Lead-free halide double perovskites are stable and versatile materials for a wide range of applications, particularly for lighting, thanks to their very efficient emission of warm white light. Element substitution in halide double perovskite is recognized as a powerful method for tuning the emission wavelength and improve the efficiency. This review provides an overview on composition and recent progress in halide double perovskite with main focus on the synthesis and emission properties of chloride-based compounds.

In recent years, inorganic chloride-based lead-free double perovskites (DPs) with formula Cs2M+M3+Cl6, more properly known as elpasolites, have emerged as single-component white light emitters for phosphors and LEDs.

The most prominent property of DPs is broadband, visible light emission with quantum yield approaching unity, a feature that, combined with outstanding stability, has motivated researchers to study in depth their properties and photophysics. Furthermore, the versatile perovskite structure allows to incorporate a variety of ions as substituting elements, resulting in the opportunity to control the absorption and emission processes. Both absorption and emission spectra of double perovskites are ideally suited for lighting purposes. The absorption is typical of large gap semiconductors and insulators, with a steep, direct bandgap in the blue or near UV spectral region so that most compounds are transparent across most or all the visible spectrum. On the other hand, emission is broadband and mostly in the visible spectrum. The corresponding color temperature spans from warm white (as low as 2500 K color temperature) to cold white (higher than 6000 K), with extremely high color rendering index values. DPs compare therefore very favorably with the current technology for white light emission, which is based on semiconductor compounds, such as InGaN, with yellow emitting YAG:Ce3+; however, the resulting light typically lacks a red component thus generating a cool-white emission not ideal for indoor general lighting.1 

Recent reviews describe the developments of DPs both in the form of colloidal nanocrystals and microcrystals, also insights from computational studies and thermodynamic stability are explored along with other emerging DP-inspired materials such as the so-called vacancy-ordered perovskite in the form of Cs2M4+X6.2–5 This review will explore the physical origin of the optical properties of double perovskites, specifically the Na/Ag and In-based, combining both experimental evidence and insights from computational studies. In particular, the discussion will highlight the roles of self-trapped excitons of parity forbidden optical transitions and of localized orbitals. Synthesis strategies and composition for the most studied double perovskites will be reviewed, including the partial substitution of M+ or M3+ elements with a vast library of metal ions to tune optical properties.

Chloride-based microcrystalline DPs will be discussed explicitly, although most of the arguments are common to their colloidal nanocrystalline counterparts. A brief paragraph is also devoted to the only bromide-based stable compound Cs2AgBiBr6.

Finally, the prospects for applications will be discussed, including phosphors, light-emitting devices, and fast and nontoxic photodetectors for UV light and biomedical imaging.

The general halide perovskite AMX3 has a crystal structure characterized by the M2+ ions octahedrally coordinated in a 3D network of corner-sharing [MX6] octahedra and the A+ ion in the sites among them [Fig. 1(a)].

FIG. 1.

(a) Perovskite AMX3 crystal structure with X in red, A in violet, and M octahedrally coordinated. (b) Double perovskite (elpasolite) Cs2M+M3+Cl6 structure with space group Pm-3m with Cl in green and Cs in red and M+/M3+ octahedrally coordinated.

FIG. 1.

(a) Perovskite AMX3 crystal structure with X in red, A in violet, and M octahedrally coordinated. (b) Double perovskite (elpasolite) Cs2M+M3+Cl6 structure with space group Pm-3m with Cl in green and Cs in red and M+/M3+ octahedrally coordinated.

Close modal
The crystal symmetry of a general perovskite AMX3 can be predicted by the Goldschmidt tolerance factor t, which depends on the size of cation (rA), metal (rM), and halide (rX) radii6 

The octahedral structure is not rigid; instead, it can accommodate distortions that often improve lattice stability. The Goldschmidt tolerance factor is typically between 0.7 and 1.1 and measures the degree of distortion. The ideal perovskite structure has t ≈ 1 and is cubic. When rA is larger than the optimal value, then t > 1 and the structure becomes hexagonal with the M2+ ion moving away from the octahedral center. On the other hand, if rA is too small, 0.75 < t < 1, the MX6 octahedra undergo a tilt, like in prototypical hybrid perovskite MAPbI3 (methylammonium lead iodide, CH3NH3PbI3), and the structure becomes orthorhombic.7 The structure not only determines the stability but also defect formation energy and influences the electronic bands; therefore, many of the perovskite properties depend on the kind of lattice distortion with respect to the ideal cubic structure.

