Open Access Article
Mohmmad Faizan,
Zaid Malik,
Madem Sandhya and
Ravinder Pawar
*
Laboratory of Advanced Computation and Theory for Materials and Chemistry, Department of Chemistry, National Institute of Technology Warangal (NITW), Warangal, Telangana 506004, India. E-mail: ravinder_pawar@nitw.ac.in
First published on 5th December 2025
Frustrated Lewis pairs (FLPs) have emerged as versatile metal-free catalysts for small-molecule activation, and strategies to control frustration through geometric immobilization and electronic tuning remain a topic of significant interest. Carborane cages, with their unique coordination-dependent electronic effects, have recently been shown to modulate FLP frustration. In this work, we introduce o-silaborane cages, whose coordination-based electronic effects had not previously been explored for modulating FLP reactivity. The –BH2 and –PH2 substituents were strategically placed at distinct coordinating sites of the cages to systematically compare the coordination dichotomy of o-carborane and o-silaborane frameworks in influencing the frustration of Lewis pairs. CO2 activation was employed as the model reaction to assess and compare these effects. Electronic structure analysis reveals that silaborane exerts stronger electron-withdrawing and electron-donating influences than carborane, leading to pronounced differences in acidity–basicity balance, strain distribution, and the stability of CO2 complexes. Furthermore, transition-state energetics demonstrate that site-dependent positioning of Lewis acid–base centres critically governs activation barriers. In the o-carborane framework, the acid and base groups positioned at the 1,4-sites exhibit the highest reactivity, whereas in the o-silaborane system, the 4,9-substituted arrangement is identified as the most reactive. These findings establish silaborane as a promising bridging unit, opening new design pathways for tuneable FLP-based CO2 utilization and broader small-molecule activation.
In this context, o-carborane, a twelve-vertex icosahedral, neutral carbon–boron cluster (Fig. 1a), emerges as an exceptional bridging scaffold owing to its remarkable stability and coordination-dependent electronic properties, often described as coordination dichotomy.35–37 Since its first report in 1963,38,39 experimental studies have established o-carborane as an electron-deficient polyhedral cluster composed of triangular faces formed through three-centre–two-electron (3c–2e) bonds. The cage exhibits three-dimensional aromaticity arising from electron delocalization over the entire framework.40–43 Importantly, this delocalization is non-uniform, imparting distinct electron densities at different atomic sites and thereby generating position-dependent electronic effects within the cluster. The acidity or basicity of substituents attached to the carborane polyhedron is directly governed by the electron density at the specific carbon or boron site of attachment.43–46 The electron-density distribution in o-carborane follows the order C(1,2) < B(3,6) < B(4,5,7,11) < B(8,10) < B(9,12) (Fig. 1a), indicating that the cage carbon atoms exert strong electron-withdrawing effects, whereas the B9 and B12 vertices are strongly electron-donating.43–46 Consequently, borane substitution at cage carbon sites generates highly acidic centres,47 while phosphine substitution at boron sites antipodal to the carbon atoms yields strongly basic functionalities.48,49 These inductive effects of C- and B-bound carboranyl groups were quantitatively described using inductive constants derived from 19F NMR chemical-shift measurements of para- and meta-substituted fluorobenzenes by Taft method.43,50,51 This distinct variation in electronic influence positions o-carborane as a highly versatile bridging unit capable of modulating electronic effects solely through the choice of coordination site. Such tunability is particularly advantageous for FLP chemistry, where controlling the degree of frustration is essential. Therefore, o-carborane based intramolecular FLPs are anticipated to display frustration that is inherently governed by the cage's coordination-dependent electronic dichotomy. Welch and co-workers in 2019 reported the first base- and acid-functionalized o-carborane, 1-Bcat-7-PPh2-closo-1,7-C2B10H10, although it was not considered as an IFLP due to insufficient geometrical requirements for frustration.52 Subsequently, Xie and colleagues reported the first o-carborane IFLP, 1-PPh2-2-BPh2-1,2-C2B10H10, which was shown to catalyze tri-insertion and dearomatization of terminal arylalkynes.53 More recently, Zhu and co-workers theoretically investigated o-carborane-based IFLPs (o-IFLPs) for N2 activation.54 Despite these advances, the impact of coordination dichotomy on the degree of frustration in IFLPs has received relatively little attention. Building on these developments, we investigated o-IFLPs for CO2 activation (Fig. 1b).55 Furthermore, we demonstrated that the coordination dichotomy intrinsic to the carborane cage plays a decisive role in modulating the frustration and reactivity of the embedded Lewis pairs (Fig. 1c).56 Collectively, these results highlight o-carborane frameworks as powerful and tunable bridging units for controlling FLP reactivity.
