Regulation of afterglow and self-trapped exciton emission in indium-based organic metal halides via metal ion doping for multilevel anti-counterfeiting

Hongbo Qia, Jing Lia, Hailong Yua, Jing Zhanga, Chen Chena, Qiuju Hanb and Wenzhi Wu*a
aSchool of Electronic Engineering, Heilongjiang University, Harbin, Heilongjiang 150080, China. E-mail: wuwenzhi@hlju.edu.cn
bSchool of Arts and Sciences, Northeast Agricultural University, Harbin, Heilongjiang 150030, China

Received 4th April 2025 , Accepted 10th June 2025

First published on 12th June 2025


Abstract

Zero-dimensional hybrid metal halides (0D HMHs) have sparked extensive research in the field of optoelectronic materials due to their unique physical and chemical properties. This work innovatively incorporates In3+ into a triphenyl-sulfide-based organic phosphorescent system, successfully constructing a novel 0D hybrid metal halide, (Ph3S)2InCl5. This new material achieves a synergistic output of blue photoluminescence (PL) and green afterglow, which originate from the intrinsic excitation of [Ph3S]+. Through ns2 metal ion (Bi3+/Sb3+) doping engineering, a dual-channel energy transfer pathway is established, enabling the transition from singlet and triplet states to self-trapped exciton states, thereby achieving dynamic control of fluorescence and phosphorescence emissions. Additionally, temperature-dependent PL spectra, time-resolved photoluminescence (TRPL), and Raman spectroscopy are employed to investigate the enhanced photoluminescence of the doped samples, revealing the process of STE (self-trapped excitons) recombination and the electron–phonon coupling processes. Based on these findings, a phosphorescence-PL dual-mode dynamic switching encryption system is constructed, utilizing a time-resolved multi-level decryption strategy to achieve high-order optical anti-counterfeiting. This work not only aids in the in-depth understanding of STE formation in In-based organic metal halides but also provides important guidance for the modulation strategy of STE and afterglow emissions in other 0D HMH luminescent materials.


1. Introduction

Zero-dimensional hybrid metal halides (0D HMHs) attract significant attention in materials science and optoelectronics due to their unique structures and excellent optical properties, which hold promising applications in areas such as photovoltaic cells,1 scintillators,2,3 light-emitting diodes (LEDs),4,5 photodetectors,6 information encryption,7,8 and lasers.9 Unlike inorganic metal halides,10,11 hybrid metal halides are organic–inorganic composite materials that typically consist of inorganic metal halide ions and organic cations.12 The structure of these materials is often composed of alternating organic cations and inorganic halide networks, where the metal halide anion units are completely isolated by the organic cations.13,14 This unique arrangement allows them to exhibit the advantageous properties of both organic and inorganic materials.

Organic cations serve as independent luminous centers, providing emissions that differ from those of the inorganic metal halide units, which impart distinctive optical properties to the materials, including photoluminescence (PL), phosphorescence, and thermally activated delayed fluorescence.15–17 In particular, organic molecules with room temperature phosphorescence (RTP) properties, such as diphenyl sulfone (SF),18 triphenylamine (TPA),19 4-phenylbenzylamine (PBA),20 tetraphenylene (TEP),21 triphenylphosphine (TPP),22 and triphenylsulfonium (TPS),23 combine with inorganic units to form a rigid structure. This structure effectively reduces non-radiative relaxation induced by molecular vibrations and rotations, improves phosphorescence efficiency and extends lifetime.24–26 This attracts widespread attention in fields such as biomedical imaging,27,28 sensors,29 and anti-counterfeiting encryption technologies.30,31

Metal ion doping is a well-recognized strategy for tuning the bandgap of materials. In particular, incorporating ions with an ns2 electronic configuration, such as Bi3+ and Sb3+, can enhance the stability of the material, improve luminescent properties, and introduce new photoluminescent characteristics, such as high quantum yield, substantial Stokes shift, and new luminous centers.32–34 Unlike traditional dopants that involve d- and f-electrons, ns2 dopants leverage the s-electrons, which allow for the simultaneous modulation of the optical absorption and emission characteristics of the materials. However, the large free volume of organic cations in the mixture often leads to a loss of the persistent luminescence associated with these organic cations when combined with luminescent metal halide polyhedra.8,35,36 To address this challenge, we propose a strategy that involves the incorporation of In3+ ions into organic phosphorescent molecules. This approach aims to enhance the afterglow of the organic compounds while simultaneously introducing ns2 ion doping to dynamically regulate the persistent luminescence and STE emissions. However, the complexity of the energy level structure and the various energy transfer pathways introduced by doping complicate the understanding of the mechanisms behind afterglow and STE emissions. This complexity necessitates a detailed investigation into the energy transfer mechanisms and interactions between the doped ions and the luminescent centers to unravel the emission characteristics and optimize the properties for luminescent applications.

