Pandiselvi
Durairaj
,
Sonia
Das
and
Sunandan
Sarkar
*
Department of Chemistry, National Institute of Technology, Tiruchirappalli, Tamil Nadu 620015, India. E-mail: ssarkar@nitt.edu
First published on 28th October 2025
Spin–orbit coupling (SOC)-assisted intersystem crossing (ISC) plays a pivotal role in designing metal-free organic systems for optoelectronic applications. We computationally designed a new structural motif, i.e., 12-bromo-1-azaperylene (12-BAP), which incorporates three crucial factors that promote rapid ISC: a change in state character during singlet–triplet conversion (1ππ* → 3nπ*), a pronounced heavy atom effect (HAE), and a favourable energy alignment between the 1ππ* and 3nπ* states. Notably, the close spatial positioning of the heavy Br atom near the site of orbital angular momentum change intensifies the HAE. As a result, a strong SOC (89 cm−1) between the 1ππ* and 3nπ* states drives ultrafast ISC (1012 s−1). In contrast, azaperylene and its 12-hydroxy derivatives exhibit limited ISC efficiency owing to the higher energetic position of the 3nπ* state. Br substitution at the 12-position of 1-azaperylene yields the highest SOC and fastest ISC among all Br-substituted variants. Efficient triplet-state generation is crucial for the development of high-performance organic phosphorescent emitters and photodynamic therapeutic agents. The 12-BAP motif promotes ISC, providing a versatile scaffold for the rational design of functional organic materials.
Heavier non-metal chalcogens and halogens enhance SOC and ISC in organic materials, reducing dependence on heavy metals.15–21 Organic systems featuring aromatic carbonyls or nitrogen-containing heterocycles (bearing lone-pair electrons) facilitate ISC via pronounced SOC, which originates from a change in the nature of transition orbitals (nπ* ↔ ππ*) between initial and final excited states.22,23 This process is known as the El-Sayed-allowed transition for the spin-flip process.4,23 Since SOC implies that the spin (S) and orbital (L) angular momentum of an electron are coupled, a spin-flip transition must follow the orbital angular momentum change (ΔL) according to the law of angular momentum conservation.20 A change in orbital character between the initial and final states can produce nonzero SOC, thereby allowing spin-forbidden singlet-to-triplet transitions. High SOC is associated with the nπ* ↔ ππ* transition because the nonbonding (n) orbital lies perpendicular to the π-orbital, enabling electron spin flip via a 90° orbital rotation. In contrast, the ππ* → ππ* transition in a planar system exhibits negligible SOC and is known as an El-Sayed-forbidden process, since spin flip cannot occur without a change in orbital orientation. The increase in SOC within twisted π-conjugated frameworks is attributed to π-orbital mixing and the resultant effective orbital angular momentum.24,25 Accordingly, non-planarity promotes state interactions that reinforce the ππ* → ππ* transition as an El-Sayed-allowed process.
Over the past decade, the Kim group has developed a strategy to enhance room-temperature phosphorescence (RTP) through non-covalent halogen bonding between the carbonyl moiety of 4-bromobenzaldehyde and the Br atom of a neighbouring molecule (C
O⋯Br).7–9 A heavy Br nucleus near the nπ* site activates the intermolecular heavy atom effect (HAE), promoting ISC and RTP. Importantly, their crystal design principle imparts rigidity to the system, reducing energy loss via molecular vibrations. Sarkar et al. demonstrated an alternative approach wherein substitution of a heavy Br atom proximal to the C
O group orbitals enhanced ISC in ortho-bromobenzaldehyde.26 This enhancement originates from intramolecular HAE, which operates effectively through lateral interactions between the orbitals of the Br atom and the C
O group. To date, various systems featuring heavy halogens near ΔL sites have been developed, wherein inter- or intramolecular HAEs play a pivotal role in boosting SOC and promoting the triplet-state population.27–36 In this work, we focused on intramolecular HAE, facilitated by strategic substitution that places the heavy atom in close proximity to the key chromophoric orbitals.
