Yoko
Fukui
*a,
Yukihiro
Yoshida
*b,
Hiroshi
Kitagawa
b and
Yohei
Jikihara
a
aNBC Meshtec Inc., 2-50-3 Toyoda, Hino, Tokyo 191-0053, Japan. E-mail: fukui.yoko@nisshin.com
bDivision of Chemistry, Graduate School of Science, Kyoto University, Kitashirakawa-Oiwakecho, Sakyo-ku, Kyoto 606-8502, Japan. E-mail: yoshiday@ssc.kuchem.kyoto-u.ac.jp
First published on 17th April 2024
In our preceding paper (Y. Fukui et al., Phys. Chem. Chem. Phys., 2023, 25, 25594–25602), we reported a systematic study of the Ag+-ion conducting behaviour of silver iodide (AgI)-loaded mesoporous aluminas (MPAs) with different pore diameters and AgI-loading ratios. By optimising the control parameters, the Ag+-ion conductivity has reached 7.2 × 10−4 S cm−1 at room temperature, which is more than three orders of magnitude higher than that of bulk AgI. In the present study, the effect of silver bromide (AgBr)-doping in the AgI/MPA composites on Ag+-ion conductivity is systematically investigated for the first time, using variable-temperature powder X-ray diffraction, differential scanning calorimetry, and electrochemical impedance spectroscopy measurements. The AgBr-doped AgI/MPA composites, AgI-AgBr/MPA, formed a homogeneous β/γ-AgI-structured solid solution (β/γ-AgIss) for the composites with AgBr ≤ 10 mol%, above which the composites underwent a phase separation into β/γ-AgIss and face-centred cubic AgBr solid solutions (AgBrss). The onset temperature of the exothermic peaks attributed to the transition from α-AgI-structured solid-solution phase to β/γ-AgIss or AgBrss decreased with increasing the AgBr-doping ratio. The room-temperature ionic conductivity of the AgI–AgBr/MPA composites exhibited a volcano-type dependence on the AgBr-doping ratio with the highest value (1.6 × 10−3 S cm−1) when the AgBr content was 10 mol%. This value is more than twice as high as that of the highest conducting AgI/MPA found in our previous study.
Ions in ionic solids are essentially immobile due to the electrostatic interactions between the oppositely charged ions. Among them, a silver ion with a 4d10 electron configuration is particularly promising as a carrier ion in solid-state ionic conductors, primarily owing to its soft acidic nature.10 In particular, silver iodide (AgI) with a low room-temperature ionic conductivity (ca. 10−7 S cm−1) exhibits an extraordinary high ionic conductivity (ca. 1 S cm−1) in the high-temperature α-phase (T > 147 °C), where the melted Ag+ ions migrate in the immobile I− sublattice.11–15 It is known that the reduction in the size of AgI particles leads to the stabilisation of the highly ion-conducting α-phase by virtue of the high surface energy; for example, the transition temperature from the α-phase to the low-temperature β- and γ-phases is significantly lowered to 37 °C for AgI nanoparticles with a diameter of 6.3 nm.16–19 However, organic polymers embedded with the AgI nanoparticles to prevent their aggregation apparently disturb the long-range Ag+-ion migration, which is critical for their practical use in the field of solid-state ionics. Another way to increase the room-temperature ionic conductivity of AgI is the introduction of interstitial Ag+ ions near the surface of the β/γ-AgI particles (even if AgI is not in the α-phase), because the formation energy of Frenkel pairs comprised of an interstitial Ag+ ion and a Ag+-ion vacant site decreases with decreasing particle size.20 In addition, the incorporation of the AgI particles into insulating mesoporous metal oxides, such as alumina,21–32 silica,33–39 zeolite,40 and zirconia,33 is beneficial for enhanced ionic conductivity as a consequence of the space-charge layer formed at the heterogeneous interface.41–46
Our group has recently reported the effect of the pore size of mesoporous alumina (MPA) and the filling level of AgI into MPA on Ag+-ion conductivity.47 We found that the AgI/MPA composite, in which the pore space was nearly fully occupied by β/γ-AgI, exhibited the highest room-temperature ionic conductivity when MPA has an average pore size of 7.1 nm. Notably, the ionic conductivity, 7.2 × 10−4 S cm−1, is more than three orders of magnitude higher than that of the bulk β/γ-AgI (ca. 1.5 × 10−7 S cm−1).16 In this study, we focused on the solid-solution system with homovalent substitutions of immobile I− ions, because the substitution efficiently produces a local distortion in the lattice to induce the Frenkel defects.48–73 In fact, the bulk AgI–AgBr solid solutions showed a significant increase in ionic conductivity compared with that of the parent AgI, which motivated us to investigate the effect of the homovalent substitution on the Ag+-ion conductivity of the AgI/MPA composites. To the best of our knowledge, the simultaneous introduction of AgI and AgBr into mesoporous materials has not yet been achieved. This paper presents the dependence of the room-temperature structural and ion-conducting properties of AgI/AgBr-loaded MPA composites (hereafter AgI–AgBr/MPA) on the AgBr-doping level, where a MPA with the highest conducting AgI/MPA composite in ref. 47 (pore diameter: 7.1 nm) was utilised. In addition, we examined the variable-temperature structural, calorimetric, and ion-conducting properties, especially for the purpose of the assessment of the thermal stability of each phase in the AgI–AgBr/MPA composites.
