(25°C), where I(175°C) is the integrated intensity at 175 °C, and I(25°C) is the integrated intensity at 25 °C). As shown in Fig. 3a, the PL peak of the Cs2CdCl4:Mn2+ crystal shows a clear enhancement and a blue shift as the temperature is increased. The blue shift of the emission peak at high temperature is because the crystal field strength of the material becomes weaker, which is generally accepted (Fig. 3b). It can be seen that the PL intensity decreases slowly before −100 °C, and then begins to increase slowly. As the temperature continues to rise, between 75 and 175 °C, the luminescence intensity increases rapidly and reaches the strongest state. Such a heating process can be repeated many times without any signs of change (Fig. 3d).
In order to obtain the mechanism of the temperature-dependent PL, it is necessary to understand the reasons for the PL enhancement of the Cs2CdCl4:Mn2+ perovskite crystals at high temperature, which is crucial for further analysis. In general, two possible scenarios can be assumed to explain the higher PL intensity at temperatures higher than room temperature. (1) The PL origin is related to the non-intrinsic radiation defect state, and the defect concentration increases at high temperature. This has recently been reported, and energy transfer from the trap state to Mn2+ has been observed at high temperatures.47 (2) If the PL originates from intrinsic interband or exciton recombination, it is necessary to verify the reduction of non-radiative recombination centers at high temperature. However, the luminescence enhancement is clearly not due to the decrease of the radiation centers, but the increase in the energy transfer path to Mn2+ at high temperature. Since significant self-trapped exciton (STE) emission can be observed at low temperature, the whole temperature-rise process refers to multiple photophysical behaviors.
First, we observe the normal emission intensity of Cs2CdCl4:Mn2+ in the region from −180 to −100 °C (I−180°C to I−100°C) as shown Fig. 3c. This is initially used to return to the ground state radiation transition energy due to the phonon vibration loss, that is, thermal quenching behavior. Defect levels are not involved during this low-temperature process due to the lack of effective thermal activation energy. In region II (from −80 to 250 °C), the emission intensity at 175 °C is 329% of that at 20 °C. Nonetheless, Cs2CdCl4:Mn2+ exhibits the zero-thermal quenching phenomenon close to the working temperature of the LED chip, indicating its practical application potential. Generally, electron–phonon coupling becomes stronger and leads to the loss of luminescence intensity at high temperature. Hence, the thermal quenching and thermo-stimulated radiation dynamic process may form a competitive relationship to affect the luminescence intensity. Our initial hypothesis was that the STE energy of the host was transferred to Mn2+; however, since the STE luminescence is so faint, it is hard to double the luminescence of Mn2+.
Through XPS, we discovered an intriguing phenomenon in which the signal peaks of Cl in Cs2CdCl4 and Cl in Cs2CdCl4:Mn2+ moved and expanded significantly (Fig. 4a and b). The material itself has Cl− vacancy defects, and the introduction of Mn2+ can control the Cl− vacancy within a certain range, thereby maintaining stability at high temperature. Due to the high temperature, excessive Cl vacancy defects will lead to luminescence quenching. Therefore, the introduction of Mn avoids a large number of Cl vacancies at high temperatures and maintains a relatively balanced Cl vacancy ratio, which significantly enhances the anti-thermal quenching of Mn2+. This is because a large number of Cl defects will bring about a large number of non-radiative complexes. This is the reason why we observe the anti-thermal quenching effect at high temperature.
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Fig. 4 XPS spectrum of Cl in (a) Cs2CdCl4 and (b) Cs2CdCl4:Mn2+. (c) Temperature-dependent XRD patterns. (d) TG curve of Cs2CdCl4:Mn2+. |
To test the hypothesis proposed above, we obtained the following series of high temperature material characterization data. The material's luminous phase did not change at high temperatures, according to high temperature XRD (Fig. 4c). The TG curve proves that the quality of the sample does not change with the increase in temperature. The water adsorbed by the sample is lost (Fig. 4d). Subsequently, we examined the material's PLQY at different temperatures and discovered that, in addition to the PLQY of the material increasing at high temperatures, the absorption also increased, reaching a maximum before then declining (Table 2). The trend in the temperature-dependent quantum yield is similar to that of the temperature-dependent luminescence. The luminescence of the material is enhanced with the increase in temperature. It is further proved that the luminescence of the material is indeed enhanced at high temperature, which is very beneficial for practical applications of the material.