The M2+ cation can be replaced by a monovalent and a trivalent ion thus neutralizing the overall charge in the lattice and resulting in the elpasolite or ordered double perovskite Cs2M+M3+Cl6 [Fig. 1(b)]. The definition of the Goldschmidt tolerance factor t can be extended to double perovskites by using the arithmetic average of the two M-site radii as the radius of the metal cation rM. The range of stability is found for 0.8 < t < 1.8 However, additional conditions exist limiting the size mismatch between the two metal cations, for example, the limit case for rather small size M+ ions, such as lithium, where hexagonal symmetry is observed even if coupled with large size M3+ ions, such as lutetium, with t = 0.978.9 

The crystal structure of halide DPs Cs2M+M3+Cl6 is face-centered cubic with space group Fm-3m, consisting of a 3D framework of corner-shared octahedra with M+ and M3+ alternatively in the center, Cl in the octahedra vertices thus forming MCl6 and Cs in the external cavities among octahedra.

According to the extended Goldschmidt tolerance factor, Ag+ and Na+ have appropriate size for octahedral coordination of chloride or bromide ions in the perovskite lattice along with In3+, Bi3+, and Sb3+;10,11 however, the Sb3+ compound shows a pronounced instability in air, thus making it a bad candidate for applications.12 

Several strategies can be used to synthesize halide DPs in the form of powder and crystals. The most common synthetic approaches are based on hydrothermal methods,13,14 supersaturation crystallization or solution precipitation, and solid-state reaction13 (Fig. 2).

FIG. 2.

Scheme of DPs synthesis techniques. Top: hydrothermal synthesis for large single crystals. Middle: supersaturation method for microcrystals. Bottom: solid state synthesis for powders.

FIG. 2.

Scheme of DPs synthesis techniques. Top: hydrothermal synthesis for large single crystals. Middle: supersaturation method for microcrystals. Bottom: solid state synthesis for powders.

Close modal

The hydrothermal method, with Teflon-lined stainless steel autoclave, allows the growth of mm-sized, high quality single crystals as reported by Luo et al. for Cs2AgInCl6 with trap density as low as 8.6 × 108 cm−3.15 In a typical synthesis procedure, metal chlorides are dissolved in a HCl solution and then heated in autoclave at 150–180 °C with a subsequent slow cooling that determines the final size of the single crystal.

The supersaturation crystallization method is the simplest synthetic approach for the synthesis of microcrystals as it needs ambient conditions to dissolve precursor salts in the hydrohalic acid at relatively low temperature.14 In a typical reaction, both metal chlorides and oxides can be used and dissolved in a HCl solution at 100 °C after vigorous stirring, and then the solution is cooled down. As the temperature decreases, the solution enters in a supersaturated state, and eventually crystals start to nucleate and grow. The size control of the products is therefore poor while the reproducibility of the pure phase is optimal.

Single-phase polycrystalline powders are mainly obtained by solid-state reaction in a fused silica ampoule.16,17 The halide salts are mixed in appropriate molar ratio, and the ampoule is sealed under low pressure and heated typically around 500 °C for a few hours. More recently, a “green” synthesis under mild conditions has been developed.18 In a typical reaction, two stable and transparent precursor solutions are prepared, one slightly acid with chlorides and the other one slightly basic with metal acetates. The formation of DPs occurs when the two solutions are mixed for a certain amount of time, without the use of high temperature or acids but with excess of proper cations during the reaction. All the possible substituting ions are proved to be incorporated uniformly into the DPs without phase separation.

Regardless of the synthetic method, inorganic halide DPs show excellent stability in ambient atmosphere over months, either in the dark or under illumination, even in the presence of moisture.19,20 The thermal stability was also explored on microcrystals, and all the compositions are stable until 400 °C, while Cs2AgInCl6 is stable until 525 °C as no additional phase or decomposition signal in the XRD pattern was detected.21,22

Colloidal nanocrystals can be synthesized by the most common strategies, such as hot-injection method and antisolvent recrystallization, resulting in cubic nanocrystals with narrow size distribution. For more details, we refer to the several excellent reviews on DP colloidal nanocrystals and references therein.23–25 

The near unit emission efficiency of Na/Ag–In/Bi DPs is linked to the simultaneous presence of different ions in the same site. In their pure form, the two most stable undoped compounds Cs2AgInCl6 and Cs2NaInCl6 show a very low emission quantum yield. Volonakis et al.26,27 synthesized Cs2AgInCl6 and, by combining first-principles calculations and experimental data, found out the direct nature of its bandgap and investigated the photoluminescence emission in the visible range under UV light. All the compounds with either Na+ or Ag+ in the monovalent site and In3+ in the trivalent site have direct and large bandgap (larger than 3 eV), and the emission is broad-band in the visible range. Such compounds however show a nearly zero intrinsic photoluminescence quantum yield and the absorption at photon energies close to the bandgap edge is low.

