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. 2023 Feb 22;12(2):e202200226. doi: 10.1002/open.202200226

Tin Bromido Aluminate Networks with Bright Luminescence

Silke Wolf 1, Ralf Köppe 1, Peter W Roesky 1, Claus Feldmann 1,
PMCID: PMC9944849  PMID: 36811286

Abstract

The novel tin bromido aluminates [Sn3(AlBr4)6](Al2Br6) (1), Sn(AlBr4)2 (2), [EMIm][Sn(AlBr4)3] (3) and [BMPyr][Sn(AlBr4)3] (4) ([EMIm]: 1‐ethyl‐3‐methylimidazolium, [BMPyr]: 1‐butyl‐1‐methyl‐pyrrolidinium), are obtained from a ionic‐liquid‐based reaction of AlBr3 and SnCl2 or SnBr2, resulting in colorless and transparent crystals. 1 contains a neutral, inorganic 3[Sn3(AlBr4)6] network filled with intercalated Al2Br6 molecules. 2 represents a 3D structure isotypic to Pb(AlCl4)2 or α‐Sr[GaCl4]2. 3 and 4 exhibit infinite 1[Sn(AlBr4)3]n− chains that are separated by the voluminous [EMIm]+/[BMPyr]+ cations. All title compounds contain Sn2+ coordinated by AlBr4 tetrahedra, resulting in chains or 3D networks. Moreover, all title compounds show photoluminescence due to Br→Al3+ ligand‐to‐metal charge‐transfer excitation, followed by 5s 2 p 0←5s 1 p 1 emission on Sn2+. Most surprisingly, the luminescence is highly efficient (quantum yield >50 %). Specifically, 3 and 4 exhibit outstanding quantum yields of 98 and 99 %, which are the highest values observed for Sn2+‐based luminescence so far. The title compounds have been characterized by single‐crystal structure analysis, elemental analysis, energy‐dispersive X‐ray analysis, thermogravimetry, infrared and Raman spectroscopy, UV‐Vis and photoluminescence spectroscopy.

Keywords: emission quantum yield, ionic liquid, luminescence, network structure, tin bromido aluminates


The tin bromido aluminates [Sn3(AlBr4)6](Al2Br6), Sn(AlBr4)2, [EMIm][Sn(AlBr4)3] and [BMPyr][Sn(AlBr4)3] are prepared in ionic liquids. Some exhibit 3D network structures and bright Sn2+‐based photoluminescence with quantum yields near 100 %.

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Introduction

Sn2+‐based luminescent materials are typically less efficient in terms of quantum yield (QY) and light output (LO) as compared to, for instance, Mn2+‐based luminescent materials or lanthanide‐doped materials (e. g., with Eu2+, Eu3+, Tb3+). [1] This lower performance can be related to the 5s 2 p 0↔5s 1 p 1 transition on Sn2+ and the strong coupling of both s and p orbitals with the lattice. In the case of tin, lattice coupling is much stronger than for the respective dd, df, and ff transitions on transition metal cations or lanthanide metal cations. [1] Due to lattice strong coupling, sp transitions are more sensitive to loss processes (e. g., lattice vibrations, lattice defects, impurities), show larger Stokes shifts and broader peak widths, and thus, a generally lower efficiency. [1] Consequently, the number of efficient Sn2+‐based luminescent materials is low with, for instance, Ba2Li2Si2O7 : Sn2+, M 3(PO4)2 : Sn2+ (M: Mg, Ca, Sr, Ba), or Ca5(PO4)3F : Sn2+ having quantum yields up to 85 % at maximum.[ 2 , 3 ] These phosphors contain Sn2+ with concentrations of 1–10 mol− %, since concentration quenching is usually observed for higher Sn2+ concentrations (>10 mol− %).[ 1 , 2 ] In addition to these conventional phosphors, organic‐inorganic hybrid tin halides have entered the literature since 2019 in the wake of methylammonium lead iodide perovskite as a novel solar absorber. [4] Here, efficient fluorescence has been reported, particularly for hybrid tin bromides and iodides. Due to the small bandgaps of these compounds (e. g., [C8H17NH3]2[SnBr4], [(PEA)4SnBr6][(PEA)Br] ⋅ (CCl2H2)2 with PEA: phenylethylammonium), however, luminescence usually originates from semiconductor‐type valence band to conduction band transitions, superimposing the sp transition of Sn2+. [5]

