Akash
Singh‡
ab,
Yi
Xie‡
ab,
Curtis
Adams
III
b,
Benjamin G.
Bobay
c and
David B.
Mitzi
*ad
aDepartment of Mechanical Engineering and Materials Science, Duke University, Durham, North Carolina 27708, USA. E-mail: david.mitzi@duke.edu
bUniversity Program in Materials Science and Engineering, Duke University, Durham, North Carolina 27708, USA
cDuke University NMR Center, Duke University Medical Center, Durham, North Carolina 27710, USA
dDepartment of Chemistry, Duke University, Durham, North Carolina 27708, USA
First published on 19th March 2024
The recent discovery of glass-forming metal halide perovskites (MHPs) provides opportunities to broaden the application domain beyond traditionally celebrated optoelectronic research fueled by associated crystalline counterparts. In this regard, it is crucial to diversify the compositional space of glass-forming MHPs and introduce varied crystallization kinetics via synthetic structural engineering. Here, we compare two MHPs with slightly varying structural attributes, utilizing isomer organic cations with the same elemental composition, and demonstrate how this change in functional group position impacts the kinetics of glass formation and subsequent crystallization by multiple orders of magnitude. (S)-(−)-1-(1-Naphthyl)ethylammonium lead bromide (S(1-1)NPB) exhibits a lower melting point (Tm) of 175 °C and the melt readily vitrifies under a critical cooling rate (CCR) of 0.3 °C s−1. In contrast, (S)-(−)-1-(2-naphthyl)ethylammonium lead bromide (S(1-2)NPB) displays a Tm ∼193 °C and requires a CCR of 2500 °C s−1, necessitating the use of ultrafast calorimetry for glass formation and study of the underlying kinetics. The distinct Tm and glass-formation kinetics of the isomer MHPs are further understood through a combination of calorimetric and single-crystal X-ray diffraction studies on their crystalline counterparts, highlighting the influence of altered organic–inorganic hydrogen bonding interactions and entropic changes around melting, providing insights into the factors driving their divergent behaviors.
Glasses can broadly be categorized as good or poor glass formers, depending on their ease of vitrification and the required critical cooling rate (CCR).22 This classification has a direct impact on their glass-crystal transformation rates. Good glass formers can be vitrified with lower critical cooling rates (10−5 to 100 °C s−1) and tend to exhibit slow or negligible glass-crystal transformations within practical timescales. Examples of good glass formers include inorganic oxides,23 certain molecular organics,24 polymeric,25 and hybrid metal–organic framework glasses.26 These glasses find applications in fields such as optical fibers,27 gas storage,28 and phase-change energy storage systems.29,30 On the other hand, poor glass formers require very high cooling rates (103 to 1010 °C s−1) and exhibit faster glass-crystallization kinetics.31 They are suitable for applications that require fast switching times, such as memory17 and computing devices.19 Metals32 and some chalcogenides,31 particularly Ge–Sb–Te (GST), are known to possess such characteristics. Given the wide range of available organic cations and inorganic frameworks capable of forming 2D or 1D MHPs33 and the ability to tune their thermal properties, including the melting temperature (Tm) with a range of over 150 °C,34–41 it is conceivable that within the MHP family, a wide range of glass-forming ability and varying crystallization kinetics can be achieved. The previously reported S(1-1)NPB perovskite, known for its exemplary glass-forming ability, exhibits a low Tm of 175 °C and a CCR of as low as 0.3 °C s−1 with slow glass-crystal transformation kinetics.12,42 However, in order to broaden the application potential of MHPs in fields that demand rapid switching, it is crucial to develop the capability to control and modulate the glass-forming and glass-crystallization kinetics.