Polyaromatic hydrocarbons, such as perylenes, are emerging as robust photosensitizers due to superior photostability and light absorption.37 Rachford et al. reported fluorescence quenching via efficient ISC in Pt(II) complexes, where the Pt(II) center is coordinated in the bay region of two perylenediimide (PDI) units.38 Heavy-metal-free strategies have been developed for triplet exciton formation to circumvent the need for expensive metals. For example, Tiley et al. revealed ultrafast triplet formation upon replacing oxygen atoms with heavier sulfur in PDI.16 Lee et al. recently developed a thione-derived PDI–peptide bioconjugate that showed rapid ISC and served as a photosensitizer for bioimaging and PDT.39 Wu et al. reported an ISC quantum yield exceeding 90% in fused di-PDI systems, which efficiently functioned as photosensitizers for 1O2 generation.40 Modifying the bay region of perylenes by Br atoms distorts the π-system, offering an effective approach to enhancing SOC and accelerating ISC.41,42
Interestingly, bay-region engineering of perylenes affords strategic control over optoelectronic properties. For example, nitrogen doping at these sites enhances molar absorptivity, fluorescence efficiency, and host–guest interactions.43 Gryko et al. reported 1-azaperylene as a bright fluorophore with high optical emission,44 while its hydroxy derivative (12-hydroxy-1-azaperylene) showed reduced fluorescence due to excited-state intramolecular proton transfer (ESIPT).45 Hirono et al. synthesized mono- to tetra-azaperylenes via bay-position nitrogen substitution on perylene and observed a progressive decline in the fluorescence quantum yield with increasing nitrogen content due to enhanced nonradiative decay.46
In this work, we discussed the photophysical properties of a newly designed structural scaffold, in which halogens (F, Cl, and Br) are substituted at the 12-position of 1-azaperylene. The key objective is to elucidate how the heavy elements near the n-orbital of pyridinic-N promote the ISC and quench the fluorescence. Fig. 1 displays the pristine azaperylene (AP) and its 12-substituted derivatives (12-XAP). We estimated the fluorescence and ISC rate constants of these systems using theoretical and computational methods to predict the possible deactivation of the S1 state. We further examined how the substitution of Br at different positions in AP modulates the electronic structure and provides a rationale for designing metal-free spin-conversion scaffolds via HAE.
The fluorescence quantum yield (Φfl) governs photoluminescence efficiency by quantifying the radiative and nonradiative decay rate constants, which is defined as
![]() | (1) |
refers to the sum of nonradiative decay rate constants. Typically, kfl is high when the S1 state has high OS, while substantial SOC between S1 and adjacent triplet states accelerates ISC, increasing the triplet population. Thus, the estimation of ISC rate constants is crucial for a comprehensive understanding of the photophysical behaviour of AP and 12-XAP. The fluorescence rate constants (kfl) were estimated using the Strickler–Berg equation:12,58![]() | (2) |
![]() | (3) |
SOC introduces relativistic correction to the non-relativistic Hamiltonian, typically included through perturbative treatment. SOC enables state mixing and is thus essential for the description of key photophysical properties in molecular systems, for example, ISC. The Breit–Pauli Hamiltonian is utilized to compute the SOC matrix elements between non-relativistic electronic states. The form of the Breit–Pauli spin–orbit (SO) operator (in atomic units) is61–64
![]() | (4) |
The first term in eqn (4) captures one-electron SO effects, which grow strongly with Z and dominate in heavy atoms, while the two-electron term is appreciable in the case of light-atom systems, as it carries an opposite sign and a magnitude comparable to that of the one-electron term. However, a full evaluation of SOC is computationally expensive due to its two-electron term.65 The computational burden can be mitigated by approximating the two-electron term with an effective one-electron SO operator of mean-field character.62 Alternatively, two-electron effects are treated empirically in the one-electron SO operator by replacing the nuclear charge with effective value,66 and accordingly eqn (4) is reduced to an effective one-electron SO operator of the form:
![]() | (5) |
Koseki, Gordon, and co-workers notably determined Zeff values for main group elements using the multiconfiguration self-consistent field method with relativistic effective core potentials (MCSCF/SBK).66 They also formulated the scaling factor (Zeff) using the MCSCF method with all-electron basis sets as follows:
| Zeff = ymZA | (6) |
| y1 = 0.45 + 0.05n for Li–F |
| y2 = 0.98 − 0.01n for Na–Cl |
| y3 = 1.21 − 0.03n for K, Ca, Ga–Br |
| y4 = 1.24 for Rb, Sr, In–I |
Chiodo and Russo derived the scaling factor via all-electron DFT calculations using the B3LYP functional and DZVP basis set.69 Their formula defines the scaling factor as follows:
| Zeff = ymZA | (7) |
| y1 = 0.2516 + 0.0626n for B–F |
| y2 = 0.7213 + 0.0144n for Al–Cl |
| y3 = 0.8791 + 0.0039n for Ga–Br |
| y4 = 0.9228 + 0.0017n for In–I. |
Their study revealed that the FSS of diatomic systems calculated using Zeff (B3LYP/DZVP) showed excellent agreement with full-operator results and experimental data. In this work, SOC matrix elements between singlet and triplet states were evaluated using the effective one-electron SO operator (eqn (5)) and Chiodo-derived Zeff values (eqn (7)). The ωB97X-D functional and aug-cc-pVTZ all-electron basis set were used for these calculations.
| Molecule | E ab | f ab | E em | f em | k fl |
|---|---|---|---|---|---|
| AP | 3.464 | 0.635 | 3.063 | 0.680 | 2.47 × 108 |
| 12-HAP | 3.383 | 0.591 | 3.059 | 0.621 | 2.30 × 108 |
| 12-FAP | 3.533 | 0.647 | 3.126 | 0.690 | 2.61 × 108 |
| 12-CAP | 3.507 | 0.626 | 3.100 | 0.671 | 2.49 × 108 |
| 12-BAP | 3.493 | 0.611 | 3.087 | 0.657 | 2.42 × 108 |
Hydroxy substitution at the 12-position of AP (12-HAP) resulted in a 0.08 eV redshift in Eab compared to AP, while a slight redshift was observed in Eem. This trend aligns with previous experimental observations, though the experimentally measured values exhibited significantly larger redshifts.44 The redshift is underestimated because the TDDFT calculations were performed without accounting for dielectric medium effects, whereas the experimental measurements were conducted in various solvents. Our computational data revealed that the redshift observed in 12-HAP originates from an increase in its HOMO energy level, attributed to the strong electron-donating effect of the OH group (Fig. S1). Furthermore, the OH group promoted more extensive π-conjugation in the HOMO of 12-HAP relative to AP. In the past, Deperasińska et al. reported a ∼0.28 eV energy separation between Eab and Eem in 12-HAP from gas-phase TDDFT-B3LYP calculations.45 Our TDDFT calculations using the ωB97X-D functional in the gas phase estimated a 0.32 eV energy difference, closely matching the previous result.
In contrast, halogen substitution at the 12-position of AP (12-FAP, 12-CAP, and 12-BAP) exhibited blueshifts in both Eab and Eem compared to AP. This effect arises from the electron-withdrawing nature of halogens, which influences FMOs and their energies (Fig. S1). The 0.07 eV blueshift in 12-FAP, the most pronounced among the halogenated derivatives, stems from the higher electronegativity of F. While larger halogens like Cl and Br typically reduce the energy gap relative to F, resulting in a less pronounced effect. The S1 state of AP and 12-XAP originated from the HOMO → LUMO transition (Table S1), exhibiting a high transition dipole moment and substantial oscillator strength (OS). Consequently, their fluorescence rate constants (kfl ≈ 108 s−1) are significant, as kfl is directly proportional to OS according to the Strickler–Berg relationship.12,58 The experimentally determined kfl values for perylene and AP are 108 s−1, indicating that the calculated kfl value for AP aligns well with experimental results.46 Prior experimental studies have demonstrated that AP and 12-HAP exhibit strong fluorescence.45,46 To date, the synthesis and spectroscopic analysis of 12-halogenated AP derivatives have not been reported. This work used computational methods to predict the photophysical behaviour of 12-halogenated AP derivatives.