Using ionic‐liquid‐based synthesis, we could recently prepare the chlorido metallates [BMIm][Sn3Cl7] as well as [BMIm][Sn(AlCl4)3] and [BMPyr][Sn(AlCl4)3] ([BMIm]: 1‐butyl‐3‐methylimidazolium, [BMPyr]: 1‐butyl‐1‐methyl‐pyrrolidinium), which contain 2[Sn3Cl7] zigzag‐planes as well as 1[Sn(AlCl4)3] chains. [6] Although they contain Sn2+ as a regular lattice constituent with molar quantities (instead of a dopant in a non‐luminescent lattice), they exhibit efficient luminescence with high quantum yields of 46, 51 and 76 %, respectively. This finding and specifically the missing concentration quenching can be ascribed to the large distances between the luminescent Sn2+ centers (≥386 pm in [BMIm][Sn3Cl7], ≥647 pm in [BMPyr][Sn(AlCl4)3]). [6] Regarding these promising luminescence features, even more efficient emission and higher quantum yields could be expected for heavier halides with lower vibrational losses and more rigid network structures. With [Sn3(AlBr4)6](Al2Br6) (1), Sn(AlBr4)2 (2), [EMIm][Sn(AlBr4)3] (3) and [BMPyr][Sn(AlBr4)3] (4) ([EMIm]: 1‐ethyl‐3‐methylimidazolium), we now obtained four novel tin bromido aluminates with network structures showing extraordinary quantum yields up to 99 %.

Results and Discussion

Ionic‐liquid‐based synthesis

[Sn3(AlBr4)6](Al2Br6) (1), Sn(AlBr4)2 (2), [EMIm][Sn(AlBr4)3] (3) and [BMPyr][Sn(AlBr4)3] (4) were prepared by reacting SnCl2 or SnBr2 in a Lewis‐acidic ionic liquid established by a mixture of [Cation]Cl/Br ([Cation]: [BMIm]: 1‐butyl‐3‐methylimidazolium, [EMIm]: 1‐ethyl‐3‐methylimidazolium, [BMPyr]: 1‐butyl‐1‐methyl‐pyrrolidinium) and AlBr3 with a ratio of 1 : 3 (Table S1, Supporting Information). The ratio of 1 : 3 turned out to be crucial for all reactions. On the one hand, the yield drops significantly when using less AlBr3, until no solid compound was obtained at all. With an increasing amount of AlBr3, on the other hand, some AlBr3 remains undissolved, resulting in mixtures of the title compound and AlBr3. All reactions were performed in sealed, argon‐filled glass ampoules by heating to 45–100 °C and result in colorless crystals of the title compounds (Figure 1). While, in principle, all compounds can be obtained at 45 °C, crystal size and quality especially of 24 were improved by performing the reaction at 100 °C. Temperatures >150 °C lead to a decomposition of the ionic liquid as indicated by their reddish‐brown color after the reaction. In sum, the formation of the title compounds can be rationalized with the following reactions [Eqs. (1–4]:

3SnBr2+8AlBr3[Sn3(AlBr4)6](Al2Br6) (1)
SnCl2+3AlBr3+[BMIm]ClSn(AlBr4)2+[BMIm]++[AlCl3Br]- (2)
SnBr2+4AlBr3+[EMIm]Cl[EMIm][Sn(AlBr4)3]+AlBr2Cl (3)
SnBr2+3AlBr3+[BMPyr]Br[BMPyr][Sn(AlBr4)3] (4)

Figure 1.

Figure 1

Unit cells and photos of single crystals of a) [Sn3(AlBr4)6][Al2Br6] (1), b) Sn(AlBr4)2 (2), c) [EMIm][Sn(AlBr4)3] (3), d) [BMPyr][Sn(AlBr4)3] (4) (Sn2+ coordination polyhedra: grey, [AlBr4]: orange, Al2Br6: green, [EMIm]+/[BMPyr]+: grey with both possible positions displayed in (c) and (d)).