In this study, we examine and modulate the glass-forming and glass-crystallization kinetics in a 2D MHP by replacing the (S)-(−)-1-(1-naphthyl)ethylammonium (S(1-1)NEA) cation in S(1-1)NPB with isomeric (S)-(−)-1-(2-naphthyl)ethylammonium (S(1-2)NEA), which ultimately leads to differing arrangement of the organic cations, intermolecular interactions, and structural distortions for the crystalline versions of the MHPs, despite the same overall atomic composition.43 Interestingly, the resulting 2D MHPs, namely S(1-1)NPB and [(S)-(−)-1-(2-naphthyl)ethylammonium]2PbBr4 (henceforth referred to as S(1-2)NPB), exhibit vastly different glass-forming properties. S(1-1)NPB demonstrates facile glass formation under laboratory timescales, while S(1-2)NPB does not readily vitrify under conditions achievable using conventional calorimetry. Additionally, melt-quenching in thin-film configuration doesn't permit complete vitrification of S(1-2)NPB under typical laboratory experimental timescales, thus, necessitating the use of ultrafast calorimetry44 to study in situ glass formation and glass-crystallization kinetics.
By employing a range of cooling and heating rates spanning two orders of magnitude, we determine the CCR required for glass formation and the characteristic glass transition temperature (Tg) in S(1-2)NPB. Additionally, a Kissinger kinetic modeling is performed to calculate the activation energy required for glass-crystal transformation over a wide temperature range (∼70 °C) facilitated by various heating rates (50–5000 °C s−1). Finally, the distinct thermal and glass-forming properties are elucidated through a comprehensive analysis of the crystal structures of the two MHPs, by scrutinizing the intricate interplay of hydrogen (H) bonding interactions between the organic and inorganic sub lattices, and by understanding the entropic changes around melting. The findings provided in this work establish a fundamental framework for analyzing the impact of structural factors on the kinetics of glass formation and crystallization and serve as a new material design strategy to diversify the family of glass forming MHPs, aiding in broadening their application space.
A conventional differential scanning calorimetry (DSC) measurement of S(1-2)NPB reveals a higher melting point, Tm = 193.4 °C (Fig. 2a), compared to the S(1-1)NPB counterpart, which has a melting point of 175.0 °C,12,13 as also recently reported by Moon et al.43 Furthermore, unlike S(1-1)NPB, which vitrifies into a glassy state at a moderate cooling rate of 20 °C min−1,12S(1-2)NPB does not undergo glass formation even at a cooling rate of 50 °C min−1 (maximum achievable in conventional DSC in the temperature range of interest, Fig. 2a). Instead, an exothermic peak appears during the melt cooling step. However, melt cooling does not lead to complete recovery to a crystalline phase, as indicated by the smaller enthalpy of melt crystallization (ΔHc = 4.0 J g−1) compared to the enthalpy of melting (ΔHm = 37.6 J g−1). Incomplete melt crystallization may be attributed to one of two prospective phenomena—i.e., either partial glass formation or significant decomposition of the MHP. To investigate this observation further, we conducted an iterative DSC measurement and extended it to even lower temperatures, down to −25 °C, with the expectation of possibly observing a glass transition or the cold crystallization of the partial formed glass during the subsequent heating run. However, in the subsequent runs, no signatures of glass transition or cold crystallization were observed; a decrease in Tm and ΔHm, as well as melt crystallization temperature (Tc) and ΔHc over three iterations (Fig. 2b) point to the partial decomposition (organic and hydrogen halide components) of the S(1-2)NPB sample during repeated heat-cool cycles.35,37,46 We expect that S(1-2)NPB will be more susceptible to decomposition upon melting relative to S(1-1)NPB due to the higher Tm. Thermogravimetric analysis (TGA) performed on S(1-2)NPB crystals reveals a degradation onset temperature (Td) of ∼219 °C, exceeding the Tm of ∼193 °C (Fig. 2c). However, partial decomposition cannot be precluded even at temperatures below Td, due to the kinetic nature of the decomposition.37,46Fig. 2d shows a TGA profile for S(1-2)NPB crystals maintained at 195 °C (slightly above Tm), confirming substantial degradation of the sample when subjected to prolonged exposure at elevated temperatures. Furthermore, 1H nuclear magnetic resonance (NMR) measurements conducted on S(1-2)NPB samples that underwent single and multiple extended cycles of melt-quenching in ambient conditions reveal a partial loss of organic molecules (indicated by a reduction in the area under the NMR peaks associated with the H atoms, Fig. S1 and Table S2†) accompanied by a certain degree of molecular degradation (as evidenced by broadening and shifting of peak positions, Fig. S1†), when compared to the pristine S(1-2)NPB sample. The above results highlight the importance of considering sample degradation when exploring hybrid perovskite properties at temperatures near or exceeding 200 °C, as also highlighted during our recent evaluation of the glass-formation characteristics of 1-MeHa2PbI4.46 The use of ultrafast calorimetry, nevertheless, largely circumvents decomposition due to the rapid measurement timescales, as discussed later in the text.