The optical emission mechanism, with large Stokes shift and broadband emission, has been linked to the formation of self-trapped excitons (STEs), i.e., bound electron–hole pairs trapped by the distortion of the soft lattice induced by the presence of an electronic excited state.28 After photoexcitation, an ultrafast transition occurs from a free exciton to an STE; the strong electron−phonon coupling favors the Jahn−Teller distortion of octahedra upon excitation, and consequently the optical emission from STEs occurs with a reduced photon energy with respect to the bandgap.29 

The low emission quantum yield of the undoped Cs2AgInCl6 has been instead traced back to the parity-forbidden nature of inter-band transitions, related to a high symmetry lattice. The parity-forbidden transition between the valence band maximum (VBM) and the conduction band minimum (CBM) in Cs2AgInCl6 was analyzed by Meng et al. using density functional theory with Perdew–Burke–Ernzerhof (DFT-PBE) approach calculations11 and by Liu et al.30 by ab initio calculations with the Variational Pseudo-Self-Interaction corrected approach (VPSIC).31 It was demonstrated that both the VBM and CBM lie at the Γ point, giving rise to a direct bandgap of about 2.1 eV and a parity-forbidden transition. The VBM is mainly constituted by Ag 4d and Cl 3p orbitals, while the CBM derives from unoccupied In 5s states. The calculated absorption coefficient is below 104 cm−1 and shows an onset with a tail about 1 eV long. Luo et al. experimentally observed two absorption edges: one at 2.1 eV that is parity-forbidden thus extremely weak, and the other one at 3.2 eV with a radiative recombination between electrons in CBM and holes in a lower level VBM-2, which is about 1.10 eV larger than the fundamental direct bandgap. The 3.2 eV transition is parity-allowed and shows a sharp absorption spectrum. These characteristics can explain the experimental optical bandgap of 3.2 eV with a photoluminescence emission energy of 2.1 eV15 (see Table I).

TABLE I.

Bandgap size and photoluminescence quantum yield in chloride DPs with various doping ions.

Bandgap (eV)
CompoundDopant contentPLQY (%) PL max (nm)DirectIndirectReferences
Cs2Na0.6Ag0.4InCl6 Bi3+ = 1% 97.7% (595) 3.08  30  
Bi3+ = 1% 97.3% (555) 6.42  32  
Bi3+ = 0,4% 86.2% (∼550) ⋯  33  
Cu = 1% 62.6% (605) 2.3  34  
Bi3+ = 0.3%, Yb3+ = 13.6% 38.3% (1540) ⋯  35  
Sm = 35% 22% (540)  3.82 32  
Cs2Na0.2Ag0.8InCl6 Mn 1%–100% 21%–41% (618) 3.67–3.82  32  
Yb3+ = 40% 46% (996) 3.4  36  
82% (400-1100) 
Cs2AgIn0.7Cr0.3 Cl6 Yb3+ = 1% 45% (1000) Direct  37  
Cs2Na1-xBi1-xMn2xCl6 x = 0.004 15% (590) ⋯  38  
Cs2NaInCl6 Sb = 5% 79% (455) 5.1  39  
Bi3+/Ho3+ 99% (455) Direct  40  
0.1%–21.5% 72% (655)   41  
Yb3+ = 5.8% 39.4% (994) ⋯   
Cs2AgInCl6 ⋯ ⋯ 3.23–3.53  27, 42, and 13  
Mn = 0.9% 3%–5% (619)   21  
Er3+ = 0.03–4% 7.9% (994 and 1540)   41  
Yb3+ = 6.9%     
Cs2AgBiCl6  ⋯  2.2–2.77 1, 43, 14, and 44  
Cs2AgSbCl6  ⋯  2.24–2.61 13 and 42  
Cs2AgSbBr6  ⋯  1.64–1.93 45 and 46  
Cs2AgBiBr6  ⋯  1.70–2.25 47, 10, 19, 48, 14, 44, 49, 46, and 50  
Bandgap (eV)
CompoundDopant contentPLQY (%) PL max (nm)DirectIndirectReferences
Cs2Na0.6Ag0.4InCl6 Bi3+ = 1% 97.7% (595) 3.08  30  
Bi3+ = 1% 97.3% (555) 6.42  32  
Bi3+ = 0,4% 86.2% (∼550) ⋯  33  
Cu = 1% 62.6% (605) 2.3  34  
Bi3+ = 0.3%, Yb3+ = 13.6% 38.3% (1540) ⋯  35  
Sm = 35% 22% (540)  3.82 32  
Cs2Na0.2Ag0.8InCl6 Mn 1%–100% 21%–41% (618) 3.67–3.82  32  
Yb3+ = 40% 46% (996) 3.4  36  
82% (400-1100) 
Cs2AgIn0.7Cr0.3 Cl6 Yb3+ = 1% 45% (1000) Direct  37  
Cs2Na1-xBi1-xMn2xCl6 x = 0.004 15% (590) ⋯  38  
Cs2NaInCl6 Sb = 5% 79% (455) 5.1  39  
Bi3+/Ho3+ 99% (455) Direct  40  
0.1%–21.5% 72% (655)   41  
Yb3+ = 5.8% 39.4% (994) ⋯   
Cs2AgInCl6 ⋯ ⋯ 3.23–3.53  27, 42, and 13  
Mn = 0.9% 3%–5% (619)   21  
Er3+ = 0.03–4% 7.9% (994 and 1540)   41  
Yb3+ = 6.9%     
Cs2AgBiCl6  ⋯  2.2–2.77 1, 43, 14, and 44  
Cs2AgSbCl6  ⋯  2.24–2.61 13 and 42  
Cs2AgSbBr6  ⋯  1.64–1.93 45 and 46  
Cs2AgBiBr6  ⋯  1.70–2.25 47, 10, 19, 48, 14, 44, 49, 46, and 50  