In this study, In3+ ions are incorporated into the organic phosphorescent molecule triphenyl sulfide, resulting in the synthesis of the 0D HMH (Ph3S)2InCl5. Additionally, the introduction of Bi3+ and Sb3+ ions with lone pair electrons establishes energy transfer pathways from singlet and triplet states to STE states, enabling controllable modulation of PL and phosphorescence emissions. Compared to the triphenyl sulfide organic molecule, (Ph3S)2InCl5 exhibits significantly enhanced afterglow. However, after doping with Bi3+, the persistent luminescence is notably reduced, and it completely disappears upon doping with Sb3+, revealing only STE emission. Temperature-dependent PL spectra, TRPL spectra, and Raman spectra are employed to elucidate the STE recombination process and the electron–phonon coupling dynamics. Finally, a dynamic persistent phosphorescence–photoluminescence switchable dual-mode encryption system is achieved through time-resolved multi-level encryption technology.

2. Results and discussion

2.1 Basic optical and structural characterization

The synthesis of (Ph3S)2InCl5 crystals occurs via the solvent evaporation method by using triphenylsulfonium and InCl3 in DMF solution. The structure observed along the a-axis is depicted in Fig. 1(a). In this structure, one In atom coordinates with five Cl atoms, forming a distorted [InCl5]2− pyramidal structure. The Ph3S+ cations isolate the [InCl5]2− pentagonal units, thereby constituting a zero-dimensional organic–inorganic hybrid material. The crystal structure adopts the C2 space group of the monoclinic crystal system, and the unit parameters are a = 15.819 Å, b = 14.712 Å, c = 9.508 Å, α = 90°, β = 126.42°, and γ = 90°. The crystal data and structural refinement of (Ph3S)2InCl5 are shown in Table S1. The morphology and distribution of elements are characterized using scanning electron microscopy (SEM) and energy-dispersive spectroscopy (EDS) (Fig. 1(b)). The elements S, In, and Cl show uniform distribution, with the ratio of S, In, and Cl being 3.4[thin space (1/6-em)]:[thin space (1/6-em)]1.8[thin space (1/6-em)]:[thin space (1/6-em)]7.7 (Table S1), which is close to 2[thin space (1/6-em)]:[thin space (1/6-em)]1[thin space (1/6-em)]:[thin space (1/6-em)]5, corresponding to the stoichiometry of (Ph3S)2InCl5. Given the similar ionic radii of In3+ (CN = 5, 0.71 Å), Sb3+ (CN = 5, 0.80 Å) and Bi3+ (CN = 5, 0.96 Å),37 indium-based hybrids serve as the matrix to modify its PL properties by co-doping with ns2 electrons from Bi3+ and Sb3+. By adding BiCl3 and SbCl3 separately to the DMF solution of Ph3SCl and InCl3, (Ph3S)2In1−xBixCl5 and (Ph3S)2In1−xSbxCl5 crystals (x = 0–0.2) are obtained.
image file: d5qi00894h-f1.tif
Fig. 1 (a) Structural view of (Ph3S)2InCl5 and the corresponding organic cation and detailed view of the crystal structure showing the [InCl5]2− pyramid. (b) SEM image of (Ph3S)2InCl5 and elemental distribution of In, Cl, C and S. (c) PXRD spectrum of (Ph3S)2InCl5 and its simulation results. (d) XPS spectrum of the (Ph3S)2InCl5 single crystal. High-resolution XPS spectra of (e) Bi 4f and (f) Sb 3d.

The SEM and EDS characterization are shown in Fig. S1, where Bi and Sb elements are uniformly distributed, demonstrating that Bi3+/Sb3+ ions are successfully incorporated homogeneously into the (Ph3S)2InCl5 lattice. The Bi3+/Sb3+ ions partially replace In3+ to form [BiCl5]2− and [SbCl5]2− pentagonal units. The doping concentrations of Bi3+/Sb3+ are detailed in Tables S2 and S3. The precursor containing 1 mmol [Ph3S]+, 0.45 mmol In3+, and 0.05 mmol Bi3+/Sb3+ yields (Ph3S)2In0.9Bi0.1Cl5 and (Ph3S)2In0.9Sb0.1Cl5 with doping amounts of approximately 12.5% and 10.5% (Bi/[In + Bi] × 100%, Sb/[In + Sb] × 100%), which are consistent with the actual feed ratio. Subsequently, X-ray photoelectron spectroscopy (XPS) further confirms the successful doping of Bi3+/Sb3+, as shown in Fig. 1(d). The XPS spectrum exhibits two peaks at 445.1 eV and 452.9 eV corresponding to the 3d characteristic peaks of In, while the peak at 284.8 eV corresponds to the 1s characteristic peak of C. The high-resolution XPS spectra of Cl, S, Bi, O, and Sb are illustrated in Fig. 1(e, f) and S2. After doping with Bi3+/Sb3+, the peaks of O 1s, C 1s, S 2p, and Cl 2p exhibit certain positive shifts. This is attributed to the weaker electronegativity of In3+ ions being replaced by the stronger electronegativity of Bi3+/Sb3+ ions, leading to positive shifts in binding energy. Furthermore, the successful synthesis of the crystals can also be verified using powder X-ray diffraction (PXRD). As shown in Fig. 1(c) and S3, the PXRD of the measured samples exhibits a high degree of correspondence with the simulated single-crystal X-ray diffraction (SCXRD), and there are no additional diffraction peaks, indicating the successful synthesis of (Ph3S)2InCl5 without the formation of impurities. As the concentration of Bi3+/Sb3+ increases, the XRD peaks of the Sb3+ doped samples shift towards lower diffraction angles. This shift occurs because the ionic radius of Bi3+ (0.96 Å) is larger than that of Sb3+ (0.80 Å) and In3+ (0.71 Å), resulting in lattice expansion, which confirms that Bi3+/Sb3+ successfully replaces a portion of In3+. Additionally, the XRD peaks of the doped samples show a high degree of consistency with the XRD peaks of the matrix and the simulated XRD peaks (Fig. 1(c)), indicating that no phase transition occurs with the doping of Bi3+/Sb3+.

