Yangbo Zhang and
Qingyun Wan*
Department of Chemistry, The Chinese University of Hong Kong, Shatin, Hong Kong SAR, China. E-mail: qingyunwan@cuhk.edu.hk
First published on 25th June 2025
Metal–metal (M–M) closed-shell interaction, also known as metallophilicity, is frequently observed in d10 and d8 metal complexes featuring a close M–M distance. It has shown a significant impact on diverse chemical systems, influencing structural, catalytic, and photophysical properties. The strength of both M–M interactions and the resulting M–M distances is highly dependent on various types of coordinating ligands. Recent studies have revealed that metallophilicity is repulsive in nature due to strong M–M Pauli repulsion (Q. Wan, J. Yang, W.-P. To and C.-M. Che, Strong metal–metal Pauli repulsion leads to repulsive metallophilicity in closed-shell d8 and d10 organometallic complexes, Proc. Natl. Acad. Sci. U. S. A., 2021, 118, e2019265118). However, little is known about the role of ligands in M–M repulsions. Here, we elucidate how metal–ligand (M–L) coordination modulates M–M repulsion through two key mechanisms: π-backbonding and σ-donor interactions. By systematically evaluating ligands spanning a spectrum of π-accepting and σ-donating strengths, we uncover opposing ligand effects. Strong π-backbonding weakens M–M Pauli repulsion, enabling shorter intermetallic distances, whereas the σ-donating interaction increases the repulsion, lengthening M–M contacts. These computational insights establish a ligand-design framework for tuning metallophilicity in closed-shell metal complexes and advance the fundamental understanding of M–M interactions from the perspective of M–L coordination.
While the repulsive nature of metallophilicity has been revealed, the role of ligands in modulating this repulsion remains a critical unresolved question. Ligands are well known to exert dramatic control over M–M distances: for instance, Au(I) complexes exhibit Au–Au separations spanning from non-interacting (>3.8 Å) to significantly shorter than the sum of van der Waals radii (∼2.5 Å), depending on the ligand identity, as summarized in several comprehensive reviews.3,5 Such variability highlights the dual capacity of ligands to either amplify or mitigate repulsive M–M interactions, yet the mechanistic origins of this modulation remain poorly defined. In this work, we address this gap by systematically dissecting how σ-donor and π-acceptor ligands tune M–M Pauli repulsion (Scheme 1).
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Scheme 1 Top: previous work, repulsive M–M interaction in closed-shell d8 and d10 transition metal complexes. Bottom: this work, the role of π-acceptor and σ-donor ligands in M–M interactions. |
Transition metal atoms can coordinate with a wide range of ligands, which are broadly categorized as π-acceptors, π-donors or σ-donors (Scheme 1).40 π-Acceptor ligands, such as CO and nitriles (R–CN), feature low-energy π* orbitals that accept electron density from filled metal d-orbitals, enabling π-backbonding interactions. In contrast, strong σ-donor ligands like cyanide (CN−) and alkynides (R–C
C−) coordinate through lone pairs, donating electron density to vacant metal orbitals (d/s/p). These contrasting bonding mechanisms exert striking effects on metallophilicity: structural studies reveal that π-acceptors promote shortened M–M distances, while σ-donors favour elongation, as shown in Fig. 1 and 7.3,5
Here, we bridge this gap through computational investigation of ligand-mediated M–M interactions. By utilizing energy decomposition analysis (EDA) and natural orbital for chemical valence (NOCV) methods, we demonstrate that π-backbonding interactions delocalize electron density from metal centers to ligand π* orbitals, attenuating M–M Pauli repulsion and enabling closer M–M contacts. Conversely, strong σ-donor ligands enhance metal (n + 1)s-nd hybridization, intensifying Pauli repulsion and elongating M–M distances. These insights explain well the experimental structural trends shown in Fig. 1 and 7. Our findings not only resolve longstanding ambiguities in ligand–metallophilicity relationships but also establish ligand-design principles to tailor M–M interactions in functional materials for supramolecular assembly, catalysis, and optoelectronic applications.