Broadband emission with low efficiency is present in pure Cs2NaInCl6, but the partial substitution of Na with Ag bypasses the parity-forbidden transition and allows radiative recombination with higher efficiency, between 20% and 40% depending on the synthetic protocol. The emission properties studied by ultrafast spectroscopy demonstrated the presence of excitons trapped in long-lived dark states in the compound and very few bright STEs with nearly 100% radiative efficiency.30 

The homologous compound Cs2NaBiCl6 shows slow conversion to Cs3Bi2Cl9 when exposed to air;12 therefore, the Bi3+ ion is considered more suitable as doping element than main component. In halide DPs, substitution of metal cations is one of the most efficient strategies to modify the emission properties and performance.

Cs2AgBiCl6 DP is also a stable compound, but it has indirect bandgap and has therefore very low emission yields. The whole range of possible intermediate compositions Cs2AgIn1−xBixCl6, with x varied from 0 to 1, has been explored, identifying precisely the transition from direct to indirect bandgap; the transition has been attributed to the band formed by the Bi 6s lone pair.51,52

In the following paragraphs, it will be discussed how the addition of such new elements helps breaking the parity rules and provides additional emission centers. In particular, starting from Cs2NaInCl6, it is possible to move to Cs2AgBiCl6 by gradually incorporating Ag+ and Bi3+ during the synthesis, thus obtaining, for a well-defined composition, high efficient phosphors with PLQY approaching 100%.53 

1. The role of Bi3+

Luo et al. in 2018 studied the possibility to substitute chloride-based DPs with different metals in order to maximize the emission efficiency.33 The most common composition for the highest emission efficiency is Cs2Na1−xAgxIn1−yBiyCl6 with variable x and y values. The simultaneous presence of In and Bi produces PLQY approaching 100%. The highest PLQY is obtained for 1% of Bi3+ substituted in the indium site, while a higher amount of the Bi ion causes self-quenching,54 resulting in lower efficiency (see Fig. 3).

FIG. 3.

VPSIC band energies calculated for various Cs2Na1−xAgxIn1−yBiyCl6 double perovskites; color code: red for conduction In s and valence Bi s bands; magenta for Ag 4d, e.g., bands, blue for Cl p and Bi p bands.

FIG. 3.

VPSIC band energies calculated for various Cs2Na1−xAgxIn1−yBiyCl6 double perovskites; color code: red for conduction In s and valence Bi s bands; magenta for Ag 4d, e.g., bands, blue for Cl p and Bi p bands.

Close modal

Several research groups have proposed an explanation for mechanism involved in the high PLQY, which is reported to be near 100% for Cs2Na0.6Ag0.4InCl6 +1% Bi3+.

From the experimental point of view, in the presence of Bi, a new absorption peak appears at energies lower than the absorption in the pure matrix. The observation has been interpreted as evidence for the fact that the 6s states from Bi reside on top of the valence band and, given the abundance of s states from In at the bottom of the valence band, they significantly enhance the oscillator strength of optical transitions close to the band edge. In other words, the 6s2 lone pair is almost chemically inert, and thus it happens to be delocalized and resides within the energy gap of the matrix, ending up with a crucial role in optical transitions.55 

From the structural point of view, solid-state nuclear magnetic resonance (NMR) spectroscopy reveals a high degree of ordering between M+ and M3+ sites and a maximum PLQY is observed when bismuth is surrounded by 12 indium neighbors in its medium-range structure.51 

Computational simulations by VPSIC show that the host material Cs2NaInCl6 has a large direct bandgap (see Table I) while Cs2AgInCl6 has a narrower bandgap, since the CBM is composed mainly by the indium 5s states and the VBM by the Ag 4d states. However, due to the already mentioned symmetry-forbidden transition between these states, the optical gap appears even larger. The addition of Bi produces a notable change in the band structure; indeed, the Bi 6s orbitals appear at the VBM and change its parity, increasing significantly optical absorption (Fig. 4).

FIG. 4.

Left panel: emission spectrum of Cs2Na0.6Ag0.4InCl6 (black) and Cs2Na0.6Ag0.4InCl6:Bi (orange). Inset: the PLQY for different Ag fraction. Right panel: CIE color map showing the position of the emission color of DP Cs2Na1−xAgxIn1−yBiyCl6 (y = 0.02, black point). Inset: photographs of a set of DP samples with varied x and y taken under UV illumination at 370–390 nm. Adapted with permission from Stroyuk et al., J. Mater. Chem. C 10, 9938–9944 (2022). Copyright 2022 The Royal Society of Chemistry.