Analogous to o-carborane, the icosahedral 12-vertex silicon–boron cluster, o-silaborane (Fig. 1a), was first reported and examined by Seyferth and co-workers.57,58 The reaction between CH3(H)Si(NMe2)2 and B10H14 yielded 1,2-dimethyl-1,2-disila-closo-dodecaborane (i.e., o-silaborane). The isolated o-silaborane exhibited chemical stability and did not react with Me3SiCl/AlCl3 or Me3SiCl/AlBr3 in either CH2Cl2 or CHCl3.57,58 It was similarly unresponsive toward HCl/AlCl3 and HCl/AlBr3. In contrast, treatment with ethanolic KOH led to rapid and complete decomposition of the silaborane.57,58
Beyond the parent 1,2-dimethyl-1,2-disila-closo-dodecaborane i.e., o-silaborane, a diverse family of derivatives has been reported. Substitution at the silicon vertices affords closo analogues such as the 1,2-diphenyl- and 1-methyl-2-phenyl-1,2-disila-closo-dodecaboranes, which retain the characteristic Si2B10 cage geometry.59 Controlled nucleophilic attack at the Si-localized LUMO leads to cage degradation, generating nido and closo silaborates including [nido-(MeSi)B10H12]− and [closo-(MeSi)B11H11]−, as well as related arachno-type products.60 The parent cluster also forms a variety of addition products such as amido-bridged species such as [(Et2N)(MeSi)2B10H10]− and corresponding Zr/Ta amido complexes;59 alkoxide and oxo-bridged adducts including [(TMPDAH)2((Me2Si2B10H10)2O)] and [TMPDAH][(Me2Si2B10H10)OMe].61 Collectively, these derivatives demonstrate the pronounced nucleophilicity and versatile reactivity imparted by the two adjacent silicon vertices, distinguishing o-silaborane chemistry from that of the isoelectronic o-carborane. Also, the He(I) photoelectron spectroscopic studies established that the o-silaborane cage is more electron rich than the corresponding carborane cage. This difference arises because the Si atom donates more electron density to the silaborane cage than the C atom donates in o-carborane, owing to the lower effective nuclear charge of Si relative to C. Consequently, the less electronegative Si atom transfers electron density more readily to the cage, making the boron atoms in o-silaborane more electron rich than those in the carborane cage, and correspondingly rendering Si more electron withdrawing than the cage carbon atoms of o-carborane. Thus, o-silaborane is expected to impart stronger electronic effects than o-carborane, and the frustration of silaborane-bridged Lewis pairs may differ from that of carborane-supported Lewis pairs. Moreover, to the best of our knowledge, the coordination-dependent electronic effects of o-silaborane remain unexplored and have not been correlated with those of carborane, particularly in the context of IFLP frustration. This gap provides an opportunity to examine the coordination dichotomy of o-silaborane and to evaluate its potential as a bridging unit for IFLPs.
The present study aims to comparatively investigate the coordination dichotomy of o-silaborane and o-carborane in modulating Lewis-pair frustration. To this end, –PH2 and –BH2 groups were introduced at different coordination sites of both cages to generate a series of IFLPs (Fig. 1d), which were subsequently analyzed for CO2 activation to determine how variations in coordination sites influence reactivity. The use of –PH2 and –BH2 substituents allows us to isolate the electronic influence of the cages on frustration without introducing additional steric or electronic contributions from the substituents themselves. Furthermore, for the most favourable coordination sites of both cages, the reactivity of –PH2/–B(CF3)2 and –P(CH3)2/–B(CF3)2 Lewis acid–base pairs was also examined. Overall, this study elucidates the coordination dichotomy of o-silaborane and assesses its suitability as a bridging scaffold for IFLPs, while laying the foundation for future work on catalytic CO2 conversion into value-added products.