• Rh(terpy)Cl (Rh-1)41 vs. [Rh(terpy)NCCH3]+ (Rh-2)42
• Rh(CO)2ClNH2CH3 (Rh-3)43 vs. [Rh(CO)2(NCCH3)2]+ (Rh-4).44
Here, Rh-2 and Rh-4 incorporate π-acceptor ligands (acetonitrile), while Rh-1 and Rh-3 lack such ligands. Notably, aside from Cl− and NCCH3, both Rh-1 and Rh-2 coordinate to the same terpyridine (terpy) ligand; aside from Cl−/NH2CH3 and N
CCH3, both Rh-3 and Rh-4 coordinate to the same CO ligand. These comparisons exclude the potential influence of other ligand effects such as London dispersion and so on. As shown in Fig. 1, key structural trends emerged in the structural comparison: replacing the Cl− ligand in Rh-1 with the π-acceptor ligand CH3C
N (Rh-2) shortened the Rh–Rh distance from 4.90 Å (Rh-1) to 3.07 Å (Rh-2). Substituting the Cl− and NH2CH3 ligands in Rh-3 with CH3C
N ligands in Rh-4 reduced the Rh–Rh distance from 3.39–3.41 Å (Rh-3) to 3.15–3.18 Å (Rh-4). These results demonstrate that coordination of π-acceptor ligand is closely related to the short M–M distances observed in the crystal structures of d8 Rh(I) complexes.
The M–M distance trend observed in X-ray crystal structures was further validated through computational optimization of dimeric structures, thereby excluding contributions from the crystal packing effect. As shown in Fig. 1c, the optimized structures retain the key experimental trends (Fig. 1a and b): Rh complexes with π-acceptor ligands exhibit shorter Rh–Rh distances than analogues without such ligands (Rh-1 vs. Rh-2; Rh-3 vs. Rh-4). Notably, both optimized configurations of the [Rh-1]2 dimer shown in Fig. 1c maintain longer Rh–Rh distances than those of [Rh-2]2. This consistency between solution-phase calculations and solid-state structural data indicates that the observed distance variations are primarily driven by ligand electronic properties rather than crystal packing or solvent effects.
For d8–d8 closed-shell systems, the role of π-acceptor ligands in reducing M–M Pauli repulsion can be rationalized through an illustrative molecular orbital (MO) diagram shown in Scheme 2. First, we need to consider the ligand field splitting diagram of a metal with a d8 electronic configuration.40 As shown in Scheme 2, for a d8 metal complex (e.g., Rh(I), Ir(I), Pt(II), or Pd(II)) with square planar coordination geometry, dx2−y2 is a strongly antibonding orbital with respect to M–L interactions and remains unoccupied, while dz2 is a weakly antibonding orbital and remains occupied.40 The remaining three orbitals (dxz, dxy and dyz) are degenerate, non-bonding and occupied M–L orbitals.40
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Scheme 2 Schematic illustration of the role of the π-acceptor ligand in weakening the M–M Pauli repulsion for d8–d8 closed-shell metal complexes. Schematic illustration of the MO for d10–d10 closed-shell metal complexes has been provided in the ESI.† |
Next, we need to derive the formation of M–M bonding and antibonding orbitals from the occupied d orbitals of two d8 metal atoms.40 Defining the M–M bond axis as the z-axis, then the two dz2 orbitals can overlap in a σ-type manner to form a bonding σ orbital and an antibonding σ* orbital (Scheme 2). Similarly, the dxz and dyz orbitals can overlap with another set of dxz and dyz orbitals in a π-fashion, forming two degenerate bonding π orbitals and two degenerate antibonding π* orbitals. Since the π orbital overlap is smaller than the σ overlap, the energy splitting between the bonding and antibonding π orbitals is smaller than that between the bonding and antibonding σ orbitals. Furthermore, the dxy orbital can overlap with another dxy orbital in a δ-type manner, resulting in bonding δ orbitals and antibonding δ* orbitals. The δ orbital overlap is even smaller than the π overlap, leading to an energy splitting between the bonding δ and the antibonding δ* orbitals that is smaller than those for the π and π* orbitals, as illustrated in Scheme 2.