Structure and composition

[Sn3(AlBr4)6](Al2Br6) (1) crystallizes in the form of colorless bars in the monoclinic space group P21 /c (Table S2, Supporting Information). 1 exhibits a unique inorganic 3[Sn3(AlBr4)6] network with intercalated Al2Br6 molecules (Figures 1 and Figure S1). To the best of our knowledge, such Al2Br6 intercalation is here observed for the first time. The non‐charged 3[Sn3(AlBr4)6] network consists of Sn atoms that are coordinated and linked by AlBr4 tetrahedra, leading to an eightfold coordination of bromine around Sn2+ (Figure 2 and Figures S1–S4). In detail, three different Sn2+ sites occur, whereof Sn1 and Sn3 are largely similar to each other. Thus, Sn1 and Sn3 exhibit Sn−Br distances of 287.4(1) (Sn2−Br18) to 322.3(1) pm (Sn3−Br19) (Figure 2 and Figures S3,S4), which is comparable to SnBr2. [7] The SnBr8 polyhedra can be described as significantly distorted bicapped trigonal prisms. In sum, Sn1 and Sn3 are each coordinated by four μ2‐coordinating AlBr4 tetrahedra (Figure 2, and Figure S2). In contrast, Sn2 shows (7+1) coordination, with six Sn−Br distances between 300.4(1) (Sn3−Br26) and 321.1(1) pm (Sn3−Br14) and one slightly elongated distance of 332.7(1) pm (Sn2−Br17). Finally, one Sn−Br distance is much more elongated with 351.3(1) pm (Sn2−Br24) (Figure 2), which even exceeds the longest Sn−Br distances in SnBr2 (338.7 pm in α‐SnBr2, 341.8 pm in o‐SnBr2). [7b] This elongation can be rationalized by the (7+1) coordination of Sn2+ in 1 compared to the sixfold coordination of Sn2+ in SnBr2. [7] In contrast to Sn1 and Sn3, Sn2 is coordinated by five AlBr4 tetrahedra. Three AlBr4 tetrahedra are μ2‐coordinating and two only with one bromine atom (Figure S2). All AlBr4 tetrahedra show distorted tetrahedral geometries with Al−Br distances of 226.4(2) (Al7−Br24) and 234.0(2) pm (Al5−Br18) as well as Br−Al−Br angles of 104.1(1) to 115.8(1)°, which fits well with literature data.[ 3 , 8 ] In sum, the AlBr4 tetrahedra connect Sn2+ to an inorganic 3D network with pores in the b,c plane. Such intercalation of aluminium halides – to the best of our knowledge – is observed for the first time. Moreover, such 3D networks were rarely observed for halogenidoaluminates. Thus, (AlBr4)‐interconnected arrangements were yet described only for Sn(C7H8)(AlBr4)2⋅C7H8, Sn(C9H12)(AlBr4)2, and (C9H12)SnBr(AlBr4). [3]

Figure 2.

Figure 2

Sn2+ coordination and Sn−Br distances (in pm) in [Sn3(AlBr4)6](Al2Br6) (1) for the different crystallographic sites: a) Sn1, b) Sn2, c) Sn3.

The pores in the 3[Sn3(AlBr4)6] network are filled with non‐charged Al2Br6 molecules with similar molecular features as Al2Br6 molecules in solid or gaseous AlBr3. [9] The Al−Br distances are 221.1(2)–221.8(2) pm for terminal Br atoms and 240.4(2)–241.9(2) pm for bridging Br atoms, which are well comparable with solid AlBr3 (221.9–222.3 and 240.4–242.2 pm) [9a] as well as gaseous AlBr3 (222.7 and 242.1 pm). [9b] The similar distances and angles of the Al2Br6 molecules in 3[Sn3(AlBr4)6] and in solid/gaseous AlBr3 point to neglectable binding of the molecules with the 3[Sn3(AlBr4)6] matrix. The shortest non‐bonding Al…Br contact in 1 (414 pm) is even longer than that in solid Al2Br6 (394 pm). [10]

The similarity of Al2Br6 molecules in 1 with pure AlBr3 is further validated by Fourier‐transform infrared (FTIR) spectroscopy and Raman spectroscopy (Figure 3). In this regard, FTIR spectroscopy was performed for all title compounds. For 3 and 4, the spectra are dominated by vibrations of the [EMIm]+/[BMPyr]+ cation (3250–2900, 3100–2800 cm−1). For 1 and 2, weak vibrations of [BMIm]+ are also observed due to adhered ionic liquid on the crystal surfaces, which is in accordance with elemental analysis (Figure 3a). Regarding the Al2Br6 molecule in 1, moreover, Raman spectra were recorded and exhibit vibrations similar to pure AlBr3 (Figure 3b), [11] which again points to the single‐molecule‐like behavior of Al2Br6 in 3[Sn3(AlBr4)6]. [12] The signals at 413, 215, and 134 cm−1 are attributed to slightly disturbed (<7 cm−1) fully symmetric terminal and bridging Al−Br stretching vibrations (representation ag of a molecule of D 2h symmetry) as well as to the rocking mode of the terminal AlBr2 group. The band at 215 cm−1 is superimposed by the symmetric vibration of AlBr4. [13]

Figure 3.