To gain further insight into the differing reactivities of the studied IFLPs, the strain developed along the reaction pathway arising from structural distortion of the reactants and the evolution of interaction energies were analyzed. The strain energies in the CMs and TSs were calculated as follows:
| ΔEstrain (IFLP\_CM) = ECM-geomIFLP − EoptIFLP |
| ΔEstrain (IFLP\_TS) = ETS-geomIFLP – Eopt or CM-geomIFLP |
Here, ETS-geom and ECM-geom denote the single-point energies of the fragments in the geometries they adopt within the transition state and reactant complex, respectively, while Eopt refers to the energy of the fully optimized fragment in its equilibrium structure. The ΔEstrain (IFLP_CM), ΔEstrain (CO2_CM) represents the strain induced in the IFLP and CO2 in the CMs, while ΔEstrain (IFLP_TS), ΔEstrain (CO2_TS), indicates the strain induced in the IFLP and CO2 in the TSs. It is important to note that if a CM is more stable than the isolated reactants, the strain required to reach the TS is referenced from the CM geometries rather than the isolated fragments. The resulting strain–interaction energy profiles provide detailed insights into how different coordinating sites influence the reaction pathways, thereby revealing the impact of coordination dichotomy in carborane and silaborane cages on the frustration of the Lewis pairs.
| General structure of the o-carborane and o-silaborane cage | ||||
|---|---|---|---|---|
| Hydride ion affinity (kcal mol−1) | Proton ion affinity (kcal mol−1) | |||
| –BH2 + H− → [BH3]− | –PH2 + H+ → [PH3]+ | |||
| Coordinating sites | C | Si | C | Si |
| 1st | −93.96 | −120.29 | 16.64 | 23.02 |
| 3rd | −85.76 | −82.54 | 2.25 | −7.14 |
| 4th | −76.25 | −75.41 | −5.76 | −12.60 |
| 8th | −68.53 | −66.68 | −14.25 | −20.61 |
| 9th | −65.77 | −64.30 | −17.15 | −22.31 |
From Table 1, it is evident that moving from the 1st to the 9th coordinating site via the 3rd, 4th, and 8th positions, the HIA values become progressively less negative, signifying a decrease in acidity of the –BH2. This trend reflects the gradual increase in electron-donating character at these sites. Correspondingly, the PIA values increase (i.e., becomes more negative), indicating enhanced basicity of the –PH2 unit across the same sequence of positions. Importantly, both o-carborane and o-silaborane display a similar trend in the variation of acidity and basicity, though the magnitude of these effects differs markedly between the two systems. For example, the HIA of –BH2 at the 1st position in o-carborane is −93.96 kcal mol−1, whereas in o-silaborane it is significantly more negative (i.e., −120.29 kcal mol−1), highlighting the stronger electron-withdrawing effect of Si relative to C. Further, at the 3rd position, the HIA of –BH2 in o-carborane is ∼3 kcal mol−1 lower than in o-silaborane (see Table 1), indicating that the B atom at 3rd position in o-carborane is more electron withdrawing than the corresponding atom in o-silaborane. This electronic disparity is also reflected in the PIA values. The –PH2 unit at the 3rd coordinating site in o-carborane has a PIA of 2.25 kcal mol−1, compared to −7.14 kcal mol−1 in o-silaborane, indicating greater basicity in the latter. A similar trend is observed at the 4th, 8th, and 9th coordinating sites, where o-carborane consistently shows higher HIA values (more acidic –BH2) compared to o-silaborane.
Conversely, o-silaborane exhibits significantly more negative PIA values at these sites i.e., −12.60, −20.61, and −22.31 kcal mol−1, respectively, confirming its stronger electron-donating character relative to o-carborane. Thus, the comparative analysis of HIA and PIA values demonstrates that while both cages exhibit analogous electronic dichotomy, o-silaborane exerts more pronounced electron-withdrawing and electron-donating effects at 1st and 9th coordinating sites in comparison to the o-carborane. This distinction underscores the importance of examining how the coordination dichotomy of the silaborane cage influences the frustration of supported Lewis pairs. The distinct electronic behavior of the o-silaborane cage, as reflected in the HIA and PIA trends, is further supported by experimental photoelectron spectroscopic data. Seyferth and co-workers reported He(I) photoelectron spectra for 1,2-disila-closo-dodecaborane, which revealed that the silaborane cage possesses a notably more electron-rich valence framework than its carborane counterpart.57,58 This observation arises from the greater ability of silicon to donate electron density into the delocalized cage bonding network, owing to its lower effective nuclear charge and more diffuse valence orbitals relative to carbon. Consequently, while the cage as a whole becomes more electron rich, the Si atom itself becomes more electron deficient, thereby exerting a stronger inductive electron-withdrawing influence on substituents bound to it. The enhanced acidity of –BH2 and the deeper PIA values observed in o-silaborane at several coordinating positions align precisely with this experimental insight. Thus, the He(I) photoelectron spectrum not only validates the intrinsic electronic enrichment of the silaborane cage but also corroborates the stronger inductive modulation exerted by silicon, reinforcing the interpretation of the HIA/PIA trends discussed above.