In Scheme 2, the M–M bonding orbitals—comprising one σ, two π, and one δ orbital—along with the corresponding antibonding orbitals (one σ*, two π*, and one δ*), are fully occupied. As demonstrated in our previous work on Rh(I), Pt(II) and Pd(II) systems, the closed-shell electronic configuration of two d8 metals with planar coordination geometry results in strong M–M Pauli repulsion, the magnitude of which is reflected in the energy splitting between the occupied M–M bonding and antibonding orbitals.36,37
The M–L coordination bond plays a critical role in determining both the energy levels and electron density distribution of the metal d orbitals.40 This, in turn, modulates the extent of M–M orbital overlap, thereby influencing the magnitude of M–M Pauli repulsion and the resulting M–M distances observed in the crystal structures of these complexes. Among various types of M–L coordination bonds, π-backbonding is a particularly important interaction in transition metal complexes. This interaction typically occurs when a ligand, such as carbon monoxide, accepts electron density from the metal through the overlap of a metal d orbital and a ligand π* orbital. This process, termed “back-bonding,” stabilizes the metal's d orbitals as the ligand acts as a π-acceptor. Consequently, M–M π and π* orbitals are stabilized, as illustrated in Scheme 2. Since M–M Pauli repulsion is positively correlated with the degree of overlap between two occupied d orbitals,45,46 it is expected that the presence of π-acceptor ligands weakens M–M Pauli repulsion arising from π-type interactions, leading to shorter M–M distances.
To computationally prove the speculation illustrated in Scheme 2, we performed Energy Decomposition Analysis (EDA),47–49 Natural Orbitals for Chemical Valence (NOCV) analysis, molecular orbital (MO) diagram calculations, and high-level Domain-based Local Pair Natural Orbital Coupled Cluster with Singles, Doubles, and perturbative Triples (DLPNO-CCSD(T)) computations on Rh complexes, using the AMS (Amsterdam Modeling Suite) 2024.150,51 and ORCA 6.0 package.52,53
We first examined the formation of π-backbonding interactions between the metal and the ligand in complexes Rh-1 and Rh-2. EDA-NOCV54 analysis decomposes electron density changes into chemically understandable components using fragment molecular orbitals. Herein, the energetic quantification of M–L π interactions was calculated for the Rh–Cl bonds in the optimized Rh-1 monomer and the Rh–N bonds in the optimized Rh-2 monomer. The NOCV deformation density channels are depicted in Fig. 2 with the red and blue regions symbolizing the depletion and accumulation of electron density, respectively. One NOCV deformation density channel corresponding to Rh–Cl π-bonds shows electron transfer from the Rh atom to the Cl atom, with an orbital energy of −2.34 kcal mol−1 of Rh-1. Similarly, one NOCV deformation density channel, representing Rh–N π-bonds, exhibits electron transfer from the Rh atom to the N atom, with a stronger orbital energy of −8.99 kcal mol−1 of Rh-2.
The difference in the energy of NOCV calculations between Rh-1 and Rh-2 indicates different π-accepting abilities between –Cl− and the –NCCH3 ligand. For the N
CCH3 ligand, the N atom forms a triple bond with the C atom, consisting of one σ bond and two π bonds. The two empty π* orbitals in the N
CCH3 ligand lie at relatively low energy, enabling efficient acceptance of d electron density from the Rh atom. The NOCV analysis suggests that stronger π-backbonding interaction occurs in Rh-2, leading to a reduction in the d orbital's electron density in Rh-2 compared to Rh-1. This is expected to reduce the dπ–dπ* orbital splitting energy and weaken the M–M Pauli repulsion in the Rh-2 dimer compared to the Rh-1 dimer. Next, we conducted MO calculations on the Rh-1 and Rh-2 dimers to validate this hypothesis.
Based on this consideration, we examined and compared the dπ–dπ* orbital splitting energy in the optimized Rh-1 and Rh-2 dimers using MO calculations. As shown in Fig. 3, the orbital splitting energy between the M–M π(dxz–dxz) bonding orbital and the π*(dxz–dxz) antibonding orbital was calculated to be 0.408 eV in Rh-1 and 0.393 eV in Rh-2. The orbital splitting energy for M–M π-type interactions between the two Rh atoms is consistently smaller in Rh-2 than that in Rh-1. In comparison to the Rh-1 dimer, we expect that the smaller dπ–dπ* orbital energy splitting in the Rh-2 dimer would lead to decreased M–M Pauli repulsion.36,37 Finally, we calculated the M–M Pauli repulsion in the Rh-1 and Rh-2 dimers to prove this relationship.