The optical properties of (Ph3S)2InCl5 are revealed through absorption spectra, PL spectra, PLE spectra, and TRPL spectra. The absorption spectra of (Ph3S)2In0.9Bi0.1Cl5 and (Ph3S)2In0.9Sb0.1Cl5 at x = 0, 0.05, 0.1, 0.15, and 0.2 are shown in Fig. S4. The high-energy absorption peak at 277 nm is a combination of the π–π* transition of the phenyl group and the absorption of [InCl5]2−.38–40 The prominent absorption peak at 335 nm corresponds to the transition from Bi3+ 1S0 to 3P1, while the absorption peak at 301 nm corresponds to the transition from Sb3+ 1S0 to 1P1, and the absorption peak at 331 nm is due to the transition from Sb3+ 1S0 to 3P1. Additionally, as the doping concentration increases, the corresponding absorption peaks gradually intensify. These UV-visible absorption results indicate the presence of multiple electronic absorption transitions. The band gaps are calculated using the Tauc plot. As shown in Fig. S5, Bi3+/Sb3+ doping leads to a narrowing of the band gap. With increasing doping concentration, the band gap of (Ph3S)2In1−xBixCl5 (x = 0, 0.05, 0.1, 0.15, 0.2) decreases from 4.15 eV to 3.54 eV, while the band gap of (Ph3S)2In1−xSbxCl5 (x = 0, 0.05, 0.1, 0.15, 0.2) decreases from 4.15 eV to 3.87 eV. This reduction is attributed to the increased lattice distortion caused by the higher doping concentration, resulting in a decrease in the band gap. The PLE and PL spectra of (Ph3S)2InCl5 are shown in Fig. S6(a). It can be observed that the excitation and emission spectra of (Ph3S)2InCl5 are generally consistent with those of TPS-Cl. The TRPL spectrum of (Ph3S)2InCl5 under 375 nm excitation monitored at 440 nm (prompt PL peak) is presented in Fig. S6(b), revealing a PL lifetime of 0.78 ns, which is similar to that of TPS-Cl.23 This further indicates that [InCl5]2− does not directly participate in the luminescence process, and the emission of (Ph3S)2InCl5 originates from the organic Ph3S+ cation. The Ex–Em scans of TPS-Cl and (Ph3S)2InCl5, which are shown in Fig. S9(a) and (b), indicate that they have consistent luminescent centers, and it can be observed that they exhibit excitation wavelength dependence, which suggests the presence of multiple emission centers in this organic emitter. The similar wavelength-dependent PL spectra further confirm that these PL emissions arise from the relaxation of the same excited state. After doping, as shown in Fig. S9(c) and 4(d), (Ph3S)2In1−xBixCl5 exhibits a blue broad emission at 490 nm, while (Ph3S)2In1−xSbxCl5 displays a yellow broad emission at 610 nm. As illustrated in Fig. S7 and S8, the PL intensity increases with the increasing doping concentration of Bi3+/Sb3+, reaching a maximum at x = 0.1. For x > 0.1, the PL intensity decreases with increasing doping concentration, attributed to PL quenching from excessive doping. Therefore, in subsequent tests, the sample with x = 0.1 was selected for further study, which resulted in the measurement of the PLQY of (Ph3S)2In0.9Bi0.1Cl5 of 32.23%. Surprisingly, we found that (Ph3S)2In0.9Sb0.1Cl5 exhibited superior optical performance, with a PLQY that reached as high as 89.72% (Fig. 4(c) and S10). This lays a solid foundation for its future applications in the optoelectronic field, such as in light-emitting diodes (LEDs), laser diodes (LDs), and photodetectors.41,42