Furthermore, attempts to prepare a melt-quenched film of S(1-2)NPB using a melt pressing technique, which had previously led to complete glass formation for S(1-1)NPB12 and offers higher cooling rates (see ESI†), did not result in complete vitrification. Instead, crystalline peaks corresponding to the (00l) family of planes were observed in the melt-quenched film (Fig. 3). Interestingly, we observe a significant shift in the 00l plane peak positions coupled with broader full width at half maximum (FWHM) values compared to those of the pristine powdered crystals, likely reflecting some disordering introduced by the quenching process. Upon annealing the film at 140 °C for 5 minutes, the diffraction peaks sharpened (Table S3†), indicating enhanced crystallinity, and the 00l plane peaks shifted back to the positions observed for the original crystals.47 Additionally, multiple peaks corresponding to different crystallographic orientations of the film emerged in the annealed film, which match with the simulated powder pattern obtained from the single crystal X-ray diffraction (SC-XRD) data (Fig. S2†). The details of the (002) XRD peak position and the corresponding FWHM for all the curves in Fig. 3 and S2 are listed in Table S3.†
Based on the above analysis, we conclude that S(1-2)NPB has a higher tendency to crystallize during the melt-quenching process relative to S(1-1)NPB, indicating that conventional laboratory-scale cooling rates are not sufficient to access a glassy state. Additionally, the higher Tm of S(1-2)NPB increases the likelihood of partial decomposition when maintained in the melt state over a prolonged duration. Earlier studies have suggested that partial decomposition, which includes the loss of organic components, aids in frustrating the reordering process during melt-quenching and facilitates glass formation compared to a pure stoichiometric melt.14,46,48 However, glass formation upon partial decomposition during multiple heat-cool cycles (Fig. 2b) is not observed under the employed melt-quench rate of 50 °C min−1, suggesting the requirement of faster cooling rate for vitrification of the S(1-2)NPB melt. As a result, an ultrafast (“flash”) calorimetry technique,44,46 which provides ultrafast cooling (up to 4000 °C s−1) and heating (up to 40000 °C s−1) rates, is employed to achieve and study vitrification in the S(1-2)NPB system. The faster heating/cooling timescales provided by the ultrafast calorimetry may also circumvent the decomposition of the MHPs at elevated temperatures, which typically occurs during conventional DSC measurements. To achieve the combined effects, ultrafast colorimetry is thus performed on a small single crystal of S(1-2)NPB (∼166 ng, as described in the ESI†).49 Additionally, a small amount of silicone oil has been applied to cover the sample, providing protection against significant decomposition during heating and maintaining the sample at elevated temperatures.46 Measurements conducted solely on silicone oil did not reveal any discernible features, indicating that silicone oil itself does not undergo any transitions within the temperature range of interest (Fig. S3†).