FIG. 4.

Left panel: emission spectrum of Cs2Na0.6Ag0.4InCl6 (black) and Cs2Na0.6Ag0.4InCl6:Bi (orange). Inset: the PLQY for different Ag fraction. Right panel: CIE color map showing the position of the emission color of DP Cs2Na1−xAgxIn1−yBiyCl6 (y = 0.02, black point). Inset: photographs of a set of DP samples with varied x and y taken under UV illumination at 370–390 nm. Adapted with permission from Stroyuk et al., J. Mater. Chem. C 10, 9938–9944 (2022). Copyright 2022 The Royal Society of Chemistry.

Close modal

Electronic structure calculations overwhelmingly deal with the ground state of the crystal, and thus they can be directly compared to experimental absorption spectra, since absorption starts from the ground state. Concerning optical emission, however, the process starts from the excited state, which is notoriously difficult to calculate, especially when, like in DPs, the electronic state couples strongly to the lattice degrees of freedom and produces polaronic distortions and self-trapping phenomena. For such a reason, it is extremely difficult to reproduce from first-principle calculations the broadband emission spectrum attributed to STEs. Concerning the role of Bi doping, the link between electronic structure calculations and photoluminescence emission quantum yield is therefore mostly qualitative. On one hand, the 6s Bi states at the top of the valence band are very likely to increase the oscillator strength for optical emission, much like they do for optical absorption.30 On the other hand, other effects have been studied, like the role of Bi in passivating defects responsible for non-radiative decay of optical excitation,29 or its ability to provide localized sites for efficient optical recombination.56 

To further complicate matters, but also rendering them more interesting, the effect of Bi doping on the emission quantum yield is deeply intertwined in the presence of the other monovalent metal cations, namely, Ag and Na. Experimentally, some amount of each of these two elements is needed to achieve efficient emission. The role of Ag has been linked to the need to change the valence band parity and thus bypass the selection rules that forbid dipole transitions.29,56 On the other hand, calculations show that Na orbitals do not contribute significantly to optical transitions close to the band-edge, so the role of Na appears to be more of a structural one, providing the spatial confinement of optical excitations that favors localization and self-trapping.29 

Ultrafast spectroscopy was used to explore the lifetime and recombination processes for the STEs in DPs. In particular, the comparison between transient absorption (TA) and time-resolved photoluminescence (TRPL) has highlighted the fact that long-lived STEs form independently of Bi doping, but the presence of Bi atoms transforms the STEs from almost completely dark to almost completely bright.30 The minimum fraction of Bi3+ sufficient to turn STEs almost completely bright and thus achieve PLQY above 80% was measured to be less than 0.1%. The same ultrafast spectroscopy methods revealed that the presence of Ag is instead crucial to form STEs to begin with. Again, fractions as low as 1% of Ag atoms are sufficient to turn most of the optical excitations into STEs.

2. In3+ substitution with Sb3+

Indirect bandgap is typically formed when lone-pair cations are present, e.g., in Cs2AgSbCl6,57 while direct bandgap materials are obtained with In substituting Sb.13 Nevertheless, some ions like Sb3+ are still attractive as dopant in direct bandgap compounds to improve the emission properties of DPs without affecting the absorption rate. The Sb3+ emission properties are strictly related to its crystallographic environment: in fivefold coordination, Sb3+ ions emit orange light while in six-fold coordination emit blue light.58 The six-fold coordination radius of Sb3+ is suitable for incorporation in DPs as In3+ substitution without evident phase separation and, although it is slightly shorter than In3+, the lattice parameter of chloride DP with increasing amount of Sb3+ is larger than the host In3+ matrix.13,39

The first report of blue emission involves the Sb3+ doping of Cs2NaInCl6.59 The parity symmetries at the CBM and VBM in the bare Cs2NaInCl6 are the same, but the Sb3+ addition in the trivalent site produces a broadband blue emission at 450 nm with STE behavior and lifetime exceeding 1 µs.60 

The incorporation of both Sb3+ and Bi3+ ions into Cs2NaInCl6, on the other hand, is able to generate a dual-emission blue and yellow light with a PLQY of 77%61,62 originated by different [SbCl6]3− distortions related to STEs (Fig. 5). Surprisingly, the Sb3+ doped DP shows improved thermal stability with respect to the undoped counterpart, with a decomposition temperature of 600 °C and an excellent stability under environmental conditions and illumination.59 

FIG. 5.

Dual-emission white-light PL in Sb3+/Bi3+ co-doped single crystals and schematic of the energy level structure of blue and yellow emissive self-trapped excitons. Adapted with permission from Zhou et al., ACS Energy Lett. 6, 3343–3351 (2021). Copyright 2021 American Chemical Society.

FIG. 5.