Figure 3

Vibrational spectra of the title compounds: a) FTIR spectra of all title compounds with [BMIm]Cl as a reference, b) Raman spectra (λexc :532 nm) of [Sn3(AlBr4)6](Al2Br6) (1, light blue) and Al2Br6 molecules in solid AlBr3 (black) as a reference.

Sn(AlBr4)2 (2) crystallizes as colorless blocks in the space group Pbca (Table S2 and Figure S3 in the Supporting Information). Similar to 1, 2 is also a 3D network with its structure isotypic to Pb(AlCl4)2 [14] and α‐Sr[GaCl4]2, [14] respectively. Each Sn2+ ion in 2 is coordinated by nine Br atoms of four μ2‐coordinating AlBr4 tetrahedra and one Br atom of a fifth AlBr4 tetrahedron (Figure 4 and Figure S4). The coordination polyhedron of Sn2+ can either be described as a significantly distorted tricapped trigonal prism or as a capped square antiprism. In parallel to the crystallographic c axis, pairs of these SnBr9 polyhedra are found to share only one edge. There are three sets of Sn−Br distances (Figure 4). The first set ranges from 284.0(1) (Sn−Br1) to 313.3(1) (Sn−Br8) pm and compares to the shorter distances in 1 or SnBr2. [7] The second set of 336.6(1) (Sn−Br7) to 349.3(1) pm (Sn−Br3) is in the range of the longest distances in 1 or SnBr2 (Table 1). [7] With 388.2(1) pm (Sn−Br6), the longest distance is shorter than the sum of the van der Waals radii (403 pm) [15] but longer than distances usually considered for significant interactions. These long distances are observed between Sn2+ and Br atoms of the two edge‐sharing SnBr9 polyhedra (Figure 4). The increased Sn−Br distances in 2, compared to 1, can be ascribed to the higher coordination number of nine in 2. However, by analogy with the isotypic structures Pb(AlCl4)2 [12] and α‐Sr[GaCl4]2, [12b] the description as SnBr9 polyhedra seems reasonable. In accordance with 1, all AlBr4 tetrahedra in 2 are also slightly distorted with Al−Br distances and angles similar to literature data.[ 3 , 8 ]

Figure 4.

Figure 4

Coordination of Sn2+ and Sn−Br distances (in pm) in Sn(AlBr4)2 (2): a) polyhedra and distances, b) edge‐sharing SnBr9 polyhedra.

Table 1.

Sn−Br distances in [Sn3(AlBr4)6](Al2Br6) (1), Sn(AlBr4)2 (2), [EMIm][Sn(AlBr4)3] (3) and [BMPyr][Sn(AlBr4)3] (4) in comparison to selected reference compounds.

Compound

Sn2+ coordination

Short distances [pm]

Long distances [pm]

1

8

287.4(1)–322.3(1)

/

7+1

300.4(1)–332.7(1)

351.3(1)

2

4+4+1

284.0(1)–313.3(1)

336.6(1)–349.3(1), 388.2(1)

3

8

300.2(1)–322.1(1)

/

4

8

297.3(1)–321.6(1)

/

α‐SnBr2 [7b]

6

285.9–333.7

/

o‐SnBr2 [7b]

6

280.6–312.2

341.8

Sn(C9H12)(AlBr4)2 [8a]

6+η6‐C9H12

291.5–338.0

/

Finally, [EMIm][Sn(AlBr4)3] (3) and [BMPyr][Sn(AlBr4)3] (4) crystallize as colorless, elongated plates in the monoclinic space group C2/c (Table S2). As most interesting building unit, both contain infinite 1[Sn(AlBr4)3] chains (Figure S5), similar to those previously observed in, for example, [BMIm][Sn(AlCl4)3].[ 6 , 16 ] In the 1[Sn(AlBr4)3] chains, each Sn2+ is surrounded by three μ2‐coordinating AlBr4 tetrahedra and two μ1‐coordinating Br ions of two additional AlBr4 tetrahedra resulting in an eightfold coordination of Sn2+ with Br in a distorted squared anti‐prismatic geometry (Figure 1 and Figures S3,S4). Four of the five AlBr4 tetrahedra interlink neighboring Sn2+ in a μ2‐μ1 fashion to chains along the crystallographic c axis (Figure S5). The residual fifth AlBr4 tetrahedron coordinates two Br to one Sn atom, together resulting in an eightfold coordination of Sn2+. Such coordination was previously observed in, for example, Sn(C9H12)(AlBr4)2. [8a]