As a preliminary test, three heat-cool cycles were performed on S(1-2)NPB perovskite using the ultrafast calorimetry technique (Fig. 4a), similar to the conventional DSC measurements (Fig. 2b). In the first heating cycle, the single crystal of the material exhibits a sharp melting peak (Tm ≈ 192 °C). Upon cooling the melt at the same rate (250 °C s−1), we observe a broad exothermic peak, indicating melt crystallization (Tc). The broadness of the peak derives from the kinetic nature of crystallization, as induced by employing a higher melt-cooling rate (250 °C s−1) compared to the conventional DSC method (0.8 °C s−1 or 50 °C min−1). In the second heating cycle, the material exhibits cold crystallization (Tx), suggesting partial glass formation during the preceding cooling cycle. After complete crystallization during continued heating, the sample melts (Tm) again, but with a broader endotherm. The broadening of the melting peak could be attributed to the change in the form factor of the sample i.e., formation of a blob (Fig. 4b) leading to a change in overall thermal conductivity profile (i.e., thermal gradient) across the sample in the second heating run as opposed to a lamellar flat crystal (used in the 1st heating cycle) with a more uniform thermal profile.50 Nevertheless, slight decomposition of the crystal at elevated temperature cannot be precluded, which could aid in broadening of the melting peak alongside a slight reduction of Tm (Fig. 4a).46 Upon cooling the melt, we observe a similar exothermic peak associated with partial melt crystallization, similar to the first cooling cycle with comparable enthalpy values (Table S4†). The glass formation ratio, detailed in Table S4,† reveals vitrification of ∼30% of the melt into a glassy state after melt-quenching, which crystallizes on subsequent heating. To demonstrate the consistency of the thermal features, we performed a third iteration of heating and cooling, which showed the preservation of thermal characteristics without significant changes, confirming that the sample is not undergoing significant decomposition during the subsequent cycling (Fig. 4a).
After recognizing the usefulness of the flash-DSC instrument in effectively demonstrating the melting, partial glass formation, and cold crystallization of the S(1-2)NPB sample, we proceeded to conduct an iterative heating-cooling test. In this test, we varied the cooling rates (250–5000 °C s−1) while maintaining the same heating rate (250 °C s−1), aiming to determine the CCR required for complete glass formation. As shown in Fig. 5a, the S(1-2)NPB sample exhibits partial melt crystallization (Tc) up to cooling rates of 1000 °C s−1 (as indicated in the inset for clarity). However, when cooled at rates higher than this, specifically at 2500 °C s−1, the curve does not exhibit any exothermic crystallization feature. Instead, a glass transition regime is observed, characterized by a change in the baseline (due to a change in specific heat capacity) of the measured curve.12,42,46,51,52 Cooling at even higher rates, such as 5000 °C s−1, also resulted in glass formation; however, it is accompanied by the loss of signal at temperatures below ∼50 °C due to instrument cooling rate limitations in this temperature range.44 Upon analyzing the subsequent heating curves (Fig. 5b), we observe a clear trend toward increasing cold crystallization exothermic peak intensity and area with increased preceding cooling rate.
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Fig. 5 Determination of critical cooling rate (CCR). (a) Cooling curves of S(1-2)NPB melt obtained at various cooling rates. A partial melt crystallization peak (Tc) is observed for a cooling rate up to 1000 °C s−1 (see inset). However, cooling at higher rates (such as 2500 °C s−1) results only in a change of baseline (with no observed peaks in the green curve) suggesting complete glass formation. The vertical axis is only for representation of scale of magnitude, i.e., the curves are vertically offset for clarity. (b) Subsequent heating cycles, all performed at 250 °C s−1, reveal a glass transition regime (Tg; refer to Fig. S4† for a close-up view). Cold crystallization (Tx) exotherms after various cooling rates (250–5000 °C s−1) show an increase in cold crystallization enthalpy (ΔHx) as the preceding cooling rate increases, which