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Fig. 3 Calculated MO diagram for the Rh-1 dimer (left) and the Rh-2 dimer (right), highlighting the dπ bonding and dπ* antibonding orbitals. Isovalue = 0.03. |
M–M Pauli repulsion for the Rh-1 and Rh-2 dimers has been calculated using the EDA method, and the results are plotted in Fig. 4. In the calculations, the M–M distance in the Rh(I) dimers 1 and 2 was set from 3.3 Å to 2.9 Å, to compare the M–M Pauli repulsion at equal M–M distances. As shown in Fig. 4a, Rh–Rh Pauli repulsion increased with the decrease of the Rh–Rh distance in both the Rh-1 and Rh-2 dimers, and the M–M Pauli repulsion in the Rh-1 dimer is always stronger than that in the Rh-2 dimer. For instance, at an Rh–Rh distance of 3.0 Å, the M–M Pauli repulsion was 32.60 kcal mol−1 in the Rh-1 dimer, compared to 29.82 kcal mol−1 in the Rh-2 dimer, representing a 2.78 kcal mol−1 reduction. This calculated trend in M–M Pauli repulsion for Rh-1 and Rh-2 aligns with the trend observed in the M–M distances from their respective X-ray crystal structures (Fig. 1). The trend in Rh–Rh Pauli repulsion has been further validated through DLPNO-CCSD(T) calculations, which confirm that the Rh-2 complex—featuring the π-accepting CH3CN ligand—exhibits weaker metal–metal Pauli repulsion than Rh-1 (Fig. S1†).
The results of EDA, NOCV and MO calculations demonstrate a mechanistic pathway: the ligand's π-accepting ability directly influences the M–M dπ–dπ* orbital splitting energy, which in turn determines the magnitude of M–M Pauli repulsion. To summarize, coordination to π-acceptor ligands decreases the dπ–dπ*(M–M) orbital splitting and weakens M–M Pauli repulsion, facilitating the formation of close M–M contact in the Rh-2 complex compared to Rh-1.
Similarly, NOCV calculations were performed on the Rh-3 and Rh-4 monomers, revealing total Rh → L π-bonding interactions of −17.42 and −18.99 kcal mol−1, respectively (Fig. S2†). At every M–M distance in Fig. 4b, stronger M–M Pauli repulsion is observed in the Rh-3 dimer (with Cl−/NH2CH3 ligands) than in the Rh-4 dimer (with π-acceptor NCCH3 ligands). The NOCV and EDA results suggest that the stronger π-backbonding interaction in Rh-4 contributes to weaker M–M Pauli repulsion, and consequently, a shorter M–M distance in Rh-4 (3.15–3.18 Å) than in Rh-3 (3.39–3.41 Å) shown in Fig. 1.
In addition to the Rh(I) d8 systems, the relationship between the d10–d10 Pauli repulsion and the π acceptor ligand is demonstrated in the MO diagram of Scheme S1.† Different from the d8 closed-shell metal atom with four fully occupied metal d orbitals, the d10 metal atom has five fully occupied d orbitals.40 These d orbitals, when interacting between two metal atoms, contribute to one σ-type bonding and antibonding orbital, two π-type bonding and antibonding orbitals, and two δ-type bonding and antibonding orbitals. Similarly, the formation of π-backbonding interactions between the d10 metal atom and the ligand stabilizes the M–M π-type bonding and antibonding orbitals, leading to weakened M–M Pauli repulsion in d10–d10 metal complex systems (Scheme S1†).
To further validate the relationship between ligand π-accepting ability and M–M Pauli repulsion, we systematically evaluated diverse ligands (L = NH3, PH3, CO, NCCH3, CNCH3, CCCH3, CN, Cl, Br, I) in [Rh(terpy)L]2 dimers (model system). Following structural optimization, we correlated M–M distances with three parameters: molecular volume (reflecting steric effects), ligand–ligand (L–L) dispersion interactions, and M–M Pauli repulsion energy. In Fig. 5, M–M distances show no clear correlation with the molecular volume or L–L dispersion but exhibit a positive correlation with both M–M Pauli repulsion energy and ligand π-accepting strength (Fig. 5, 6 and Table S1†). As shown in Fig. 5, increasing M–M distances in [Rh(terpy)L]2 dimers (L = CO → Cl−) correlate with progressively stronger M–M Pauli repulsion. Correspondingly, enhanced Pauli repulsion occurs concomitantly with weakened Rh → L π-interactions, as evidenced by the EDA-NOCV analysis in Fig. 6. This absence of steric/L–L dispersion correlations, coupled with electronic dependence, provides evidence that ligand π-accepting capability primarily governs M–M distances through Pauli repulsion modulation.