Dual-emission white-light PL in Sb3+/Bi3+ co-doped single crystals and schematic of the energy level structure of blue and yellow emissive self-trapped excitons. Adapted with permission from Zhou et al., ACS Energy Lett. 6, 3343–3351 (2021). Copyright 2021 American Chemical Society.

Close modal

3. In3+ substitution with lanthanides

The octahedral site of DPs is also suitable for incorporation of lanthanide (Ln3+) ions, such as Yb3+ and Er3+, Nd3+, Ho3+, and Tm3+. The presence of such ions endows DPs with sharp atomic-like optical transitions, often covering the near-infrared (NIR) wavelength bands that are relevant for solid-state lasers (e.g., the 1 µm emission from Yb3+ and Nd3+) and optical communications (1.55 µm emission from Er3+).

Yb3+ ions have a simple f-electronic structure, involving only two multiplets responsible for a single (2F5/22F7/2) transition manifold in the NIR range, at ∼1 µm wavelength. Mahor et al. synthesized Yb3+-doped Cs2AgInCl6 microcrystals and studied the emission properties.63 The incorporation of Yb3+ ions in the DP matrix was below 2% and the NIR photoluminescence showed millisecond-long lifetimes that are close to the intrinsic radiative limit upon UV light excitation, via energy transfer from the host matrix absorbing the light to the f-electron states of the lanthanide. The efficient Yb3+ emission was traced back to the low energy distribution of the DP phonon modes, resulting in negligible non-radiative losses.64 

Bi3+ and Ln3+ co-doping is effective in enhancing the optical emission performance of DPs, both in terms of spectral range and quantum efficiency. Based on the Cs2Na0.6Ag0.4InCl6 host matrix, Bi3+ and Yb3+ co-doping was shown to result in a dual emission consisting of highly efficient, warm-white emission from the STEs and 1 µm emission from the Yb3+ ions.65 The underlying mechanism is an energy transfer process from the STEs of the DP matrix to the Yb3+ ions, as represented in the scheme of Fig. 6. Similarly, Er3+-doping allows for multiple characteristic emission lines spanning the visible and the NIR, arising from the optical transitions 2H11/24I15/2 (525 nm), 4S3/24I15/2 (550 nm), 4F9/24I15/2 (665 nm), 4I9/24I15/2 (805 nm), and 4I13/24I15/2 (1540 nm).35,41,66 As a matter of fact, the presence of Bi3+ is crucial to realizing strong emission from lanthanides through STE-to-Ln3+ energy transfer.66 Quite importantly, concentration quenching effects was found to occur in Er3+-doped DPs as the ion concentration reaches up to values larger than 18%.35 

FIG. 6.

Energy diagram of lanthanide-based DPs, highlighting energy transfer from self-trapped exciton states to Yb3+ electronic states followed by Yb3+ emission around 1 µm. Yb3+ electronic states are labeled using spectroscopic notation.

FIG. 6.

Energy diagram of lanthanide-based DPs, highlighting energy transfer from self-trapped exciton states to Yb3+ electronic states followed by Yb3+ emission around 1 µm. Yb3+ electronic states are labeled using spectroscopic notation.

Close modal

Yb3+-doped DPs also represent a promising platform for highly sensitive thermal detection as the dual-emission from STEs and Yb3+ ions can be modified by tuning the energy transfer between the two emission centers. In fact, the intensity of the Yb3+ NIR PL is sensitive to the lattice temperature and decreases with increasing temperature, whereas its lifetime exhibits only a negligible temperature sensitivity.67 In addition, the visible emission from STEs is highly sensitive to the temperature, and its lifetime decreases sensibly with increasing temperature, which reflects on the energy transfer to Yb3+ levels. The STE/Yb3+ PL intensity ratio turns out to be an effective parameter for optical thermometer sensitivity. Simultaneous doping with Er3+ ions, whose emission is sensitized via cascaded energy transfer, can be exploited to further increase the materials thermal sensitivity.68 

By doping the host matrix with multiple NIR Ln3+, such as Nd, Yb, Er, and Tm, Chen’s group realized a material with ultrabroad band emission from the visible to the NIR, covering the 400–2000 nm emission range.69 Again, the multiband emission from the lanthanides arises from cascaded energy transfer starting from STEs through the lanthanide electronic levels. A compact light source was also fabricated with the Ln-doped DP coupled with a commercial UV LED chip to obtain an ultrabroad emission as shown in Fig. 7.

FIG. 7.

Ultrabroadband LED based on Bi3+/Ln3+ co-doped DP. PL spectrum of the corresponding LED device with an operating current of 200 mA. Inset: Photographs of the LED taken by visible-light camera and NIR camera. Adapted with permission from Jin et al., Light: Sci. Appl. 11, 52 (2022). Copyright 2022, Author(s).

FIG. 7.