saturates after melt-quenching at 2500 °C s−1 due to the complete recovery of the crystallized phase during subsequent heating. Broad features in the temperature range ∼125–150 °C could potentially result from secondary crystallization effects arising from multiple ordering processes and associated kinetics, possibly attributable to the hybrid nature of the organic–inorganic MHP when subjected to ultrafast heating.53,54 The vertical axis is only for representation of scale of magnitude, i.e., the curves are vertically offset for clarity. (c) Enthalpy of the primary cold crystallization (area under the heat flow vs. temperature curve) during heating at 250 °C s−1 after the melt quenching of S(1-2)NPB sample at various cooling rates. The glass formation ratios after melt-quenching at various cooling rates are provided in Table S5† for reference. |
When comparing the cooling rates of 250 °C s−1 and 2500 °C s−1, it becomes evident that the larger cold crystallization peak observed during the subsequent heating cycle results from essentially complete vitrification in the latter case. On the other hand, when cooled at 250 °C s−1, the sample undergoes partial melt crystallization during cooling and additional cold crystallization during subsequent heating. Fig. 5c plots the enthalpy of the primary cold crystallization as a function of the preceding melt cooling rate and points to a saturation of the crystallization enthalpy beyond 2500 °C s−1, suggesting that this cooling rate serves as the approximate CCR for S(1-2)NPB. The glass formation ratio after melt-quenching at various cooling rates (250–5000 °C s−1) is provided in Table S5† for reference. Furthermore, a glass transition (Tg) regime during heating (Fig. 5b) has also been observed at temperatures prior to cold crystallization (Tx). Notably, the S(1-1)NPB counterpart demonstrates a considerably lower CCR value of only 0.33 °C s−1,12 which is approximately 7500 times lower than for the S(1-2)NPB perovskite being investigated. This observation emphasizes how the diverse positions of functional groups in the organic cation can significantly influence the glass-forming kinetics across multiple orders of magnitude.
After determining the CCR, we conducted a study on the kinetics of glass-crystallization of S(1-2)NPB. The sample was repeatedly subjected to glass formation by cooling it at 2500 °C s−1 and then heating at various ramp rates spanning two orders of magnitude, ranging from 50 to 5000 °C s−1. All the cooling curves obtained consistently exhibit a distinct glass transition regime, with a reproducible Tg of 52.6 °C (obtained by mid-point height method,55 Fig. S5†). The heating curves display noticeable shifts in the Tx (indicated by arrows in Fig. 6a), ranging from 87.3 °C to 154.2 °C when the heating rate is varied from 50–5000 °C s−1, respectively. The Tg values are also seen to shift towards higher temperatures (Fig. S6†) on increasing the heating rate akin to what was observed in the S(1-1)NPB system.42 The gradual shift in Tx and Tg on increasing the heating rate is attributed to the competition between the internal molecular reorganization timescale vs. the external experimental timescale provided to the sample during the respective transition through control of heating rates. The shifts in the transition temperatures (Tx and Tg) reveal that they are predominantly governed by the underlying kinetics of molecular/atomic motions, in contrast to Tm, which is a single valued thermodynamic quantity (i.e., not significantly affected by the heating ramp rates).46 Moreover, when comparing the initial heating cycle (50 °C s−1) with the final heating cycle studied (also at 50 °C s−1, obtained immediately after the kinetic analysis), the positions of the Tx and Tm remain unchanged (Fig. S7†). This observation further highlights the robustness of the measurement and indicates minimal organic and hydrogen bromide loss during heating cycles, as facilitated by the presence of silicone oil and the very short heating times.46 For instance, in the conventional DSC experiment conducted in Fig. 2b, the sample remains above Tm (during heating, dwelling, and cooling) for about 2.1 minutes in one cycle. In contrast, during the flash-DSC measurement (Fig. 5), the sample only stays above Tm for approximately 0.1 second, leading to insignificant degradation.