To this end, various unique combinations of adjacent coordinating sites were considered for Lewis pair substitution, as illustrated in Fig. 1d. The coordinating sites for the –BH2 and –PH2 units were selected based on two criteria: (a) the sites must be adjacent, and (b) the electronic effect at these sites should favour either the acidic fragment (–BH2), the basic fragment (–PH2), or both. Initially, –BH2 was placed at the 1st position and –PH2 at the 2nd position, such that the electron-withdrawing effect at the 1st site enhanced the acidity of –BH2 while simultaneously reducing the basicity of –PH2. Subsequently, the –PH2 group was shifted to the 3rd and 4th positions, with –BH2 fixed at the 1st position, to improve the basicity of the –PH2 site. In another arrangement, –BH2 was moved from the 1st to the 4th and 12th positions, corresponding to the relocation of –PH2 to the 9th coordinating site. These substitutions collectively increased the basicity of –PH2 while decreasing the acidity of –BH2. Finally, the groups were positioned with –BH2 at the 3rd site and –PH2 at the 8th site, a configuration expected to impart moderate electronic effects on both acidic and basic centres. The IFLPs generated from these positional variations (see Fig. 1d) were fully optimised and analysed to assess the initial electronic influences of the coordinating sites.
Analysis of Fig. 2 shows that relocating the –PH2 unit from Y2 (Y = C, Si) in YPB1 to B3 and B4 in YPB2 and YPB3 results in a slight but noticeable decrease in the P–B bond distance, accompanied by an increase in the electron density (ρ) at the bond critical point (X) between the P and B atoms. For example, in CPB1 the P–B distance is 2.09 Å, which shortens to 2.07 Å in CPB2 and 2.06 Å in CPB3. Correspondingly, the electron density (ρ) at X increases from 0.0805 a.u. in CPB1 to 0.0875 and 0.0904 a.u. in CPB2 and CPB3, respectively. A similar trend in P–B distances and electron densities can be observed for the SiPBn (n = 1–3) systems. These observations indicate stronger P–B interactions upon relocating the –PH2 group to the B3 and B4 sites, consistent with the enhanced basicity of the –PH2 substituent at these positions, as reflected in the PIA values (see Table 1). It is further evident from Fig. 2 that silaborane-supported IFLPs exhibit shorter P–B distances and higher electron densities at X compared to their carborane-supported counterparts. For instance, the PB distance in SiPB1 was observed to be 2.02 Å which is 0.07 Å smaller than the PB distance in CPB1, also the ρ at Y in SiPB1 was found to be 0.0951 a. u. which is greater than in case of CPB1. Similar observation can also be made for SiPB2 and SiPB3 from Fig. 2. These observations can be attributed to the more pronounced electron-withdrawing and electron-donating effects at the 1st–4th positions of the silaborane cage relative to the carborane cage, as indicated by the HIA and PIA values discussed earlier.
Fig. 3 shows that in CPB4 and SiPB4, relocation of the –BH2 group from Y1 (Y = C, Si) to the B4 position, along with the corresponding shift of the –PH2 group to B9, leads to a decrease in electron density (ρ) at the X and an increase in the P–B distance relative to YPB3 (Y = C, Si). The repositioning of –PH2 to B9 enhances its basicity, as indicated by the PIA values (see Table 1). However, the transfer of –BH2 from C1/Si1 to B4 reduces its acidity, thereby diminishing its electron-accepting ability. This combination results in the elongation of the P–B bond and the reduction of ρ. Further relocation of –BH2 and –PH2 from B4 to B9 and from B9 to B12, respectively, forming CPB5, produces an additional increase in P–B distance and a further decrease in ρ. An even more pronounced effect is observed in SiPB5, which exhibits the longest P–B distance (3.57 Å) and the absence of a bond critical point between P and B atoms among all the IFLPs studied so far. This striking behaviour can be attributed to the strongly quenched acidity of the –BH2 group at the B4 position in SiPB5 compared to other cases. Finally, placement of the –BH2 and –PH2 groups at the second most electron-withdrawing and electron-donating positions, namely the 3rd and 8th sites of the cages, generates the IFLPs CPB6 and SiPB6. These systems exhibit moderate P–B bond distances of 2.07 and 2.04 Å and ρ of 0.0886 and 0.0913 a.u., respectively. Overall, the electronic structure analysis of the IFLPs provides an initial understanding of how coordination dichotomy influences the reactivity of the active site.