For 3, the Sn−Br distances are 300.2(1) pm (Sn−Br5) to non‐bridging AlBr4, 313.4(1) and 322.1(1) pm (Sn−Br1, Sn−Br2) to μ2‐coordinating AlBr4, and 321.0(1) pm (Sn−Br3) to corner‐sharing AlBr4. For 4, the Sn−Br distances are 297.3(1) pm (Sn−Br5) to the non‐bridging AlBr4, 312.8(1) and 321.6(1) pm (Sn−Br1, Sn−Br2) to the μ2‐coordinating AlBr4 and 320.8(1) pm (Sn−Br3) to the corner‐sharing AlBr4 (Table 1 and Figure S4). These distances are similar to the observed distances in 1 and 2 and agree with literature data, for example, 291.4–338.0 pm in Sn(C9H12)(AlBr4)2. [8a] Again, all AlBr4 tetrahedra in 3 and 4 are slightly distorted with the expected distances and angles.[ 3 , 8 ] Moreover, distances and angles of the [EMIm]+ and [PMPyr]+ cations are as expected. For both, two more‐or‐less mirrored positions were observed in the crystal structure, which were tackled by split atom positions for all atoms with 50 % probability of finding for each position.

Material properties

To validate of the chemical composition of the title compounds, energy‐dispersive X‐ray spectroscopy (EDXS), elemental analysis (C,H,N), and thermogravimetry (TG) were performed. First of all, EDXS confirms the presence of Sn and Al/Br. Here, it must be noticed that Al and Br cannot be reliably distinguished due to the similar energy of the Al−K α emission (1.486 eV) and the Br−L α emission (1.480 eV). Moreover, single crystals of the title compounds decompose rapidly under electron bombardment in vacuum (30 kV) due to Al2Br6 release (Figure S6, Supporting Information). Elemental analysis shows the absence of C/H/N for 1 and 2 and confirms the presence of [EMIm]+ and [BMPyr]+ in 3 and 4 (Table S3). Due to total decomposition of the title compounds, finally, TG allows to quantify the chemical composition and to study the thermal properties. All title compounds show a one‐step decomposition with dark grey residues of elemental tin remaining (Figure S7). Decomposition of 1 starts at 210 °C with a total weight loss of 85.8 %, whereas 2 decomposes at 270 °C with a total loss of 90.6 %, which can be ascribed to the following reactions [Eqs. (5,6]:

[Sn3(AlBr4)6](Al2Br6)3Sn(12.0%)+4Al2Br6(71.9%)+3Br2(16.1%) (5)
Sn(AlBr4)2Sn(14.6%)+Al2Br6(65.7%)+Br2(19.7%) (6)

3 and 4 show comparable decomposition processes starting at 75 and 80 °C with total weight losses of 91.2 and 87.6 %, respectively [Eqs. (7,8]:

[C6H11N2][Sn(AlBr4)3]Sn(9.3%)+1.5Al2Br6(63.1%)+1.5Br2(18.9%)+C2H4(2.2%)+N(C3H4)2(CH3)(6.5%) (7)
[C9H20N][Sn(AlBr4)3]Sn(9.1%)+1.5Al2Br6(61.5%)+1.5Br2(18.5%)+C4H8(4.3%)+NH(C4H8)(CH3)(6.6%) (8)

Regarding the optical properties, first of all, ultraviolet‐visible (UV‐Vis) spectroscopy was performed (Figure S8). Here, weak absorption is observed below 420 (1), 450 (2), and 400 nm (3, 4), which is in accordance with the colorless appearance of the title compounds (Figures 1, 5). The UV‐Vis spectra are compared to those of SnBr2 and AlBr3 as references. Valence‐band‐to‐conduction‐band absorption is observed for SnBr2 with high intensity below 400 nm, which is in accordance with its yellowish color. [17] In contrast, the absorption of the title compounds compares to colorless AlBr3 (Figure S8). Here, weak absorption at 230–400 nm occurs and can be ascribed to Br→Al3+ ligand‐to‐metal charge‐transfer (LMCT) absorption. Intense valence‐band to conduction‐band absorption is observed for AlBr3 below 230 nm. Similar to AlBr3, thus, the weak absorption at 230 to 420/450/400 nm can be attributed to the title compounds, too. The additional absorption of the title compounds, therefore, is attributed to an LMCT transition.