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Fig. 6 Kinetics of glass crystallization. (a) Heating curves of S(1-2)NPB obtained at different ramp rates after the glass formation step (melt quenching at CCR, see Fig. S5†). The shift in the cold crystallization peak (Tx, shown by arrow) with increasing heating rate suggests the kinetic nature of glass-crystallization behavior. The vertical axis is only for representation of scale of magnitude, i.e., the curves are vertically offset for clarity. (b) The shifts in Tx values are used in constructing a Kissinger plot to determine the activation energy of glass crystallization (EA, slope of the curve). The slope of the plot shows a large deviation from a linear trend over the course of change in heating ramp rates (50–5000 °C s−1), revealing breakdown of Arrhenius behavior. |
The observed notable shifts in the Tx values across various heating rates can be utilized to determine the activation energy of the glass-crystallization process for S(1-2)NPB by employing the well-established model proposed by Kissinger.56,57 The Kissinger model extends the principles of Arrhenius and first-order reaction rate equations to non-isothermal conditions and allows for the determination of the activation energy (EA) associated with the glass-crystallization process by considering the change in the peak position of the cold crystallization exotherm (Tx) as a function of the heating rate (qh).56,57 This model offers a straightforward approach to extract the activation energy (EA) using eqn (i):
![]() | (i) |
In conventional DSC measurements, the range of qh is limited, resulting in a Kissinger plot that typically appears as a straight line and thereby providing a single EA value.31,42 Our previous work on crystallization kinetics of S(1-1)NPB shows this behavior—i.e., the Kissinger plot displayed a linear relationship with a single activation energy of approximately 365 kJ mol−1 centered at around 110 °C.42 However, in cases where a wider range of heating rates is employed (as in flash-DSC measurements), the plot may exhibit nonlinearity, indicating a departure from Arrhenius behavior.31 The Kissinger plot for S(1-2)NPB exhibits such behavior (Fig. 6b), where the obtained slope shows a curvature, resulting in a decrease in EA with increasing temperature (143.7 to 43.0 kJ mol−1 with increasing temperature from 87.3 to 154.2 °C). This behavior is not uncommon and has previously been observed in many glass-forming chalcogenide materials.31,58–62 Comparing activation energy of glass crystallization across different glass-forming families, including organic, inorganic, hybrid, and metallic glasses, might not be meaningful due to their distinct characteristic temperatures (Tg and Tx). However, meaningful comparisons can be made within a specific glass-forming family, such as MHPs under similar energy landscapes. For instance, comparing S(1-1)NPB and S(1-2)NPB at ∼110 °C (similar energy landscape) reveals a significant difference. S(1-1)NPB has an activation energy of 365 kJ mol−1 for glass-crystal transformation, while S(1-2)NPB exhibits a much lower activation energy of approximately 86 kJ mol−1. The lower activation energy in S(1-2)NPB indicates a faster reorganization timescale of the glass, i.e., a higher propensity for crystallization compared to the S(1-1)NPB counterpart. However, it is crucial to note that the lower EA value of glass-crystallization in S(1-2)NPB serves only as a necessary condition for explaining higher CCR (Table 1), and the authors are not aware of any direct mathematical relationship that exists between them.
S(1-1)NPB | S(1-2)NPB | |
---|---|---|
T m | 175.0 °C | 193.4 °C |
ΔHm | 43.2 J g−1 | 37.6 J g−1 |
ΔSm | 96.5 mJ g−1 K−1 | 80.6 mJ g−1 K−1 |
CCR | 0.3 °C s−1 | 2500 °C s−1 |
E A (at 110 °C) | ∼365 kJ mol−1 | ∼86 kJ mol−1 |
In the case of S(1-2)NPB, the process of glass formation does not necessitate significant removal of organic and hydrogen halide components, contrasting with the recently described case for 1-methylhexylammonium lead iodide (1-MeHa2PbI4) perovskite comprising flexible aliphatic organic cations, which requires ∼15% mass loss to achieve vitrification under the cooling rates supported by flash-DSC.46 Given that flash-DSC employs an ∼100 ng-scale single crystal for the measurement, the effect of particle size on the crystallization kinetics of the S(1-2)NPB glass could not readily be examined in the current study. However, there is no evidence from the current flash-DSC data pointing toward distinction between nucleation and growth processes, rather yielding a convoluted feature (Fig. 6a) similar to what was previously observed in S(1-1)NPB using conventional DSC.42