It also highlights differences in the extent of electronic effects between carborane and silaborane cages, consistent with the acidity and basicity trends reflected in the HIA and PIA values. The optimized geometries of the CMs formed through the interaction of CO2 with silaborane- and carborane-based IFLPs are depicted in Fig. 4 and Fig. S2 (SI), along with the zero-point corrected relative energies (ΔE, in kcal mol−1) and the key geometrical parameters. From the optimized structures shown in Fig. 4 and S2, it is evident that CO2 binding induces expansion of the P–B bond and an increase in the angle projected by the –PH2 and –BH2 groups on the silaborane and carborane cages. This structural distortion suggests that CO2 coordination introduces strain into the molecular system, which in turn governs the overall relative energies of the resulting CMs. Accordingly, strain–interaction profiles have been calculated and are presented in Fig. 4 and S2. For silaborane, in SiPB1CM the P–C and B–O distances and O–C–O bond angle were 3.92 Å, 2.39 Å, and 178.9°, respectively (see Fig. 4). The calculated interaction energy was −6.32 kcal mol−1, while the strain energy was 1.80 kcal mol−1. Since the interaction energy dominates the induced strain, a stable CM (SiPB1CM) is formed, with ΔE = –5.26 kcal mol−1. In SiPB2CM, the P–C and B–O distances and O–C–O angle were 3.44 Å, 2.06 Å, and 176.8°, respectively, which are smaller than in SiPB1CM. This contraction indicates stronger interaction between CO2 and the IFLP SiPB2, consistent with the enhanced basicity of the –PH2 group as suggested earlier by PIA values. The interaction energy was −9.92 kcal mol−1, more negative than in SiPB1CM. However, the strain developed in SiPB2CM was nearly 20 kcal mol−1 greater than in SiPB1CM (Fig. 4). Similarly, in SiPB3CM the P–C and B–O distances and the O–C–O angle decreased further, reflecting enhanced interaction, as supported by the calculated interaction energy of −11.89 kcal mol−1 (see Fig. 4).
In this case, however, the induced strain reached 28.58 kcal mol−1, higher than in SiPB2CM. For both SiPB2CM and SiPB3CM, the strain energy dominates the interaction energy, resulting in relatively unstable CMs with ΔE values of 11.02 kcal mol−1 and 16.34 kcal mol−1, respectively. It is noteworthy that the induced strain correlates with the extent of intramolecular –PH2⋯–BH2 interaction in SiPB1, SiPB2, and SiPB3, as indicated by the ρ values at the bond critical point (X). The order of strain energies (i.e., SiPB1CM < SiPB2CM < SiPB3CM) follows the trend in ρ values (i.e., SiPB1 < SiPB2 < SiPB3). Thus, higher ρ values imply stronger internal interactions, requiring proportionally higher energies to achieve the geometrical deformations necessary for CO2 binding. Further, in SiPB4CM, the interaction energy was −5.64 kcal mol−1 which is less negative than in SiPB3CM, while the induced strain was 5.81 kcal mol−1, nearly 23 kcal mol−1 lower than in SiPB3CM. The reduced interaction energy arises from diminished acidity of the –BH2 group, consistent with longer B–O and P–C distances and a larger O–C–O angle compared to SiPB3CM. The smaller strain is attributed to weaker –PH2⋯–BH2 interaction, as reflected in the lower ρ value.