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Fig. 5 Model system [Rh(terpy)L]2 and correlation analysis. Chemical structures of the [Rh(terpy)L]2 dimer (top) with the corresponding plots of the molecular volume, L–L dispersion interaction, and M–M Pauli repulsion versus the M–M distance in the fully optimized geometries (bottom). All data points are tabulated in Table S1.† |
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Fig. 6 Calculated EDA-NOCV deformation orbital energies correspond to the Rh → L π interaction in the model system of Rh(terpy)L. All data points are tabulated in Table S1.† |
Notably, for relatively large ligands, steric or dispersion effects could potentially dominate.33 For instance, the dispersion interactions and softness of ligand fragments have previously been reported to govern intermolecular interactions in the Rh(I) and Au(I) closed-shell systems, while the metals play a relatively minor role.32–34,55,56 The magnitude of ligand–ligand (L–L) dispersion interactions strongly depends on the ligand size.33,34 Furthermore, recent studies demonstrate that ligand–metal interplay critically influences non-covalent interactions.55,57 However, within the scope of this work—focused on investigating the electronic tuning effects via ligands—our analyses confirm that the observed M–M distance trends are linked to the π-accepting ligand modulation ability of M–M Pauli repulsion in smaller ligand systems.
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Fig. 7 Chemical structures of (a) Au(I) and (c) Pt(II) metal complexes, together with the experimentally resolved M–M distance in their crystal structures. Note: for Au-1 and Au-2, the Au–Au distance is different when changing the countercation.5 We compared Au-1 and Au-2 with the same countercation here: nBu4N[Au-1]: d(Au–Au) = 3.0700 Å, K[Au-1]: d(Au–Au) = 3.0064/3.0430 Å. K[Au-2]: d(Au–Au) = 3.64 Å, nBu4N[Au-2]: no close Au–Au contact. Optimized structures of (b) Au(I) and (d) Pt(II) metal complexes. Calculations were performed at the PBE0-GD3BJ/SDD(Au, Pt)/6-31G* (other elements) level of theory using the PCM solvent model for ACN in Gaussian 16. |
The M–M distance trend observed in X-ray crystal structures was validated through computational optimization of the dimeric species. As shown in Fig. 7b and d, optimized structures replicate key experimental trends from Fig. 7a and c: [Au-1]2 exhibits shorter Au–Au distances than [Au-2]2, and [Pt-1]2 shows reduced Pt–Pt distances compared to [Pt-2]2. This consistency between computational and crystallographic data confirms that the observed variations originate from intrinsic electronic properties rather than crystal packing effects.
For the σ-bonding interaction between a metal and a ligand, the ligand donates electron density to the metal's empty d or s orbital through σ-type M–L interaction, which influences the composition, energy, and electron density distribution of metal orbitals. The role of strong σ-donor ligands in strengthening the M–M Pauli repulsion for d8–d8 and d10–d10 closed-shell systems is shown in Scheme S2† and Fig. 8a, respectively.
For the d10 metal complexes such as Au(I), Ag(I), or Cu(I), (n + 1)s-nd orbital hybridization plays a critical role in the formation of M–L σ-type coordination bonds (n = 3 for Cu(I), 4 for Ag(I) and 5 for Au(I)).36,37 As shown in Fig. 8a, part of the empty (n + 1)s orbitals are used to accept electron density from σ-donor ligands. Defining the M–L bond direction as the z-axis, the (n + 1)s-nd orbital hybridization reduces the metal orbital's lobe size along the z-axis while increasing its size in the xy-plane.40 When two metal atoms approach each other in the xy-plane, their sd-hybridized orbitals overlap, resulting in the formation of a bonding σ(M–M) orbital and an antibonding σ(M–M)* orbital.36,37 Coordination with a stronger σ-donor ligand enhances the extent of (n + 1)s orbital hybridization. This, in turn, increases the metal's electron density in the xy plane, resulting in greater orbital splitting and stronger M–M Pauli repulsion.