The crystals of TPS-Cl, (Ph3S)2InCl5, (Ph3S)2In0.9Bi0.1Cl5, and (Ph3S)2In0.9Sb0.1Cl5 exhibit distinct colors under natural light, ultraviolet irradiation (365 nm), and ultraviolet quenching. Under natural light, all crystals appear colorless. Under a 365 nm UV lamp, TPS-Cl, In–Cl, and In–Bi–Cl emit blue luminescence, while In–Sb–Cl emits bright orange-yellow light. When the UV lamp is turned off, a notable yellow-green afterglow is observed in the TPS-Cl, In–Cl, and In–Bi–Cl crystals. Additionally, the afterglow duration of the In–Cl crystal is the longest, approximately 1.5 seconds, while the afterglow duration of the TPS-Cl crystal is about 0.7 seconds, and the In–Bi–Cl crystal exhibits the shortest afterglow duration of approximately 0.5 seconds. No afterglow emission is observed in the In–Sb–Cl crystal. This indicates that the doping of Bi3+ and Sb3+ plays a crucial role in the afterglow of the crystals. Furthermore, the formation of [InCl5]2− significantly promotes the afterglow of [Ph3S]+.

To reveal the relationship between afterglow and In3+, Bi3+, and Sb3+, the photophysical properties of TPS-Cl, In–Cl, In–Bi–Cl, and In–Sb–Cl crystals were studied. Their prompt and delayed (obtained 10 ms after excitation) PLE spectra, as well as prompt and delayed (obtained 10 ms after excitation) PL spectra under 300 nm excitation, are shown in Fig. 3. As illustrated in Fig. 3(d), the luminescent center of TPS-Cl is located at 440 nm and exhibits a long tail. The afterglow emission center is at 515 nm, which explains the yellow-green afterglow observed in Fig. 2. The luminescent center of In–Cl, which is consistent with that of TPS-Cl as previously mentioned, indicates that their emissions originate from the organic [Ph3S]+ cation. Additionally, the afterglow emission of In–Cl aligns with that of TPS-Cl, which further supports this connection. The measured afterglow quantum yields of TPS-Cl, In–Cl and In–Bi–Cl are 1.8%, 2.5% and 0.8%, respectively.


image file: d5qi00894h-f2.tif
Fig. 2 Optical photographs of TPS-Cl, In–Cl, In–Bi–Cl, and In–Sb–Cl crystals under natural light, UV (365 nm) irradiation and UV off conditions.

image file: d5qi00894h-f3.tif
Fig. 3 The prompt and delayed PLE spectra of (a) TPS-Cl, (b) In–Cl, and (c) In–Bi–Cl. The prompt and delayed PL spectra of (d) TPS-Cl, (e) In–Cl, and (f) In–Bi–Cl. TRPL spectra and fitting curves of (g) TPS-Cl, (h) In–Cl, and (i) In–Bi–Cl.

However, the phosphorescence PLE signals in Fig. 3(a) and (b) show that the signal for TPS-Cl approaches zero in the 375–400 nm range, while In–Cl still exhibits a strong phosphorescence PLE signal. This indicates the presence of energy transfer from [InCl5]2− to the organic [Ph3S]+ cation. In other words, light in the 375–400 nm range cannot directly excite the afterglow of TPS-Cl but can excite [InCl5]2−, which then transfers energy to the triplet state of [Ph3S]+. The enhancement of the persistent luminescence observed in In–Cl, as shown in Fig. 2, is thus elucidated. The luminescent center of In–Bi–Cl is located at 490 nm, which corresponds to the typical blue emission of Bi3+. The PL of In–Bi–Cl is fundamentally consistent with that of TPS-Cl (Fig. 3(g)), indicating that the persistent emission from In–Bi–Cl still originates from the triplet state of [Ph3S]+. As illustrated in Fig. 3(c), the phosphorescence PLE signal of In–Bi–Cl exhibits a distinct excitation peak in the range of 280–320 nm, which emanates from [Ph3S]+. Additionally, the PLE signal in the same range also exhibits a prominent excitation peak from [Ph3S]+, suggesting the presence of energy transfer from [Ph3S]+ to [BiCl5]2−. In Fig. 4(b), the PLE signal of In–Bi–Cl overlaps partially with the persistent luminescence signal of TPS-Cl (indicated by the red dashed area), which further confirms the energy transfer from [Ph3S]+ to [BiCl5]2−. This also explains the reason for the decay of the persistent luminescence observed for In–Bi–Cl in Fig. 2. Under 300 nm excitation, In–Sb–Cl exhibits a dual-peak emission at 490 nm and 610 nm, as shown in Fig. S11(b), and it is noted that no PL signal is detected after the excitation ceases. The PLE spectrum of In–Sb–Cl (Fig. S11(a)) shows a prominent [Ph3S]+ PLE signal in the 280–320 nm range, indicating energy transfer from [Ph3S]+ to [SbCl5]2−. In Fig. S18, the PLE signal of In–Sb–Cl detected at 610 nm partially overlaps with the PL signal of In–Cl (indicated by the red dashed area), which further confirms the energy transfer from [Ph3S]+ to the triplet states of [SbCl5]2−. Additionally, no phosphorescence PLE signal is detectable for In–Sb–Cl, consistent with the earlier observation of the absence of a persistent luminescence signal.