Furthermore, in SiPB5CM, the induced strain was only 0.36 kcal mol−1, the smallest among all investigated systems. The absence of BCP (X) confirms negligible interaction between –PH2 and –BH2 units, justifying the minimal energy required to deform the structure for CO2 binding. The interaction energy was −4.95 kcal mol−1 which is less negative than in SiPB4CM, reflecting further reduced –BH2 acidity, as indicated by the longer P–C and B–O distances and the wider O–C–O angle. In both SiPB4CM and SiPB5CM, the interaction energy governs stability due to the low induced strain, yielding ΔE values of −0.39 and −3.70 kcal mol−1, respectively. In SiPB6CM, the strain energy was 8.28 kcal mol−1, higher than in SiPB4CM and SiPB5CM. This increase is attributed to the larger ρ value at BCP (X), indicating stronger –PH2⋯–BH2 interaction. The interaction energy was −5.68 kcal mol−1, more negative than in SiPB5CM, consistent with shorter P–C (3.47 Å) and B–O (2.48 Å) distances and a reduced O–C–O angle of 177.6°. In this case, strain dominates over the stabilizing interaction, producing a relatively unstable CM (SiPB6CM) with ΔE = 1.92 kcal mol−1.
Like in the case of SiPB1, the interaction of CO2 with CPB1 results in the formation of a CM (i.e., CPB1CM) with a ΔE value of −4.35 kcal mol−1 (see Fig. S2 in SI). The dominance of the interaction energy (−4.33 kcal mol−1) over the minute strain (0.21 kcal mol−1) developed in the structure accounts for the observed stability of CPB1CM. However, both the strain and interaction energies are smaller than those in SiPB1CM, thereby justifying the comparatively lower stability of CPB1CM with respect to SiPB1CM. In CPB2CM, a higher strain of 8.67 kcal mol−1 is induced upon interaction with CO2, while the calculated interaction energy amounts to −5.98 kcal mol−1 (Fig. S2). The strain developed in CPB2CM is significantly smaller than in its silaborane-supported analogue, SiPB2CM. This lower strain explains the reduced ΔE value of 2.29 kcal mol−1 for CPB2CM compared to SiPB2CM (Fig. S2). Unlike SiPB3CM, where both strain and interaction energies are larger than those in SiPB2CM due to the enhanced basicity, CPB3CM exhibits lower strain and interaction energies, with values of 5.41 kcal mol−1 and −5.27 kcal mol−1, respectively (see Fig. S2), both smaller than in CPB2CM despite the enhanced basicity of the –PH2 unit in CPB3CM.
To rationalise this apparent inconsistency, the electronic structures of the optimised geometries of CPB2CM and CPB3CM were critically analysed. It can be seen form Fig. 5 that in CPB2CM, the oxygen atom of CO2 interacts with the acidic hydrogen at C2. The ρ value at the corresponding BCP was measured to be 0.08812 a.u. In CPB3CM, however, the O atom interacts with the H at B3, yielding a ρ value of 0.06688 a.u., which is smaller than in CPB2CM, signifying a weaker interaction in CPB3CM. This variation is further supported by the O–H distances, which are 2.72 Å in CPB3CM compared to the shorter O–H distance observed in CPB2CM (Fig. 5). The interaction with the acidic hydrogen at C2 thus leads to slightly stronger interaction in CPB2CM. Consequently, the weaker interaction in CPB3CM induces smaller structural distortion, leading to reduced strain relative to CPB2CM and thereby justifying the higher stability of CPB3CM over CPB2CM.
![]() | ||
| Fig. 5 Optimized geometries of CPB2CM and CPB3CM signifying the interaction with the H atom at C2 and B3, respectively. (ρ is in a.u.). | ||
In CPB4CM and CPB5CM, both strain energies and interaction energies decrease due to the reduced acidity of the –BH2 unit and diminished interaction between the –PH2 and –BH2 groups. In these cases, the dominance of interaction energy over induced strain results in CMs with negative ΔE values (see Fig. S2), confirming their stability. Finally, in CPB6CM, the strain and interaction energies are 3.32 kcal mol−1 and −6.04 kcal mol−1, respectively, both greater than those observed in CPB4CM and CPB5CM (Fig. S2). This increase arises from the higher acidity of the –BH2 group and the stronger interaction between the –BH2 and –PH2 units, as indicated by the ρ value at X in CPB6CM (see Fig. 3). Overall, this analysis provides insight into how the coordination of the Lewis acid (LA) and Lewis base (LB) over the cages influences their mode of interaction with the CO2 molecule. These variations result in CMs with distinct energy profiles, which may in turn affect the course of the reaction.