While performing UV‐Vis spectroscopy, we realized that all title compounds also show luminescence (Figure 5), which was quantified by photoluminescence spectroscopy (Figure 6a). Accordingly, 14 exhibit similar absorption below 350 nm. Upon UV excitation (280–350 nm), they show bluish to greenish white emission with emission bands at 400 to 700 nm (Figures 5, 6a). The emission can be related to a 5s 1 p 1→5s 2 p 0 transition on Sn2+. Most interestingly, the luminescence process is very efficient with quantum yields >50 % for all compounds (Table 2). Specifically, 3 and 4 exhibit outstanding quantum yields of 98 and 99 %. Although, Sn2+‐based emission is well‐known in principle, the quantum yield is limited to 80–85 % or much below due to the strong coupling of s and p orbitals with the lattice.[ 1 , 2 ] Moreover, Sn2+ as a luminescence center is usually applied as a dopant (5–10 mol‐ %) in a non‐luminescent host lattice to avoid concentration quenching at higher concentrations (>10 mol‐ %).[ 2 , 3 ] Thus, the efficient Sn2+‐based luminescence is surprising, and the observed quantum yields near unity, to the best of our knowledge, are the highest ever observed for Sn2+. The extremely high quantum yields can be explained by the rigid binding of Sn2+ in the bromido‐aluminate host lattices as well as by the large distance between the luminescent Sn2+ centers (≥673.5(1) pm), so that no concentration quenching occurs despite of molar quantities of Sn2+ in the lattice.

Figure 5.

Figure 5

Photos of [Sn3(AlBr4)6](Al2Br6) (1), Sn(AlBr4)2 (2), [EMIm][Sn(AlBr4)3] (3) and [BMPyr][Sn(AlBr4)3] (4) under daylight and under UV irradiation.

Figure 6.

Figure 6

Luminescence properties of [Sn3(AlBr4)6](Al2Br6) (1), Sn(AlBr4)2 (2), [EMIm][Sn(AlBr4)3] (3) and [BMPyr][Sn(AlBr4)3] (4): a) photoluminescence spectra (with eye‐sensitivity curve), [19] b) color coordinates of the emission of 14 in the C.I.E. diagram.

Table 2.

Luminescence properties of [Sn3(AlBr4)6](Al2Br6) (1), Sn(AlBr4)2 (2), [EMIm][Sn(AlBr4)3] (3) and [BMPyr][Sn(AlBr4)3] (4).

Compound

Max. excitation [nm]

Max. emission [nm]

FWHM [nm]

CIE color coordinates x, y

Quantum yield [%]

1

310

509

139

0.351, 0.492

87

2

315

551

132

0.325, 0.455

56

3

295

497

117

0.224, 0.387

99

4

318

495

115

0.216, 0.344

98

Beside the intense luminescence and partly outstanding quantum yield, another interesting feature is the shift of the color coordinates in the C. I. E diagram (C. I. E.: Commission International de l′Eclairage) [1] between the compounds 14, which is more or less parallel to the blackbody radiation curve (Table 2, Figure 6b). Specifically, the emission of 2 is almost similar to the eye‐sensitivity curve (Figure 6a). By certain adaption of the host lattice (e. g., partial exchange of halogen, partial exchange of aluminium), [18] it could be possible to shift the color coordinates to the blackbody radiation curve and to obtain highly efficient white‐light emitting phosphors.

Conclusions

Four novel tin bromido aluminate networks were prepared by reaction of SnCl2/SnBr2 in Lewis‐acidic ionic liquids based on mixtures of [BMIm]Cl/Br or [BMPyr]Br and AlBr3. Specifically, these are [Sn3(AlBr4)6][Al2Br6] (1), Sn(AlBr4)2 (2), [EMIm][Sn(AlBr4)3] (3) and [BMPyr][Sn(AlBr4)3] (4). The crystal structures are characterized by AlBr4‐coordinated Sn2+ cations resulting in 3D networks in 1 and 2 as well as chain‐like structures in 3 and 4. Interestingly, the 3[Sn3(AlBr4)6] network of 1 contains isolated Al2Br6 molecules with distances/angles similar to Al2Br6 molecules in pure AlBr3. In general, such tin bromido aluminate networks as observed in the title compounds were rarely reported in the literature until now.