Temperature (°C) | Quantum yield | Absorption |
---|---|---|
25 | 0.90 | 0.36 |
40 | 0.91 | 0.37 |
55 | 0.92 | 0.38 |
70 | 0.92 | 0.385 |
85 | 0.92 | 0.389 |
100 | 0.93 | 0.391 |
115 | 0.94 | 0.393 |
130 | 0.94 | 0.396 |
145 | 0.94 | 0.398 |
160 | 0.95 | 0.41 |
175 | 0.95 | 0.412 |
190 | 0.94 | 0.43 |
205 | 0.94 | 0.40 |
220 | 0.94 | 0.402 |
In the information that follows, we demonstrate that the evidence points to the presence of several traps. Initially, a certain depth of lattice disorder is seen on the surface of the particles, probably as a result of the substitution of Mn2+ ions (Fig. 5a). Hence, the above finding indicated that the Cl vacancies, as electron trapping and storing sites, contributed to the enhanced emission intensity. To further support this view, the thermoluminescence (TL) glow curve, as a powerful tool to investigate the trapping state, was employed. Five trap levels were located between 300 and 600 K at various depths (Fig. 5b). E = Tm/500, where E is the average trap depth and Tm is the temperature corresponding to the peak position, is the empirical formula of Urbach.48 The computed trap depths are 0.68, 0.74, 0.86, 0.99 and 1.04 eV. Fig. 5c shows several processes of electron transfer. Some of the excited electrons transfer to the excited state of Mn2+ at room temperature, enhancing the Mn2+ emission. Deep traps catch some of them. In addition, the shallow trap's electron component contributes to the Mn2+ emission, which boosts the Mn2+ emission. Deep traps have all captured the remaining electrons. Deep trap electrons have a key role in the emission of Mn2+ at high temperatures. The abnormal luminescence phenomena are caused by the electrons of deep traps obtaining energy to jump out of the deep trap and transfer to the excited state of Mn2+. Such a host is unusual. A localized Cl vacancy trap energy level is created in the material's forbidden band through the addition of Mn2+. When the temperature increases, the electrons bound by the trap energy level are de-trapped, reaching the excited state energy level via the conduction band and undergoing electron–hole complexation when returning to the ground state. The energy is emitted in the form of yellow emission to compensate for the weakened luminescence caused by the non-radiative transitions at high temperatures. When the two processes reach dynamic equilibrium, zero-thermal quenching can be achieved. Confirmed by the Jahn–Teller effect, slight distortions lead to easier STE formation due to the enhanced electron–phonon coupling (Fig. 5a). Secondly, the doping of Mn2+ introduces a large number of defect energy states, which is a basis for the enhanced STE phenomenon compared with the host. The trap states of the Mn2+ materials were calculated via the thermoluminescence spectrum, taking into account the Cl vacancies in the lattice, to further demonstrate that defects are involved in the process of anti-thermal quenching. The energy supplement process: the light irradiation at room temperature/high temperature makes these suitable defect states capture the excited carriers. The carriers trapped by the defect state will be released to the luminescence center under the influence of thermal disturbance as the temperature increases, making up for the energy loss enforced by the thermal quenching effect and enhancing the thermal stability of the luminous material.
We further demonstrated the process of energy transfer from STE to Mn2+ by monitoring the decay time of different emission peaks at different temperatures (Fig. 5d). The conclusion that all data can be explained using a double exponential decay model, y = y0 + A1exp(−t/τ1) + A2
exp(−t/τ2), suggests that Cs2CdCl4:Mn2+ phosphors contain only a double light center (Table 3). By monitoring the excitation and emission spectra of Mn2+ at different temperatures, it is proved that energy transfer occurs between STE and Mn2+ at different temperatures (Fig. 5e). In addition, the decay time test further proves the energy transfer efficiency of Cs2CdCl4 and Mn2+. The lifetime of Mn2+ increases with increasing temperature, which is strongly related to the material's deep traps. Partly as a result of energy transfer, the host's lifetime keeps getting shorter.
T (°C) | Decay time (ms) | T (°C) | Decay time (ms) |
---|---|---|---|
−180 | 12.95 | 25 | 17.65 |
−160 | 12.58 | 50 | 19.56 |
−140 | 11.90 | 75 | 21.16 |
−120 | 11.78 | 100 | 23.25 |
−100 | 11.26 | 125 | 26.52 |
−80 | 13.36 | 150 | 28.61 |
−60 | 13.62 | 175 | 30.81 |
−40 | 13.89 | 200 | 16.62 |
−20 | 14.36 | 225 | 15.84 |
0 | 14.51 | 250 | 15.43 |
Footnote |
† CCDC 2235089. For crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d3tc00982c |
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