Our prior computational study on bromo-substituted perylenes, conducted using a comparable protocol, showed good agreement with experimental observations.42 An experimental study reported high Φfl for perylene and its ortho- and peri-bromo derivatives (P-oBr and P-pBr), while bay-substitution (P-bBr) led to marked fluorescence quenching.70 These trends were well rationalized through computational analysis, as summarized in Table 2. The calculated kfl values for perylene and P-pBr are in good agreement with experimental measurements. To explain the high Φfl observed for perylene, P-pBr, and P-oBr, the computational study revealed that the corresponding kisc values are negligible or 2–3 orders of magnitude lower than the kfl value. Conversely, the low Φfl of P-bBr is theoretically linked to a two-order increase in ISC, promoted by high SOC resulting from bay-induced π-twisting. In the present work, our calculations are consistent with the experimentally measured kfl and explained that the high Φfl of AP originated from its suppressed ISC.
To investigate the nonradiative decay via the ISC process, we first examined the potential ISC channels of AP and 12-XAP. SOC enables mixing between the unperturbed S1 and Tn states, allowing the singlet state to acquire partial triplet character and vice versa. This admixture allows spin-forbidden ISC to occur with enhanced probability. The extent of this mixing, denoted by λ, is primarily determined by the energy difference between Tn and S1 (ΔST) and the SOC strength. λ can be defined from the first-order perturbation theory as
Possible ISC channels for AP and 12-XAP were identified based on these two factors computed at the ωB97X-D/aug-cc-pVTZ level and are summarized in Table S2. The SOC matrix elements were computed using the effective one-electron SO operator (eqn (5)) with Chiodo-derived Zeff values presented in Table S3.
Table 3 presents the ΔST and SOC between the 1ππ* and 3nπ* states of halogenated AP, revealing basis set sensitivity on singlet–triplet gap and spin–orbit interactions. Inclusion of diffuse functions in the Karlsruhe triple-zeta basis set (def2-TZVPD)71 slightly increased the ΔST without greatly affecting SOC for 12-FAP and 12-CAP. The Dunning correlation-consistent basis set (aug-cc-pVTZ)72 exerted minimal impact on ΔST and showed a 1–1.5 cm−1 reduction in SOC for the heavier analogues (12-CAP and 12-BAP) relative to def2-TZVPD. The aug-cc-pVTZ includes extensive diffuse and high-angular-momentum polarization functions, offering more reliable SOC matrix elements for systems bearing heavier atoms.73 Table S4 summarizes the ΔST and SOC between the 1ππ* and 3nπ* states of 12-BAP for different density functionals. The negative ΔST from PBE0 and B3LYP reflected their underestimation of the 3nπ* state energy, whereas ωB97X-D and CAM-B3LYP provided more reliable energy alignment between 1ππ* and 3nπ* states, as range-separated hybrids better capture the excitation energies of charge-transfer or delocalized states such as nπ*. The SOC values obtained with PBE0 and B3LYP are about 20–30 cm−1 higher than those obtained using ωB97X-D and CAM-B3LYP. A prior theoretical study reported an SOC of 98 cm−1 between the 1ππ* and 3nπ* states in bromine-substituted naphthalenediimide (Br adjacent to the C