Surprisingly, all title compounds show intense bluish white to greenish white emission originating from Br→Al3+ ligand‐to‐metal charge‐transfer excitation, followed by 5s 2 p 0←5s 1 p 1 emission on Sn2+. Especially, 3 and 4 have outstanding quantum yields of 98 and 99 %, which are the highest values observed for Sn2+‐based luminescence so far. The efficient photoluminescence can be explained by the rigid binding of Sn2+ in the bromido‐aluminate network and the great distance between the luminescent Sn2+ centers (≥673.5(1) pm). As a result, loss processes due to thermal quenching and concentration quenching are low. Since the color coordinates of 14 are close to the blackbody radiation curve, certain modification of the host lattice could potentially lead to efficient white‐light emitters with quantum yields near unity.

Experimental Section

Synthesis

General. All reactions and sample handling were carried out under dried argon atmosphere using standard Schlenk techniques or argon‐filled glove boxes. Reactions were performed in Schlenk flasks and glass ampoules that were evacuated (p<10−3 mbar), heated and flushed with argon thrice prior to use. The starting materials SnCl2 (99.99 %, Sigma Aldrich), SnBr2 (99 %, ABCR), and AlBr3 (99 %, ABCR) were used as received. [BMIm]Cl (99 %, Iolitec), [EMIm]Cl (99 %, Iolitec), and [BMPyr]Br (99 %, Iolitec) were dried under reduced pressure (10−3 mbar) at 130 °C for 48 h. All compounds were handled and stored in argon‐filled glove boxes (MBraun Unilab, c(O2, H2O)<0.1 ppm).

[Sn3(AlBr4)6](Al2Br6) (1). 150 mg (0.24 equiv., 0.54 mmol) of SnBr2, 500 mg (1 equiv., 2.28 mmol) of [BMIm]Cl and 1.827 mg (3 equiv., 6.85 mmol) of AlBr3 were heated under argon in a sealed glass ampoule for 2 weeks at 45 °C. At the beginning, a yellowish ionic liquid was formed, in which crystals of 1 grow over several days as colorless cuboids or bars. Crystals can be separated from the IL by filtration through a glass filter to result in a phase‐pure compound with 20–30 % yield. 1 is highly sensitive to moisture and hydrolyses in air within seconds. To obtain large (up to 1 mm) single crystals of 1, the reaction can be alternatively performed at 100 °C for 4 h. As a result, however, a mixture of 1 and crystals of SnBr2 was obtained.

Sn(AlBr4)2 (2). 100 mg (0.18 equiv., 0.53 mmol) of SnCl2, 500 mg (1 equiv., 2.86 mmol) of [BMIm]Cl and 2.290 mg (3 equiv., 8.58 mmol) of AlBr3 were heated under argon in a sealed glass ampoule for 4 h at 100 °C. After cooling to room temperature with a rate of 1 K/h, 2 was obtained as colorless bars in a yellowish ionic liquid with 20–25 % yield. Yield and crystal quality were depending on the applied amount of ionic liquid. With less ionic liquid, the yield was increased, however, the crystal quality decreased and non‐dissolved AlBr3 remained in the sample. With more ionic liquid, the yield decreased even further due to the higher solubility. 2 is highly sensitive to moisture and hydrolyses in air within seconds. Hence, 2 needs to be handled under inert conditions. Similar to 1, the crystals can be separated from the IL via filtration through a glass filter.

[EMIm][Sn(AlBr4)3] (3). 100 mg (0.18 equiv., 0.36 mmol) of SnBr2, 300 mg (1 equiv., 2.05 mmol) of [EMIm]Cl and 1.637 mg (3 equiv, 6.14 mmol) of AlBr3 were heated under argon in a sealed glass ampoule for 4 h at 100 °C. After cooling to room temperature with a rate of 1 K/h, 3 was obtained as large colorless plates in a yellowish ionic liquid with a yield of 25–30 %. Again, yield and crystal quality were depending on the applied concentrations. 3 is highly sensitive to moisture and hydrolyses in air within seconds. Hence, 3 needs to be handled under inert conditions. Crystals can be separated from the IL via filtration through a glass filter.

[BMPyr][Sn(AlBr4)3] (4). 150 mg (0.24 equiv., 0.54 mmol) of SnBr2, 507 mg (1 equiv., 2.28 mmol) of [BMPyr]Br and 1.826 mg (3 equiv., 6.85 mmol) of AlBr3 were heated under argon in a sealed glass ampoule for 4 h at 100 °C. After cooling to room temperature with a rate of 1 K/h, 4 was obtained phase pure as colorless needles in a yellowish ionic liquid with a yield of 35–40 %. 4 is extremely sensitive to moisture and needs to be handled under inert conditions. The crystals can be separated from the IL via filtration through a glass filter.