image file: d5qi00894h-f4.tif
Fig. 4 (a) Absorption spectra of In–Cl, In–Bi–Cl and In–Sb–Cl. (b) PLE spectra of In–Bi–Cl and PL spectra of TPS-Cl. (c) PLQY of TPS-Cl, In–Cl, In–Bi–Cl and In–Sb–Cl. (d) Pseudo-color map of PL spectra of (Ph3S)2In0.9Sb0.1Cl5 at different excitation wavelengths. (e) Schematic illustrations of the excited state alignments, energy transfer and relaxation paths of excited states in TPS-Cl, In–Cl, In–Bi–Cl and In–Sb–Cl; S0, ground state; S1, the lowest singlet state; T1, the lowest triplet state; ET1, single state energy transfer; ET3, triplet state energy transfer; ISC, inter-system crossing.

To investigate the exciton dynamics in these materials, a series of time-resolved photoluminescence (TRPL) spectroscopy measurements were conducted. The persistent luminescence lifetime of TPS-Cl was measured at 515 nm, yielding a value of 150.38 ms, corresponding to the triplet emission of [Ph3S]+. In contrast, for the In–Cl associated delayed emission, the lifetime is extended to 191.85 ms when monitored at 515 nm, which is attributed to triplet energy transfer from the [InCl5]2− anion to the [Ph3S]+ cation. However, in the case of In–Bi–Cl, energy transfer from the organic [Ph3S]+ cation to the [BiCl5]2− anion resulted in partial quenching of the persistent luminescence, reducing the lifetime to 88.00 ms. The observed tri-exponential decay behavior in the afterglow arises from a combination of thermally activated delayed fluorescence (TADF), phosphorescence, and the heterogeneous microenvironment within the solid sample. Detailed results are summarized in Table S4.43,44 The long lifetime component (τ3) values of 220.97 ms, 352.97 ms, and 170.23 ms for TPS-Cl, In–Cl, and In–Bi–Cl, respectively, confirm the above energy transfer process. In the triple-exponential fitting analysis, the medium lifetime component (τ2) exhibits the highest amplitude contribution (a2), which corresponds to the radiative complexation of the triplet exciton of the organic cation [Ph3S]+. The a2 value of In–Bi–Cl decreases after Bi-doping, but is still dominant, which suggests that the radiative complexation pathway has not been completely quenched. For In–Sb–Cl, which exhibits a dual emission peak, TRPL spectroscopy was performed on both peaks. As shown in Fig. S13, a lifetime of 19.62 ns was detected at 490 nm, corresponding to the singlet state emission of [SbCl5]2−. These findings highlight the complex interactions and energy transfer processes within these hybrid materials, providing insights into their exciton dynamics and the effects of different dopants on luminescence properties. At 610 nm, the measured lifetime is as shown in Fig. S14, yielding a value of 5.32 μs, which corresponds to the triplet STE emission of [SbCl5]2−.45–47 The strong electron–phonon interactions within [SbCl5]2− cause the excited electrons and holes to induce elastic distortions in the surrounding lattice. Under the influence of the Jahn–Teller effect, this results in a broad PL emission with a high quantum yield.48,49 To further analyze the TRPL lifetimes of In–Bi–Cl and In–Sb–Cl crystals, a 405 nm picosecond laser was focused using a 10× objective to measure the PL dynamics at different positions of a single crystal. The PL images excited at various locations—top (P1), left (P2), center (P3), right (P4), and bottom (P5)—are shown in Fig. S14 and S16, where the blue emission of In–Bi–Cl and the yellow emission of In–Sb–Cl are clearly observed. The corresponding PL decay curves, illustrated in Fig. S15 and S17, show that the PL dynamics at the center and edges of the crystal are essentially similar, suggesting that the crystal is relatively uniform in structure and properties. For In–Sb–Cl, an excitation–emission (Ex–Em) scan was conducted, as shown in Fig. 4(d). Two distinct luminescent centers corresponding to the singlet and triplet emissions of [SbCl5]2− were observed. When excited within the range of 250–340 nm, both singlet and triplet emissions were detected, resulting in a white light emission. In contrast, excitation in the range of 340–400 nm led to yellow-white light emission dominated by triplet emission. These findings illustrate the complex interplay of energy transfer and electron–phonon coupling in these materials, providing valuable insights into their photoluminescent properties and potential applications in optoelectronic devices.