To further investigate the activity, i.e., the extent of frustration, the transition states (TSs) along with their geometrical parameters, ΔE, and activation energies (Ea) were evaluated and are presented in Fig. 6, along with their corresponding strain–interaction energy profiles. It can be clearly seen from Fig. 6 that, in attaining the TS geometries from the reactant complexes, the P–B and B–O distances, the OCO bond angle, and the angles projected by the –PH2 and –BH2 groups on the cage become shorter than the corresponding parameters in the CMs. This signifies the increased interaction between CO2 and the IFLPs, as well as the enhanced strain in the molecular system. The Ea for CPB1TS was calculated to be 14.19 kcal mol−1, while the strain and interaction energies were found to be 38.20 and −29.31 kcal mol−1, respectively, in going from CPB1CM to CPB1TS. In contrast, SiPB1TS exhibited strain energy nearly 10 kcal mol−1 higher than CPB1TS, which accounts for its higher Ea of 18.97 kcal mol−1, despite having stronger interaction than CPB1TS. Further, in going from CPB1TS to CPB2TS, the induced strain was reduced by ∼3 kcal mol−1, accompanied by a slight decrease of nearly 1 kcal mol−1 in the interaction energy. The diminished strain in CPB2TS results in a lower Ea of 11.37 kcal mol−1 compared to CPB1TS. Likewise, in SiPB2TS the strain was ∼5 kcal mol−1 smaller than in SiPB1TS, justifying the smaller Ea of 15.33 kcal mol−1. However, this value still remains higher than the Ea of CPB2TS due to the greater strain in SiPB2TS. In the case of CPB3, the strain induced in achieving the TS geometry from CPB3CM was found to be 25.6 kcal mol−1, while the interaction energy was −18.79 kcal mol−1. The relatively lower strain developed in CPB3TS results in a reduced Ea of 7.79 kcal mol−1 compared to CPB2TS. Furthermore, the induced strain energies in CPB4TS, CPB5TS, and CPB6TS were observed to be 28.96, 31.16, and 27.32 kcal mol−1, respectively, with interaction energies of approximately −18.5 kcal mol−1 in all cases.
Consequently, the Ea values for CPB4TS, CPB5TS, and CPB6TS were 11.10, 13.19, and 9.06 kcal mol−1, respectively, following the same order as the induced strain. Having nearly identical interaction energies, the activation barriers in these cases are controlled primarily by the strain induced in the structures. Unlike CPB3TS, SiPB3TS exhibits a strain energy of 44.15 kcal mol−1, which is considerably higher than that in SiPB2TS, resulting in an Ea of 18.67 kcal mol−1, greater than that of SiPB2TS. In the subsequent case of SiPB4TS, the Ea was found to be nearly half of that in SiPB3TS. This decrease can be attributed to the lower strain energy of 24.64 kcal mol−1 in SiPB4TS, which is also approximately half of that in SiPB3TS. It is noteworthy that SiPB4TS has a lower Ea than its carborane-based analogue, CPB4TS, again due to smaller induced strain in the former (see Fig. 6). For SiPB5TS, the induced strain was 29.53 kcal mol−1, greater than in SiPB4TS, leading to an Ea of 12.89 kcal mol−1, which is higher than in SiPB4TS. Interestingly, SiPB6TS displayed a strain energy of 31.95 kcal mol−1, greater than in SiPB5TS. Despite this higher strain, the calculated Ea was 10.33 kcal mol−1, which is lower than in SiPB5TS (see Fig. 6). This reduced barrier can be attributed to the stronger interaction in SiPB6TS, reflected in the more negative interaction energy of −21.82 kcal mol−1 compared to SiPB5TS. The overall energetic analysis, based on the strain and interaction energies developed in achieving the TS states via the CMs, provides a clear understanding of how the positions of the LA and LB units affect the overall energetics of the reaction. Different coordinating sites not only modulate the acidity and basicity of the active centers but also influence the structural deformations that dictate the reaction profile.