Ultrabroadband LED based on Bi3+/Ln3+ co-doped DP. PL spectrum of the corresponding LED device with an operating current of 200 mA. Inset: Photographs of the LED taken by visible-light camera and NIR camera. Adapted with permission from Jin et al., Light: Sci. Appl. 11, 52 (2022). Copyright 2022, Author(s).

Close modal

4. Transition-metal ions: Mn2+, Cr3+, Fe3+

In the case of Mn-doping, the ion involved is divalent (Mn2+) and can replace both Ag+ and In3+ in the Cs2AgInCl6 lattice, generating a new optical emission in the visible range. The host materials is able to transfer the excitation energy from the UV absorbed light to the Mn d-electrons and the de-excitation of Mn d-electrons generates a PL emission centered at ≈ 600 nm with the highest PLQY reaching 5% for the 0.9% doped DP.21,70

On the other hand, the host DP for Mn2+ doping can be Cs2NaBiCl6 as studied by Majher et al.38 giving an orange-red emission with ≈15% quantum yield. The proposed emission mechanism considers Bi3+ ion as the absorption site for UV light whose energy is transferred to Mn2+ that emits light centered at 590 nm.

A more recent study reports Mn2+-doped Cs2AgBiCl6 with an accurate structural study along with the stability of this material confirming the emission in the orange-red range (601 nm) due to the d-d transitions of Mn.71 

Trivalent chromium ions can be incorporated in Cs2AgInCl6 matrix as substitution of In3+ sites in octahedral coordination to obtain a broadband emission in the NIR range. The 3d energy levels of Cr3+ have found to be responsible for the emission in the 850–1350 nm range through the spin-allowed 4T24A2 transition and the overall PLQY is ≈ 22%.16 The co-doping with Cr3+ and Yb3+ is effective to improve the PLQY up to 45% in the same NIR range.37 The enhanced efficiency is attributed to a better crystallinity of the matrix that leads to a more effective energy transfer from STEs states to Cr3+ levels analogously to the already described process in Yb3+-doped compounds and reduced non-radiative recombination.

A different behavior is found in Fe3+ doping of Cs2AgInCl6, which is able to reduce the bandgap down to 1.6 eV, making it more suitable for photovoltaic applications. Nevertheless, at the atomic level, Fe3+ is found to replace In3+ and segregate the matrix in iron-rich homogeneously distributed microscopic domains of different size, depending of the Fe3+ substitution level.72 The total substitution of In3+ with Fe3+ leads to a bandgap of 1.55 eV and an efficient exciton dissociation that is promising for photovoltaic applications.73 

Besides chloride-based DPs, bromide-based ones have been studied recently as candidates for lead-free and stable solar cells, thanks to their lower bandgap and the possibility to obtain thin films by spin coating. However, most bromide DPs happen to be unstable. The only compound that was found to be relatively stable is Cs2AgBiBr6, but it has indirect bandgap that limits light absorption. In addition, carrier mobility is low and lifetime is short, possibly due to the strong electron–phonon coupling, and consequently prototype solar cells have shown low photoconversion efficiency. Several attempts have been made to improve the optoelectronic properties of bromide DPs, such as optimization of film deposition to diminish the concentration of defects states or doping with other elements to reduce the bandgap, but the solar cell efficiency is still below 5%.10,74–77

By controlling the temperature during the growth of Cs2AgBiBr6 single crystals, Gao et al. were able to reduce the bandgap of 0.26 eV possibly caused by an increased level of Ag/Bi disorder.78 The partial replacement of Ag+ ions by Cu+ ions is reported to show enhanced NIR absorption in single crystals.79 However, a single crystal is not suitable to be integrated in a device such a solar cell. Very recently, Zhang et al. developed a specific doping with atomic hydrogen that reduced the film bandgap down to 1.64 eV.80 The hydrogenation process resulted in doping atoms occupying interstitial sites and thus modifying the VB and CB levels through coupling with the perovskite cations. The highest solar cell photoconversion efficiency after hydrogenation was 6.37%, stable under illumination.

In Br-based DPs the incorporation of new ions could be employed to introduce additional physical properties. Magnetic Fe3+, added during the synthesis through FeBr3, replaces Bi3+ and forms FeBr6 homogeneously distributed clusters in the lattice and, besides extending the absorption to 800 nm thanks to bandgap narrowing, shows ferromagnetic or antiferromagnetic response that could be promising for spintronic devices.81 Furthermore, introducing Fe3+ through FeBr2 during the synthesis is reported to generate a new intermediate band that broadens the absorption to 1350 nm. Additionally, photocurrent is generated under NIR irradiation that makes this materials promising both in NIR photodetector and solar cells.82 

When doped with Yb3+, Cs2AgBiBr6 shows outstanding emission properties with PLQY up to 95% and a good stability in air. The mechanism for the emission through Yb3+ is analogous to energy transfer in chloride-based DPs. After optical excitation, electrons transfer to a nearby Yb3+ ion, which emit efficiently in the NIR region through the 2F5/22F7/2 electronic transition.83,84