To validate the schematic diagram plotted in Fig. 8a, we conducted MO calculations on Au-1 and Au-2 dimers (Fig. 8b). Because of the stronger σ-donor ligand CN− in Au-2, a greater contribution from the Au-6s orbital was observed in its 6s–5d hybridized orbital (49% in Au-2 vs. 36% in Au-1). The increased Au-6s orbital contribution enlarges the metal orbital's lobe size in the xy plane, thereby increasing the orbital splitting energy in the Au-2 dimer compared to the Au-1 dimer. As shown in Fig. 8b, the orbital splitting energy between the M–M σ(6s–5d) bonding orbital and the M–M σ*(6s–5d) antibonding orbital is calculated to be 0.739 eV in [Au-1]2 and 1.218 eV in [Au-2]2. This larger orbital splitting energy in [Au-2]2 indicates stronger Au–Au Pauli repulsion in [Au-2]2 compared to that in [Au-1]2.
We next performed EDA calculations on the Au-1 and Au-2 dimers (Fig. 9). In the calculations, M–M distances in these Au(I) dimers were set from 3.3 Å to 2.9 Å to compare the M–M Pauli repulsion at equal M–M distances. Au–Au Pauli repulsion increased with the decrease of the Au–Au distance for both Au-1 and Au-2 dimers, and the M–M Pauli repulsion in the Au-1 dimer is always stronger than that in the Au-2 dimer. For example, at an Au–Au distance of 3.0 Å, the M–M Pauli repulsion is 27.7 kcal mol−1 in the Au-1 dimer, while it is 24.2 kcal mol−1 in the Au-2 dimer. Relaxation density (defined as the electron density difference between the metal atom after ligand coordination and its pre-coordination state) of Mulliken population on the metal's s-orbitals (Δs) was examined to further characterize the ligand's σ-donating ability for complexes Au-1 and Au-2. The calculated trend of M–M Pauli repulsion in Au-1 and Au-2 is consistent with the calculated relaxation density. Specifically, Au-2 exhibits a larger 6s-orbital relaxation density (Δs = 0.9073) with the CN− ligand than Au-1 exhibits with the SCN− ligand (Δs = 0.8455), indicating that the CN− ligand donates more electron density to the Au-6s orbital. To summarize, coordination to strong σ-donor ligands increases the dσ(M–M)-dσ*(M–M) orbital splitting and strengthens the M–M Pauli repulsion, preventing the formation of close M–M contact in the Au-2 complex compared to Au-1.
Let us now consider the role of σ-bonding interaction in d8–d8 systems. As previously noted, in square-planar d8 metal complexes, the ndx2−y2 orbital is unoccupied and strongly antibonding regarding the M–L coordination.37 This orbital does not contribute to M–M Pauli repulsion. In contrast, the ndz2 weakly antibonding orbital is fully occupied and significantly contributes to M–M Pauli repulsion through the M–M σ-type interaction (Scheme 2 and S2†).33 Importantly, the ndz2 orbital can accept the ligand's electron density by the hybridization with higher empty metal-(n + 1)s orbitals to weaken the M–L antibonding interaction (n = 4 for Rh(I) and Pd(II), n = 5 for Ir(I) and Pt(II)). The relative component of the hybridized (n + 1)s orbitals is closely related to the σ-donating ability of ligands, similar to d10–d10 systems. We compared the Pt-6s orbital's population in Pt-1 and Pt-2, where the Pt-1 complex has one strong σ-donor C− ligand and the Pt-2 complex has two strong σ-donor C− ligands.
As shown in Scheme S2,† more Pt-6s orbital's components show up in the Pt-5dz2 orbital for Pt-2 (23%) than in Pt-1 (20%). In the calculated Mulliken population, Pt-2 also has more Pt-6s orbital's relaxation density than Pt-1 after ligand coordination (Δs = 0.1151 in Pt-2 vs. 0.0001 in Pt-1). The increased electron density in the Pt-6s orbital of the Pt-2 complex compared to Pt-1 is expected to amplify the Pt–Pt Pauli repulsion, which consequently elongates the Pt–Pt bond distance.
Next, we calculated and compared the M–M Pauli repulsion in Pt-1 and Pt-2 dimers (Fig. 10). M–M distances in the Pt(II) dimers were set from 3.5 Å to 3.1 Å for the comparison of M–M Pauli repulsion at equal M–M distances. As revealed in Fig. 10, the M–M Pauli repulsion in the Pt-2 dimer is always stronger than that in the Pt-1 dimer, which is consistent with the electronic configuration calculations.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d5qi01270h |
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