Notation | AgI (mol%) | AgBr (mol%) |
---|---|---|
Br0 47 | 100 | 0 |
Br1 | 99 | 1 |
Br5 | 95 | 5 |
Br10 | 90 | 10 |
Br20 | 80 | 20 |
Br30 | 70 | 30 |
The PXRD peaks of the composites with AgBr ≤ 10 mol% (i.e., Br0–Br10) were assigned only to β- or γ-AgI phases, whereas the PXRD patterns of the composites with AgBr > 10 mol% (i.e., Br20 and Br30) exhibited additional peaks that were assigned to the face-centred cubic (fcc) AgBr phase (Fig. 1(b)). Therefore, the composites with AgBr ≤ 10 mol% form a homogeneous solid solution with β/γ-AgI-type structures in which AgBr was dissolved in the AgI lattice (hereafter β/γ-AgIss), whereas those with AgBr > 10 mol% underwent a phase separation into the aforementioned β/γ-AgIss and another solid-solution phase in which AgI was dissolved in the AgBr lattice (hereafter AgBrss). Furthermore, the formation of the solid solution of AgI in the AgBr lattice is evident from the shift of the (200) reflection of AgBrss to the lower angle side than that in parent bulk AgBr (e.g., 29.9° for Br20vs. 30.9° for parent bulk AgBr) as a reflection of the partial substitution of Br atoms with larger I atoms in the AgBr lattice (ionic radius: 1.96 Å for Br−, 2.19 Å for I−74,75). On the other hand, the PXRD peaks of β/γ-AgIss were barely shifted by the heat treatment, which can be attributed to the fact that the amount of AgBr dissolved in AgI is less than that of AgI dissolved in AgBr as observed in bulk AgI–AgBr mixed crystals.52,55,73,76,77
To investigate the effect of AgBr-doping on the thermal behaviour, the DSC profiles of the AgI–AgBr/MPA composites were measured during the heating and cooling processes. Focusing on the cooling process, two exothermic peaks were observed for the composites with AgBr ≤ 10 mol% (i.e., Br0–Br10; Fig. 3(a)–(d)). Given that the composites remain a single β/γ-AgIss phase in this AgBr content region at room temperature (Fig. 1(b)), both DSC peaks can be assigned to the structural phase transition from the α- to β/γ-phases of AgIss. In our previous paper,47 we identified that the high- and low-temperature DSC peaks observed for the parent AgI/MPA composite (i.e., Br0) are associated with the bulk-like AgI occupying the core and AgI near the surface of the pores, respectively. Therefore, it is possible that the same assignment holds for AgI–AgBr/MPA composites. For the composites with AgBr > 10 mol% (i.e., Br20 and Br30), only one exothermic peak, possibly corresponding to the low-temperature side, was observed, as shown in Fig. 3(e) and (f). Because the heating scan of the DSC profile of Br20 exhibited two distinct endothermic peaks assignable to the β/γ-AgIss-to-α-AgIss and AgBrss-to-α-AgIss (α-AgIss: solid-solution phase with α-AgI structure) at ca. 110 and 170 °C, respectively,70 it is likely that the corresponding exothermic DSC peaks merge into the broad peak in the cooling process. This is reinforced by the very broad temperature range of the phase transitions observed in the temperature-dependent PXRD measurements (see below). Furthermore, the transition enthalpy comparable to those of the composites with AgBr ≤ 20 mol% (Fig. 4(a)) supports the assignment. On the other hand, the transition enthalpy of Br30 is significantly lower than the others, which may be associated with the significant increase in the AgBrss-to-α-AgIss transition temperature as observed in bulk AgI–AgBr mixed crystals (ca. 200 °C for AgBr = 30 mol%).52,55,73,76,77 The incomplete transition to α-AgIss in the measured temperature range was verified by the temperature-dependent PXRD measurements (see below).
As shown in Fig. 4(b), the onset temperatures of the peaks decreased with increasing AgBr-doping ratio. The rapid decrease in the transition temperatures of the composites with AgBr ≤ 10 mol% can be primarily attributed to the lattice distortion induced by AgBr-doping, which causes the increase in the Frenkel defect concentration to stabilise the high-temperature phase. Furthermore, the phase separation observed in the composites with AgBr > 10 mol% may suppress the α-AgIss-to-β/γ-AgIss transition in the cooling process.