The most promising field of application for chloride DPs is lighting, since they happen to be the best possible phosphor or emitter materials emitting warm white light with a spectrum almost perfectly fit for human vision and high color rendering, all with quantum efficiencies approaching unity. Furthermore, DPs are stable in air and they retain their emission spectrum and quantum yield for as long as they are tested, even if they are submersed in water. The materials platform of DPs is very flexible and can accommodate many different elements, but the optical properties are very robust against variations in stoichiometry; the warm white light emission spectrum and the high quantum yield depend on the presence of various elements in the composition, but not on their exact amounts. DPs can be engineered to emit efficiently also in the blue spectral region and in the near IR, opening to interesting prospects as laser materials, as well as optical markers in microscopy and biology.

Most optoelectronic applications, such as the realization of LEDs and lasers, require the fabrication of thin films, which is one of the main challenges of the moment. Powders and microcrystals are stable and easy to obtain, but their potential use in light emissive devices is limited due to the presence of intense light scattering. Producing high-quality thin films appear to be much more challenging, since chloride-based DPs are poorly soluble in solvents and not solution-processable. A possible option is represented by low pressure thermal-evaporation, which has been successfully demonstrated, although resulting in PLQY limited to 10%–15%. Very recently, Stroyuk et al. were able to deposit stable and transparent films from microcrystalline Cs2AgxNa1−xBiyIn1−yCl6 with partially preserved PLQY reaching 85%.85 Colloidal nanocrystals can be used as inks for the deposition of films; however, PLQY in such a form is currently lower than in the bulk counterpart probably due to un-passivated surface states or reduced electron–phonon coupling.

It should be remarked that such limitations may be moot or at least not too severe for the application as phosphors, since DPs are transparent in the visible region, and therefore microcrystals can be successfully incorporated in an inorganic glass matrix with similar refractive index to form a composite to be layered on a commercial UV LED chip to convert blue and UV light into warm white one. Doping with lanthanides, on the other hand, allows us to obtain an ultrabroad emission band from the visible range to the NIR range for applications in spectroscopic analysis and multifunctional lighting or non-destructive biomedical imaging. The emission from Yb, due to the energy transfer from STEs, has both intensity and lifetime steeply dependent on temperature and can be applied for the development of highly sensitive optical thermometers.67 

Further investigations are needed to optimize the integration in emissive devices both in the case of pure DP films and composites. The research perspective emphasizes the need for advancing film processing techniques specific to chloride DPs with all the possible ion substitutions. This involves developing methods for directly converting highly efficient powders or microcrystals into optically transparent films and improving the composite materials to preserve high quantum yield.

Any time halide perovskite structure is mentioned, materials are automatically considered promising for photovoltaics. In the case of DP, however, the prospects for photoconversion of sunlight into electric current do not appear particularly good: the bandgap of most compound is way too high for reasonable efficiency so that a very small fraction of solar photons may be absorbed. Furthermore, optical emission at photon energies well below the bandgap demonstrates that excited states may dissipate most of the photon energy before carrier extraction. To be useful as photovoltaic materials, new DPs will have to be synthesized, with much lower bandgap and possibly with a weaker coupling between electronic excitations and lattice deformation, in order to inhibit self-trapping phenomena.

This work was funded by Fondazione di Sardegna through Project No. 2F20000210007 “Perovskite materials for photovoltaics” and Project No. F73C22001160007 “Single crystal hybrid perovskite thin films for optoelectronics.” A.S. was supported by PON “Ricerca e Innovazione” 2014–2020—Fondo sociale europeo, Attraction and International Mobility—Codice AIM1809115 Num. Attività 2, Linea 2.1. Funding is acknowledged under the National Recovery and Resilience Plan (NRRP), Mission 4 Component 2 Investment 1.3 - Call for tender No. 1561 of October 11, 2022 of Ministero dell’Università e della Ricerca (MUR); funded by the European Union – NextGenerationEU, Project code PE0000021, Concession Decree No. 1561 of October 11, 2022 adopted by Ministero dell’Università e della Ricerca (MUR), CUP – F53C220007700077, according to attachment E of Decree No. 1561/2022, Project title “Network 4 Energy Sustainable Transition—NEST.”

The authors have no conflicts to disclose.

Daniela Marongiu: Supervision (equal); Writing – original draft (equal); Writing – review & editing (equal). Stefano Lai: Writing – original draft (equal). Fang Liu: Writing – review & editing (equal). Angelica Simbula: Writing – review & editing (supporting). Francesco Quochi: Writing – original draft (equal); Writing – review & editing (equal). Michele Saba: Writing – original draft (equal); Writing – review & editing (equal). Andrea Mura: Writing – review & editing (supporting). Giovanni Bongiovanni: Writing – original draft (equal); Writing – review & editing (equal).

Data sharing is not applicable to this article as no new data were created or analyzed in this study.

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