O group), calculated using the TDDFT/ωB97X-D/cc-pVTZ method and Chiodo-derived Zeff.74
| Molecule | def2-TZVP | def2-TZVPD | aug-cc-pVTZ | |||
|---|---|---|---|---|---|---|
| ΔST | SOC | ΔST | SOC | ΔST | SOC | |
| 12-FAP | 0.44 | 7.21 | 0.46 | 7.15 | 0.47 | 7.09 |
| 12-CAP | 0.22 | 20.27 | 0.23 | 20.04 | 0.24 | 18.95 |
| 12-BAP | 0.13 | 91.44 | 0.14 | 90.51 | 0.15 | 88.92 |
Fig. 2 shows that the T1 state is positioned significantly below the S1 state, leading to a large singlet–triplet energy gap (ΔST) across all systems. The 〈S1|Ĥso|T1〉 is weak due to their identical state character (ππ*). Consequently, T1 is not favourable for ISC due to low singlet–triplet mixing. The T2 state is energetically proximal to S1 for all systems, within the range of ±0.1 eV (Table S2), although SOC is low due to the ππ* nature. Among the several low-lying triplet states, the T6 of AP, T8 of 12-HAP, T4 of 12-FAP and 12-CAP, and T3 of 12-BAP exhibited a different state character (nπ*) than the S1 state (refer to Fig. 2). Thus, these triplet states produced significant SOC with the S1 state, with a notable enhancement observed as the halogen size increases (7 cm−1 for 12-FAP, 19 cm−1 for 12-CAP, and 89 cm−1 for 12-BAP). However, these triplet states are positioned above the S1 state, with a particularly large ΔST of 0.73 eV for AP and over 1.3 eV for 12-HAP at the S1-geometry. In contrast, ΔST decreases with increasing halogen size, with values of 0.47 eV for 12-FAP, 0.24 eV for 12-CAP, and 0.15 eV for 12-BAP. This is because the energy of the non-bonding orbital (n) in 12-HAP is more stabilized than AP, while it increases with the size of the halogens (refer to Fig. S2).
Considering the ΔST and SOC values, the preferred triplet states for ISC are T2 for AP and 12-HAP, T4 for 12-FAP and 12-CAP, and T3 for 12-BAP. Moreover, the proximity of T2 in 12-FAP, 12-CAP, and 12-BAP supports its potential as a viable ISC state. T6 in AP was considered for comparative evaluation due to its significant SOC. We calculated the ISC rate constants (kisc) for these channels in AP and 12-XAP using the Marcus theory.59,60,75 Details of kisc for selected channels are provided in Table S5. The kisc for the S1 → T2 transition in AP is 1.96 × 107 s−1, whereas for S1 → T6, it is 8.06 × 106 s−1. Despite a strong SOC (5.39 cm−1) between S1 and T6, the ISC is slow due to an uphill transition (ΔG ≈ 190 meV) with a high energy barrier of ∼244 meV. The kisc for the S1 → T2 transition in 12-HAP is 6.91 × 107 s−1, three times higher than that of AP due to a lower energy barrier (2.5 meV) and higher SOC (0.46 cm−1) compared to AP. For halogen-substituted AP, the kisc for the S1→T2 transition is ∼107–8 s−1. Although having a low energy barrier (<2 meV), the SOC of T2 associated with S1 is weak (∼0.20 cm−1). The kisc for the S1 → T2 transition of AP and 12-XAP is smaller than or comparable to their fluorescence rate constant (kfl ≈ 108 s−1). Hence, the S1 → T2 ISC channel cannot outcompete the fluorescence of these systems.