To finally conclude the effect of coordination dichotomy, the relative stabilities of the CO2 adducts were calculated. The optimized geometries of the formed CO2 adducts (ADs) with carborane and silaborane IFLPs are shown in Fig. 7, along with the geometrical parameters and the corresponding strain–interaction energy profiles. The zero-point corrected relative energies of the adducts are also given in the Figure. It is evident from the comparative analysis of the geometrical parameters of CMs, TSs and ADs presented in Fig. 4, 6 and 7 that the CO2 adducts possess the smallest geometrical parameters, indicating the strongest interaction between CO2 and the IFLPs and the highest strain developed in the molecular structures. It can be seen in Fig. 7 that the ΔE for CPB1AD is 8.77 kcal mol−1, while for CPB2AD and CPB3AD the values are 5.45 and 0.42 kcal mol−1, respectively. This clearly shows that the relative energy decreases when the –PH2 group is shifted from C2 to B3 and C4 due to the enhanced basicity of the –PH2 and thereby strengthens the interaction with CO2. This enhancement is also reflected in the interaction energies calculated for CPB1AD, CPB2AD, and CPB3AD, which are −66.13, −85.18, and −88.67 kcal mol−1, respectively.
Notably, the strain induced in CPB2AD and CPB3AD (88.42 and 87.09 kcal mol−1) is higher than in CPB1AD (73.01 kcal mol−1) (see Fig. 7), but the stronger interactions stabilize these adducts. In CPB4AD, ΔE increases to 1.87 kcal mol−1, higher than in CPB3AD, which can be attributed to the reduced interaction energy (−78.73 kcal mol−1). Similarly, CPB5AD exhibits a ΔE of 4.75 kcal mol−1 which is greater than CPB4AD, again due to a further decrease in interaction energy. Finally, CPB6AD, with a ΔE of 1.45 kcal mol−1 was found to be more stable than CPB5AD owing to enhanced interaction energy, despite the higher strain observed (Fig. 7). From the ΔE values in Fig. 7, it is also clear that all silaborane-supported CO2 adducts are less stable than their carborane counterparts except SiPB2AD, as their ΔE values are consistently higher. The stability pattern observed in CPB1AD to CPB2AD is reflected in SiPB1AD to SiPB2AD. Specifically, the ΔE values decrease from 12.96 to 4.10 kcal mol−1, which can be explained by the significant increase in interaction energy from −73.50 to −107.70 kcal mol−1, despite higher strain. In contrast, SiPB3AD shows a 0.50 kcal mol−1 increase in ΔE due to the rise in strain energy from 109.88 to 114.99 kcal mol−1.
Interestingly, SiPB4AD is relatively the most stable among silaborane adducts, with a ΔE of 2.76 kcal mol−1, owing to its much lower strain energy (85.75 kcal mol−1) compared to SiPB3AD (Fig. 7). For SiPB5AD and SiPB6AD, the ΔE values are 5.87 and 3.64 kcal mol−1, respectively, following a similar trend to their carborane analogues. Thus, the analysis of adducts provides a comprehensive understanding of how the coordination dichotomy in carborane and silaborane frameworks influences the stability of the formed CO2 adducts. Overall, silaborane-based IFLPs show their lowest activation barrier and most stable CO2 adduct in SiPB4, while among the o-carborane-supported IFLPs, CPB3 exhibits both the lowest activation barrier and the most stable adduct. This highlights the distinct electronic effects of carborane and silaborane cages on the LA–LB pair, which ultimately dictate their reactivity.
Additional analyses were carried out to assess the influence of more realistic substituents and alternative small-molecule activation pathways. Substituted IFLPs incorporating –PH2/B(CF3)2 and –PMe2/B(CF3)2 pairs were examined at the most reactive coordination sites (CPB3 for o-carborane and SiPB4 for o-silaborane). The computed CO2 activation barriers for these substituted systems remain comparable to those of the corresponding unsubstituted IFLPs, consistent with the idea that the intrinsic cage-induced electronic effects dominate the reactivity trends. Furthermore, to determine whether the observed patterns are general beyond CO2 activation, H2 activation was also investigated across the same series. Both substrates follow parallel trends in CM energies, activation barriers, and adduct stabilities, with CPB3 emerging as the most effective scaffold in each case. These results collectively confirm that the conclusions drawn from CO2 activation are robust and extend across different substituents and activation pathways. Full computational details, comparative energetics, and optimized structures are provided in the SI.
Overall, this study establishes silaborane as a promising and stable bridging scaffold for tuning the frustration of Lewis pairs, offering electronic control distinct from that of carborane. These insights pave the way for the rational design of next-generation metal-free catalysts for CO2 activation and other small-molecule transformations.
C Activation and CO2 Fixation, Angew. Chem., Int. Ed., 2011, 50, 3925–3928 CrossRef CAS PubMed.| This journal is © The Royal Society of Chemistry 2026 |