Table 1 lists the thermal and kinetic parameters for both glass-forming MHP systems considered in the current study. The high Tm of S(1-2)NPB ∼193 °C relative to S(1-1)NPB ∼175 °C has been recently reported by Moon et al. and attributed to the distinct organic–inorganic H-bonding interactions in the two MHPs.43 Specifically, the different configurations of S(1-1)NEA and S(1-2)NEA cations impact the relative positioning of the ammonium groups in relation to the halogen atoms in the inorganic sub-lattice and the associated organic–inorganic H-bonding interactions, resulting in deeper penetration of the ammonium groups and enhanced strength and asymmetry of H-bonding in S(1-2)NPB.43 Based on our independent SC-XRD structural investigation, average penetrations of the ammonium groups (measured as the distances of the N atoms from the plane of axial Br atoms) of 0.26 Å for S(1-2)NPB and 0.17 Å for S(1-1)NPB (Table S6†) are determined, which supports and validates the results reported by Moon et al.43 Acknowledging that the precise measurement of H atom positions is limited when using SC-XRD, where approximations rely on the positions of heavier N and C atoms,63 we have devised a supplementary methodology that quantitatively compiles and contrasts the positioning of N atoms in relation to the inorganic lattice, which serves as a means to assess the strength of organic–inorganic H-bonding. Both S(1-1)NEA and S(1-2)NEA cations predominantly adopt two types of orientations (cation A and B) in the unit cells (Fig. 7). We find overall shorter N–Pb/Br distances for cation B in S(1-2)NPB relative to S(1-1)NPB (Fig. S8†), suggesting that S(1-2)NEA cation B is positioned in closer proximity to the inorganic lattice and therefore potentially exhibits stronger H-bonding. The analysis details are reported in ESI Section S1 in the ESI.† If H atom positions and associated H-bonding interactions are considered for independent cations A and B (Table S9 and Fig. S9†), as quantified by the H-bond lengths and angles, the values for S(1-2)NPB cation A do not show a clear distinction in relative strength compared to S(1-1)NEA cation A. In contrast, S(1-2)NEA cation B exhibits stronger H-bonding, as indicated by shorter bond lengths and larger bond angles compared to S(1-1)NEA cation B, suggesting an enhanced H-bonding strength in S(1-2)NPB (Table S9†) and perhaps contributing to a higher Tm. The combined N–Pb/Br distances and H-bonding analysis and resultant consistent evaluation results from SC-XRD provide a convincing methodology to evaluate relative H-bonding strength between the two systems (see ESI Section S1 in the ESI† for more details).
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Fig. 7 (a) Schematic of cation A and B in S(1-1)NPB and S(1-2)NPB for calculation of N–Pb/Br distances (Tables S7 and S8†). Blue, red, black, and turquoise spheres denote Pb, Br, C, and N atoms, respectively. The obtained data for S(1-1)NPB is derived from our previously published work.45 (b) Radar chart of the N–Pb/Br distances of type A and B cations in S(1-1)NPB and S(1-2)NPB. Blue and green lines denote the cation A and B of S(1-1)NPB, respectively. Red and yellow lines indicate the cation A and B of S(1-2)NPB, respectively. |
While strong cohesive forces (organic–inorganic H-bonding in the case of MHPs) in the crystalline state are conventionally considered an indicator of higher Tm, this characteristic temperature is influenced by both the enthalpy and entropy contributions surrounding the melting phenomenon. At equilibrium, Tm is defined by the ratio of enthalpy of melting/fusion to the corresponding change in entropy i.e., ΔHm/ΔSm.64 When comparing S(1-1)NPB (Tm = 175 °C, ΔHm = 43.2 J g−1) with its racemic counterpart i.e., rac(1-1)NPB (Tm = 221 °C, ΔHm = 71.0 J g−1),12 for example, ΔHm qualitatively scales with Tm, suggesting a predominantly enthalpy driven melting transition, a