Analytical equipment

Single‐crystal structure analysis. For single crystal structure analysis, suitable crystals of 14 were manually selected, covered by inert‐oil (perfluoropolyalkylether), placed on a microgripper (MiTeGen), and, thereafter, immediately frozen, which prevented any contact between the crystals and air/moisture. Data collection for 24 was performed at 200 or 213 K on an IPDS II image‐plate diffractometer (Stoe, Darmstadt) using Mo‐Kα radiation (λ=0.71073 Å, graphite monochromator). Data collection for 1 was performed at 180 K on a Stoe StadiVari Diffractometer with Euler geometry (Stoe, Darmstadt) using Ga‐Kα radiation (λ=1.34143 Å, graded multilayer mirror as monochromator). Data reduction and multiscan absorption correction were conducted with the X‐AREA software package and STOE LANA (version 1.75). [20] Space group determination based on systematic absences of reflections was performed by XPREP. Using Olex2, [21] the structure was solved with the SHELXT [22] structure solution program using Intrinsic Phasing and refined with the SHELXL refinement package using Least Squares minimization. All non‐hydrogen atoms were refined anisotropically. Hydrogen atoms were constructed geometrically. Detailed information on crystal data and structure refinements are listed in the Supporting Information (Table S2). DIAMOND was used for all illustrations. [23] Refinement was checked with PLATON. [24]

Deposition Numbers 2202778 (for [BMPyr][Sn(AlBr4)3]), 2202779 (Sn(AlBr4)2), 2202780 (for [Sn3(AlBr4)6](Al2Br6)), 2202781 (for [EMIm][Sn(AlBr4)3]) contain the supplementary crystallographic data for this paper. These data are provided free of charge by the joint Cambridge Crystallographic Data Centre and Fachinformationszentrum Karlsruhe Access Structures service.

Photoluminescence spectroscopy. Excitation and emission spectra were recorded using a photoluminescence spectrometer Horiba Jobin Yvon Spex Fluorolog 3, equipped with a 450 W Xenon lamp, double monochromators for excitation and emission, an integrating sphere (Ulbricht sphere), and a photomultiplier as detector. The determination of the quantum yield was performed according to Friend et al. [25] First of all, the diffuse reflection of the samples was determined under excitation conditions. Thereafter, the emission was measured at this excitation wavelength. Integration over the reflected and emitted photons by use of the Ulbricht sphere resulted in the absolute quantum yield. Corrections were made regarding the spectral power of the excitation source, the reflection behavior of the Ulbricht sphere, and the sensitivity of the detector. The samples were placed inside a glove box in Ar‐filled air‐tight cuvettes, transferred to the spectrometer and then measured.

Supporting Information Summary

Data related to additional analytical methods (EDXS, EA, TG, FTIR, Raman, UV‐Vis) are deposited in the Supporting Information.

Conflict of interest

The authors declare no conflict of interest.

1.

Supporting information

As a service to our authors and readers, this journal provides supporting information supplied by the authors. Such materials are peer reviewed and may be re‐organized for online delivery, but are not copy‐edited or typeset. Technical support issues arising from supporting information (other than missing files) should be addressed to the authors.

Supporting Information

Acknowledgments

The authors thank the Deutsche Forschungsgemeinschaft (DFG) for funding of equipment. Moreover, we acknowledge the Karlsruhe Nano Micro Facility (KNMF), Dr. A. Eichhöfer and especially Prof. Dr. D. Fenske for data collection on a Stoe StadiVari diffractometer with Ga‐metal‐jet source.

Dedicated to Professor Hartmut Bärnighausen on the occasion of his 90th birthday

Wolf S., Köppe R., Roesky P. W., Feldmann C., ChemistryOpen 2023, 12, e202200226.

Data Availability Statement

The data that support the findings of this study are available from the corresponding author upon reasonable request.

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Associated Data

This section collects any data citations, data availability statements, or supplementary materials included in this article.

Supplementary Materials

As a service to our authors and readers, this journal provides supporting information supplied by the authors. Such materials are peer reviewed and may be re‐organized for online delivery, but are not copy‐edited or typeset. Technical support issues arising from supporting information (other than missing files) should be addressed to the authors.

Supporting Information

Data Availability Statement

The data that support the findings of this study are available from the corresponding author upon reasonable request.


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