The system regulates the luminescence mechanism through energy transfer between metal halides and organic cations. In TPS-Cl, the radiative transition from S1 to S0 produces fluorescence at 440 nm, while intersystem crossing (ISC) to the T1 state results in afterglow luminescence at 515 nm. In the In3+ system, Dexter energy transfer transmits energy from [InCl5]2− to the organic T1 state, enhancing the afterglow luminescence. After doping with Bi3+, the S1 state of [BiCl5]2− acts as an intermediate level that captures electrons from the organic S1 state (ET1), competing with the radiative transition of organic T1 luminescence, which leads to a reduction in persistent luminescence. The Sb3+ system exhibits a unique dual-channel: the S1 state generates fluorescence at 490 nm, while the T1 state, through Jahn–Teller distortion, forms a low-energy STE state (610 nm). Through multipath energy transfer, excitons from the organic S1/T1 states are trapped in the STE state, ultimately resulting in STE emission via exciton localization, which completely quenches organic persistent luminescence.

2.2 Steady-state PL spectra, transient PL spectra, and Raman spectra at different temperatures

The temperature-dependent PL spectra are used to investigate the electron–phonon coupling processes in the excited state. The temperature-dependent PL spectra of (Ph3S)2InCl5 from 80 K to 250 K are provided in the ESI. The temperature-dependent PL spectra of (Ph3S)2In0.9Bi0.1Cl5 are shown in Fig. 5(a), exhibiting strong blue emission at low temperatures. Similar to (Ph3S)2InCl5, the PL intensity of (Ph3S)2In0.9Bi0.1Cl5 gradually decreases in the temperature range of 80–150 K. From 150 to 220 K, the PL intensity decreases rapidly. Above 220 K, the intensity remains relatively constant due to the saturation of non-radiative recombination channels. Fitting yields an exciton binding energy of 53.22 meV. This exciton binding energy represents the energy required for the dissociation of excitons into free electrons and holes. The exciton binding energy of (Ph3S)2In0.9Bi0.1Cl5 is higher than that of (Ph3S)2InCl5, which is attributed to the presence of [BiCl5]2−, making it more difficult for the electron–hole pairs to dissociate. It is concurrently observed that the emission centers redshift as the temperature increases. From 80 to 240 K, the emission center of (Ph3S)2InCl5 shifts from 437.76 nm to 445.01 nm. From 80 to 300 K, the emission center of (Ph3S)2In0.9Bi0.1Cl5 shifts from 466.73 nm to 480.96 nm. This occurs due to the enhanced electron–phonon coupling at elevated temperatures, leading to a reduction in the bandgap, often referred to as the bandgap renormalization effect. In contrast, (Ph3S)2In0.9Sb0.1Cl5 exhibits a strong resistance to thermal quenching, maintaining significant emission at 400 K (as shown in Fig. 5(b)). The fitting yields an exciton binding energy of 63.52 meV, with this high exciton binding energy further confirming the presence of the STE state.50 The STE state localizes electrons and holes, resulting in enhanced stability of the excitons and an increase in their binding energy. Moreover, as the temperature increases, the full width at half maximum (FWHM) of all three samples broadens, which is attributed to the enhanced electron–phonon interactions at higher temperatures. The electron–phonon interactions can be revealed by the different FWHM values at varying temperatures using eqn (S3). The specific fitting results are shown in Fig. 3(c), where the Huang–Rhys factor of (Ph3S)2In0.9Bi0.1Cl5 is 27.75, with an average phonon energy of 43.71 meV. For (Ph3S)2In0.9Sb0.1Cl5, S is 15.62, and the average phonon energy is 35.67 meV. The smaller S value for (Ph3S)2In0.9Sb0.1Cl5 indicates weaker electron–phonon coupling in this material. The lower phonon energy is associated with its weaker electron–phonon interactions and a larger interatomic distance, thus resulting in better resistance to thermal quenching.
image file: d5qi00894h-f5.tif
Fig. 5 Pseudo color mapping of temperature-dependent PL spectra of (a) In–Bi–Cl and (b) In–Sb–Cl. (c) Fitting of the integrated PL intensities and FWHM of In–Bi–Cl and In–Sb–Cl as a function of temperature. (d) Raman spectra of In–Cl, In–Bi–Cl and In–Sb–Cl. (e) Temperature-dependent Raman spectra of In–Cl. (f) Fitting of the average lifetime of In–Bi–Cl and In–Sb–Cl as a function of temperature.

Temperature-dependent TRPL spectroscopy provides a powerful tool and method for a deeper understanding of the radiative and non-radiative relaxation mechanisms of exciton recombination. As shown in Fig. S20 and S21, we measured the TRPL spectra of (Ph3S)2In0.9Bi0.1Cl5 and (Ph3S)2In0.9Sb0.1Cl5 at different temperatures. It can be observed that their PL lifetimes decrease with increasing temperature, a phenomenon that is attributed to the enhanced electron–phonon coupling discussed above, which leads to thermally activated non-radiative recombination processes;51 additionally, the specific fitting results can be found in the ESI. By fitting the PL lifetime as a function of temperature using eqn (S4) (Fig. 5(d)), we obtained the radiative transition lifetimes of (Ph3S)2In0.9Bi0.1Cl5 and (Ph3S)2In0.9Sb0.1Cl5 to be 9.66 ns and 5.48 μs, respectively, which are close to their respective PL lifetimes. Furthermore, it corroborates the earlier fitting results indicating a smaller Huang–Rhys factor (S) and average phonon energy (ħω) in (Ph3S)2In0.9Sb0.1Cl5. We plot the potential energy diagram to study the thermal activation of carrier trapping (Fig. S27). Here, ΔE represents the energy difference between points E and C in the conduction band, which corresponds to the thermal activation energy. From the fitting in Fig. 5(d), we obtain the thermal activation energies for (Ph3S)2In0.9Bi0.1Cl5 and (Ph3S)2In0.9Sb0.1Cl5 as 122.05 meV and 403.53 meV, respectively. The energy barrier for (Ph3S)2In0.9Sb0.1Cl5 is significantly higher, making it more difficult for the non-radiative transitions caused by phonon thermal vibrations to be activated in (Ph3S)2In0.9Sb0.1Cl5.