Variable-temperature PXRD measurements of the AgI–AgBr/MPA composites were performed to understand their phase transition behaviour from a structural perspective. Fig. 5(a) shows the PXRD patterns of Br10 during heating and cooling processes. The as-prepared composite demonstrated the PXRD peaks assignable to β/γ-AgIss at 30 °C with a trace of AgBrss (2θ = 30.3°), which disappeared after cyclic heating and cooling treatments implying the metastable nature of the phase in this composite. On heating, the β/γ-AgIss peaks began to disappear at ca. 100 °C with the concurrent appearance of the α-AgIss peak, and eventually became invisible above ca. 150 °C. The phase transition was more explicit when the ratio of each phase determined by Rietveld analysis is plotted as a function of temperature (Fig. 5(b)). Refinements were performed under the assumption that only I atoms occupy the halogen sites in AgIss, whereas only Br atoms occupy the sites in AgBrss. In the subsequent cooling process, the α-AgIss phase was maintained down to ca. 60 °C, below which it underwent a reversible transformation to the β/γ-AgIss phase (Fig. 5(c)). It is readily apparent that the structural transition occurs at which an intense peak was observed in the DSC profile (Fig. 3(d)), supporting the above identification of the phase transition. In addition, we measured the temperature dependence of the PXRD patterns of Br20 (Fig. 5(d)) and Br30 (Fig. 5(g)), which underwent a phase separation into β/γ-AgIss and AgBrss at room temperature. The molar ratios of the AgI/AgBr phases were estimated to be 33:67 for Br20 and 14:86 for Br30 based on the Rietveld refinement, indicating that a significant level of I atoms was incorporated in AgBrss as mentioned above. For Br20, the gradual disappearance of both phases entailed the appearance of the α-AgIss phase in the temperature range of 110–140 °C for β/γ-AgIss and 110–180 °C for AgBrss (Fig. 5(e)), which are possibly associated with the broad endothermic DSC peaks at approximately 110 and 170 °C, respectively, in the heating process. In the cooling process, the α-AgIss phase was reversibly transformed to the β/γ-AgIss and AgBrss phases (Fig. 5(f)), although there was only one exothermic DSC peak at ca. 40 °C. Considering that gradual phase transition processes were observed in the PXRD measurements, the DSC peaks assigned to the two transitions may have merged into a broad peak as mentioned above. The temperature-dependent PXRD data of Br30 bear a few similarities to Br20, along with several striking differences. As shown in Fig. 5(h), the β/γ-AgIss phase in Br30 disappeared at ca. 120 °C in the heating process, which is associated with the broad endothermic DSC peak at approximately 110 °C. The corresponding α-AgIss-to-β/γ-AgIss transition, which is responsible for the DSC peak with the onset temperature at 30 °C, was observed at approximately 40 °C in the cooling process (Fig. 5(i)). It is noteworthy that the AgBrss phase in Br30 remained stable even at 195 °C, which must cause the observed low transition enthalpy (Fig. 4(a)). The phase diagram of the AgI–AgBr/MPA composites, in which the phase boundaries were defined when the molar ratio of β/γ-AgIss or AgBrss phase reaches 50% relative to that at 30 °C, resembles that of bulk AgI–AgBr mixed crystals55 with a slight shift towards a lower temperature (Fig. S5, ESI†).