perhaps trivial occurrence related to enthalpy–entropy compensation as typically observed in many homologous organic systems.65,66 However, S(1-2)NPB exhibits a higher Tm compared to S(1-1)NPB, although the measured ΔHm for S(1-2)NPB is smaller, at 37.6 J g−1, than the value of 43.2 J g−1 for S(1-1)NPB (Table 1; possibly attributable to different coordination in the melt states of the two systems)67 indicating that the driving force behind the higher Tm in S(1-2)NPB likely extends beyond the strength of cohesive forces in the crystalline state to the entropic contribution during the melting transition.67,68 The higher computed ΔSm = 96.5 mJ g−1 K−1 of S(1-1)NPB relative to ΔSm = 80.6 for S(1-2)NPB (Table 1) therefore presumably (at least in part) underlies the lower Tm.69–71 A more quantitative analysis of the various modes of entropy in the molten states and the local ordering in the melt state is therefore needed to better clarify this point, which is a subject of future interest. Nevertheless, examination of the free organic amines in the MHP structure reinforces the above observation; molecular S(1-1)NEA is a liquid at room temperature and exhibits a relatively high boiling point of 152 °C,72 whereas the amine S(1-2)NEA only melts above 53 °C but shows a lower boiling point of 143 °C.73 The disparate trend in characteristic temperatures indicates a stronger cohesive force in molecular S(1-1)NEA, resulting in a higher boiling point, but a lower Tm due to higher ΔSm. A similar trend in Tm is recorded in molecular organics containing naphthalene with methyl substitution at the first (−30 °C) and second (34 °C) carbon positions.70
Hence, while many physical properties such as boiling point, heat of vaporization, density, and refractive indexes can be defined through change in cohesive forces, the melting behavior is dictated by the combined contributions of both the cohesive forces and the corresponding entropy change,70 thus providing an added flexibility when selecting organic cations before synthesizing a hybrid perovskite with predictable trend in melting behavior. Moreover, a higher Tm of S(1-2)NPB may induce faster crystallization kinetics during cooling due to elevated internal thermal energy of the system, which increases the probability of overcoming the nucleation energy barrier during melt-quenching,67,74 and contributes to an increased CCR required to obtain a glassy state. On the other hand, S(1-1)NPB resists crystallization, partially because of the lower Tm, and also perhaps due to the higher ΔSm (presumably indicative of a greater number of orientations in the melt state), which reduces the overall probability for molecules to attain the precise (and singular) orientation necessary to facilitate crystallization.24,75
Footnotes |
† Electronic supplementary information (ESI) available: Methods; structural refinement data for S(1-2)NPB; summary of integration of NMR peaks for pristine and melt-processed S(1-2)NPB crystals; FWHM values calculated from XRD pattern of crystalline powder, melt-quenched and annealed films; glass formation ratio during preliminary testing of vitrification for S(1-2)NPB melt at a cooling rate of 250 °C s−1; glass formation ratio for S(1-2)NPB vitrification at various cooling rates (250–5000 °C s−1); 1H NMR spectra of the pristine and melt-quenched S(1-2)NPB crystals; simulated vs. experimental XRD pattern for S(1-2)NPB; flash-DSC heating and cooling curves of silicone oil; glass transition regime on heating for S(1-2)NPB; glass transition regime on cooling for S(1-2)NPB; glass transition regime on heating at various ramp rates for S(1-2)NPB; reproducibility test of the kinetic study for S(1-2)NPB; supplementary Section S1: organic–inorganic H-bonding analysis; ammonium group penetration into the inorganic sub-lattice; calculated difference in N–Pb/Br distances of cation A and B for S(1-1)NPB and S(1-2)NPB; organic to inorganic distances for S(1-1)NPB; organic to inorganic distances for S(1-2)NPB; hydrogen bonding interactions for S(1-1)NPB vs. S(1-2)NPB with distinct cation orientations; hydrogen bonding distances and angles for S(1-1)NPB vs. S(1-2)NPB. See DOI: https://doi.org/10.1039/d3sc06461a |
‡ These authors contributed equally to this work. |
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