The temperature-dependent PL spectra and the parameters obtained from TRPL spectra fitting for (Ph3S)2In0.9Bi0.1Cl5 and (Ph3S)2In0.9Sb0.1Cl5 are shown in Table S5. (Ph3S)2In0.9Sb0.1Cl5 exhibits smaller ħω, S and larger radiative lifetime as well as a higher thermal activation energy, indicating that its phonon thermal vibrations have a relatively weak effect on electrons, resulting in more stable PL performance at high temperatures. Considering these results comprehensively, (Ph3S)2In0.9Sb0.1Cl5 demonstrates higher thermal activation energy with temperature variations, suggesting a stronger ability to resist thermal quenching in high-temperature environments. This characteristic highlights the potential of (Ph3S)2In0.9Sb0.1Cl5 for practical applications, particularly in optoelectronic devices and luminescent materials.

In addition, the thermal vibrations of phonons in the material can also be studied using temperature-dependent Raman spectroscopy. The Raman spectrum at room temperature is shown in Fig. 5(e). With the doping of Bi3+ and Sb3+, there are essentially no changes in the Raman peaks. The three vibrational bands observed at 96.5 cm−1 (asymmetric stretching, E2g mode), 140.4 cm−1 (asymmetric stretching, Eg mode), and 251.4 cm−1 (symmetric stretching, A1g mode) originate from the vibrations of the [InCl5]2−/[BiCl5]2−/[SbCl5]2− pyramids. The modes 2E2g and 2Eg correspond to the overtone of the 96.5 cm−1 and 140.4 cm−1 modes. The peak near 1000 cm−1 is attributed to the vibrations of the C–S bond in organic molecules, while the peak at 1575.2 cm−1 is due to the vibrations of the C[double bond, length as m-dash]C bond in the benzene ring. The temperature-dependent Raman spectra of (Ph3S)2InCl5 are shown in Fig. 5(f). From 80 K to 480 K, the peaks of the organic part gradually red-shift. As the temperature increases, the intermolecular interactions may weaken, leading to a decrease in the energy of the vibrational modes of the molecules, which results in a blue shift of the Raman peaks. Moreover, at higher temperatures, thermal expansion effects may cause the molecular chains to expand and disorder, increasing the degrees of freedom of the molecules, which also contributes to the red shift of the Raman peaks. In contrast, the inorganic component exhibits a significant blue shift at high temperatures. This blue shift occurs because the increase in temperature causes lattice expansion and enhanced lattice thermal vibrations, which in turn increase the vibrational frequency of the phonons and strengthen the electron–phonon interactions. Therefore, we present the temperature-dependent frequency changes in Fig. S22. At high temperatures, temperature-dependent changes in Raman mode frequencies enable the examination of phonon scattering. The temperature coefficients for the E2g and A1g modes are −0.039 and −0.008 cm−1 K−1, respectively (eqn (S5)). The phonon vibrations for the E2g mode are more pronounced. We use eqn (S6) to fit the FWHM of the E2g mode. The fitting results are shown in Fig. S22(d), yielding a phonon energy at 0 K of 48.01 meV. The phonon lifetimes for the E2g and A1g modes are shown in Fig. S22(c) (fitting using eqn (S7)). As the temperature increases, the thermal vibrations of the phonons are enhanced, which increases the coupling between electrons and phonons. This enhanced interaction enables more rapid interaction between phonons and excited-state electrons, resulting in shorter phonon lifetimes.

To study the stability of the samples, after being placed under ambient conditions (22–28 °C, relative humidity 40–60%) for two months, the samples are characterized by PXRD and PL spectroscopy (excitation wavelength 360 nm). The PXRD patterns of all samples (Fig. S25(a–c)) are completely consistent with those of fresh samples, with no obvious impurity peaks or peak position shifts, indicating that the crystal structures remain stable in air. In terms of optical stability, the PL intensity of (Ph3S)2InCl5 decreased to 91.1% of the original value, (Ph3S)2In0.9Bi0.1Cl5 to 94.6%, and (Ph3S)2In0.9Sb0.1Cl5 to 97.6% (Fig. S25(d–f)). These data fully demonstrate that this series of materials exhibit excellent long-term stability in air, and Sb/Bi doping significantly enhances their stability.