The ionic conductivity (σ) of the AgI–AgBr/MPA composites with various AgI:AgBr molar ratios was measured using AC impedance spectroscopy (Fig. 6 and Fig. S6, ESI†). The room-temperature value (σ25°C) lies in the order of 10−4–10−3 S cm−1, which is significantly higher than that of bulk AgI (ca. 1.5 × 10−7 S cm−1).16 As shown in Fig. 6, the composites with AgBr ≤ 10 mol% exhibited an Arrhenius-type ionic conduction up to approximately 140 °C, whereas those with AgBr > 10 mol% showed a moderate continuous increase in σ with increasing temperature up to the highest measured temperature (200 °C) without any significant slope change. Considering the fact that the composites with AgBr > 10 mol% formed a phase separation between β/γ-AgIss and AgBrss at room temperature, it is possible that the phase separation suppresses the discontinuous change in σ as observed for bulk AgI, which must be reflected in a very gradual increase in the ratio of α-AgIss phase on heating (Fig. 5(e) and (h)). The activation energy (Ea) values estimated by fitting the data up to 130 °C to the Arrhenius equation, σT = Aexp(−Ea/kBT), where A is the pre-exponential factor and kB is the Boltzmann constant, are shown in Fig. 7(a). The Ea values of the bulk AgI–AgBr mixed crystals reported by Shahi and Wagner are also shown for comparison.49–51,78 The Ea value of AgX is generally expressed as Ea = Hf/2 + hm, where the migration energy of Frenkel defects (hm) is smaller than the formation enthalpy of Frenkel defects (Hf).50,79 Thus the lower Ea value of Br0 (0.32 eV) than that of bulk AgI (0.56 eV) can be attributed to the decreased Hf owing to the formation of AgI nanoparticles in the mesopores of MPA and the decreased hm owing to the space charge layer formed at the interface with MPA. The Ea values of the AgI–AgBr/MPA composites remained relatively unchanged with the AgBr content, whereas the values of the bulk AgI–AgBr mixed crystals steadily decreased with increasing AgBr content (Fig. 7(a)). Apparently, the decrease in Ea in the bulk AgI–AgBr mixed crystals arose from the decrease in Hf with increasing AgBr content due to the lattice distortion induced by the partial substitution of I with Br in the AgI lattice. At present, the factor that keeps the Ea values nearly constant in the AgI–AgBr/MPA composites is unclear. However, the tendency seems to be associated with the fact that the 2-fold increase in σ25°C with 10 mol% AgBr doping in the AgI–AgBr/MPA composite (see below) is significantly low compared with the increase in three orders of magnitude in the bulk AgI–AgBr mixed crystals. The σ value at 200 °C was the highest for the composite with AgBr = 10 mol% (i.e., Br10; 5.7 × 10−2 S cm−1), above which the value exhibited a gradual decrease with increasing AgBr content (3.4 × 10−2 S cm−1 for Br30) (Fig. S7, ESI†), primarily due to the incomplete transition to the highly ion-conducting α-phase.
Fig. 6 Temperature dependence of σ for AgI–AgBr/MPA composites with various AgI:AgBr molar ratios ((a) Br0, (b) Br1, (c) Br5, (d) Br10, (e) Br20, and (f) Br30) in heating (closed circles) and cooling (open circles) processes. The red and blue arrows indicate the onset temperatures of the transition on the high- and low-temperature sides, respectively, in the DSC cooling process (Fig. 3). |
Fig. 7 Plots of (a) Ea and (b) σ25°C against AgBr-doping ratio for AgI–AgBr/MPA composites represented by closed blue squares. Closed grey squares represent the values of bulk AgI–AgBr mixed crystals.49–51,78 |
The ion-conducting behaviour in the subsequent cooling process was considerably different from that in the heating process for each composite (Fig. 6). For the composites with AgBr ≤ 10 mol%, the temperature at which the valley-like σ behaviour was observed (ca. 100 °C) corresponds approximately to the onset temperature of the exothermic DSC peaks on the high-temperature side (red arrows). Considering the fact that the structural transformation from α-AgIss to β/γ-AgIss with an expanded lattice (e.g., 64.0 Å3 per formula unit for α-AgIss at 110 °C vs. 67.8 Å3 per formula unit for β-AgIss at 30 °C in Br10) occurs at the core of the mesopores below the temperature, the flattening or upturn of σ observed in the temperature range may be attributed to the connection of the Ag+-ion conducting percolation pathways26,80–82 formed by the α-AgIss region owing to the expanded lattice on cooling.31 Similarly, the valley-like behaviour of σ was observed at approximately 100 °C for the composites with AgBr > 10 mol%, although there is no DSC peak in the temperature range. However, given that the variable-temperature PXRD measurements of Br20 and Br30 exhibited a nearly constant or increasing unit cell volume of the α-AgIss phase on cooling (Fig. S8, ESI†), the expanded lattice may be the primary cause of the non-Arrhenius-type conduction observed in the cooling process. We confirmed that the room-temperature PXRD pattern remained unchanged after the cyclic heating and cooling processes (Fig. S9, ESI†).
As shown in Fig. 7(b), the AgBr-doping ratio dependence of σ25°C showed a volcano-type correlation with a maximum at AgBr = 10 mol% (i.e., Br10). It is evident that the σ value (1.6 × 10−3 S cm−1) is more than twice as high as that of the highest conducting AgI/MPA (i.e., Br0; 7.2 × 10−4 S cm−1) reported in our previous paper.47 An increase in σ25°C in the low AgBr-doping range is possibly related to the increase in Ag+ migration caused by an increased concentration of Frenkel defects due to the lattice distortion. A decrease in σ25°C in the high AgBr-doping range is caused by phase separation as evidenced by the PXRD measurements, which disturbs the Ag+-ion diffusion at the phase boundary in the composites (Fig. S10, ESI†).
Footnote |
† Electronic supplementary information (ESI) available: Fig. S1–S13. See DOI: https://doi.org/10.1039/d4cp00744a |
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