2.3 Multilevel anti-counterfeiting encryption system

Dynamic phosphorescence–photoluminescence switches can be used for multi-level anti-counterfeiting. The compounds (Ph3S)2InCl5, (Ph3S)2In0.9Bi0.1Cl5, and (Ph3S)2In0.9Sb0.1Cl5 are ground into powders and filled into different positions on a digital plate, as shown in Fig. 6. Under natural light, the powders appear white, showing no visible differences. When illuminated with a 365 nm UV lamp, the samples are excited and display the number 8, defined as a. After turning off the UV lamp for 0.3 seconds, both (Ph3S)2InCl5 and (Ph3S)2In0.9Bi0.1Cl5 exhibit green afterglow, while (Ph3S)2In0.9Sb0.1Cl5 shows no afterglow, thereby displaying the number 3, designated as b. After turning off the UV lamp for 1.5 seconds, the afterglow duration of (Ph3S)2InCl5 is longer than that of (Ph3S)2In0.9Bi0.1Cl5, leading to the disappearance of the afterglow from (Ph3S)2In0.9Bi0.1Cl5. As a result, the display shows the number 7, defined as c. Using the defined decryption formula (A × 3 + B)/3 − C, the encrypted result is output as 2. Therefore, through afterglow, quadruple encryption of the numbers is achieved, and this time-dependent characteristic enables dynamic and encrypted information output.
image file: d5qi00894h-f6.tif
Fig. 6 Constructing a multi-level digital anti-counterfeiting encryption system using In–Cl, In–Bi–Cl, and In–Sb–Cl. The encrypted output of RGB colors for In–Cl, In–Bi–Cl, and In–Sb–Cl based on binary code and hexadecimal code.

In addition, this study constructs an optical information decryption system with spatiotemporal resolution characteristics by integrating a dynamic phosphorescent–photoluminescent switch with the hexadecimal RGB coding system. As shown in Fig. 6, three samples are integrated into a 9 × 9 matrix, presenting a uniform white camouflage state under natural light. When a 365 nm ultraviolet excitation is applied, the main control unit, (Ph3S)2In0.9Sb0.1Cl5, exhibits characteristic orange-yellow emission (logic “1”), while the remaining control units output blue light (logic “0”), thus creating the initial binary information matrix. The system employs a first-column checking mechanism to determine data validity: when the first column value is “1”, true information parsing for that row is triggered, while a first column value of “0” marks that row as pseudo data flow. After the ultraviolet light source is turned off, the blue light signal captured at the 0.3 second timestamp is designated as interference information, while the phosphorescent decay signal extracted over a 1.5 second time window is identified as a valid information carrier. Based on a multi-level decryption algorithm, the binary data stream is grouped vertically into three rows for hexadecimal reconstruction (e.g., 10111010 → BA, 11011010 → DA, 11000001 → C1), ultimately generating color encoding output that conforms to the sRGB standard (e.g., #BADAC1).

3. Conclusions

In summary, we prepared (Ph3S)2InCl5 crystals through solvent evaporation and regulated the afterglow and STE emission by doping with Bi3+/Sb3+. We investigated the energy transfer among the components through excitation and emission spectra, ultimately demonstrating that the STE state quenches the afterglow emission, while the PLQY of (Ph3S)2In0.9Sb0.1Cl5 reaches up to 89.72%. By analyzing temperature-dependent PL, TRPL, and Raman spectra, we explored the electron–phonon coupling processes. Fitting these data allowed us to obtain physical information such as exciton binding energy, the Huang–Rhys factor, average phonon energy, thermally activated energy, radiative transition lifetime, and non-radiative transition lifetime, revealing the strong thermal quenching resistance of (Ph3S)2In0.9Sb0.1Cl5. Furthermore, the use of these materials to construct a multi-level anti-counterfeiting and information security encryption platform paves the way for designing high-security, dynamic, encrypted output anti-counterfeiting materials.

Author contributions

Hongbo Qi: data curation, formal analysis, writing – original draft, and preparation. Jing Li: conceptualization and software. Hailong Yu: conceptualization and software. Jing Zhang: software and validation. Chen Chen: software and validation. Qiuju Han: validation. Wenzhi Wu: writing – review & editing, supervision, and funding acquisition.

Conflicts of interest

There are no conflicts to declare.

Data availability

All data supporting the findings of this study are available within the paper and its ESI. Data will be made available on request from the corresponding author.

Acknowledgements

W. Z. acknowledges the financial support from the Heilongjiang Provincial Key Laboratory of Micro-nano Sensitive Devices and Systems (Heilongjiang University), the Basic Research Project for Outstanding Young Teachers of Heilongjiang Province (YQJH2023128), and the Cultivation Project of Double First-class Initiative Discipline by Heilongjiang Province (LJGXCG2022-061).

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Footnote

Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d5qi00894h

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