Interestingly, the kisc for the S1 → T4 transition in 12-FAP and 12-CAP is 6.19 × 108 s−1 and 6.04 × 1010 s−1, respectively. The S1 → T3 transition in 12-BAP exhibited an ultrafast ISC rate, with a kisc value of 2.22 × 1012 s−1 (Table S5). This improvement of rates is attributed to the enhanced SOC driven by a change in state character following El-Sayed's rule and an energetically favourable process (ΔG < 0). The effect is more pronounced in 12-BAP due to the heavy nucleus of Br near the region of orbital angular momentum change. In addition, the S1 → T3 transition in 12-BAP needs to overcome a minimal energy barrier (5.5 meV) compared to the S1 → T4 transition in 12-FAP and 12-CAP. The Br atom proximal to the pyridinic N in 12-BAP lowered the 3nπ* state energy through sidewise orbital interactions (Fig. 2). Hence, the proximity between the Br atom and pyridinic N in 12-BAP not only enhanced the SOC (89 cm−1) but also tuned the 3nπ* state energy to a favourable position, which enabled the 1ππ* → 3nπ* transition to occur on an ultrafast timescale.
The comparison of kisc for the most effective ISC channels in AP and 12-XAP is shown in Fig. 3. Since the kisc (S1 → T2) in AP and 12-HAP is lower than their kfl, ISC cannot quench their fluorescence. As a result, AP and 12-HAP exhibit intense fluorescence, as observed in previous experiments.45,46 In contrast, halogen substitution at the 12-position of AP increased the ISC rate, primarily guided by the change in state character between S1 and Tn states. The S1 → T4 ISC channel in 12-FAP and 12-CAP originates from the 1ππ* → 3nπ* transition, leading to an increased ISC rate. The ISC rate of 12-FAP is more than twice as fast as its fluorescence rate, which may result in a reduced fluorescence quantum yield. Meanwhile, 12-CAP cannot fluoresce, as its ISC rate is three orders of magnitude faster than its fluorescence rate. The ISC rate for the S1 → T3 channel in 12-BAP is the highest among all the channels and is four orders of magnitude faster than its fluorescence rate. Therefore, ISC effectively quenched the fluorescence in 12-BAP.
We strategically designed a structural motif where the bromine atom proximal to the pyridinic nitrogen in 12-BAP boosts ISC. This enhancement of ISC originates from the interplay of three key factors: (i) the orbital angular momentum change during the 1ππ* → 3nπ* transition; (ii) the heavy atom effect; and (iii) the favourable energy gap between 1ππ* and 3nπ* states. To rationalize the design principles behind efficient triplet population via ISC, we explored how the variation of Br positions in AP influences SOC and ISC. While these positional changes did not affect the fluorescence rate (kfl ≈ 108 s−1; Table S6), they significantly modified the energy spacing and SOC between the 1ππ* and 3nπ* states (Table S7). The 3nπ* state of 2-BAP (T7) was about 1.0 eV above the S1 state at the S1-geometry and had strong SOC (∼35.86 cm−1) with the S1 (1ππ*) state. Shifting the Br atom from the 2- to 3-position in AP lowered the 3nπ* state energy (T6) by 0.15 eV and reduced the SOC by 6 cm−1. A further shift to 4-BAP slightly reduced the 3nπ* state energy (T6) by 0.06 eV, while SOC dropped more sharply by 21 cm−1. The energy spacing between the 1ππ* and 3nπ* (T6) states remained mostly unchanged, fluctuating slightly between 0.68 and 0.78 eV, as Br was placed at various sites ranging from 4 to 11. Meanwhile, the SOC between these states remained within the range of 4.2 to 8.7 cm−1. Substituting Br at the 12-position of AP substantially altered the electronic structure, bringing the 3nπ* state (now T3 in 12-BAP) closer to the 1ππ* (S1) state (ΔST = 0.15 eV). Moreover, the SOC between these states (89 cm−1) reached the highest value among all observed cases.
Fig. 4 illustrates how the SOC, i.e., 〈1ππ*|Ĥso|3nπ*〉, varied with the distance between the Br atom and the pyridinic N. In 2-BAP, R is around 2.75 Å, the nearest distance between Br and N among all the systems. The SOC in 2-BAP is significantly strong (36 cm−1). However, when the Br atom shifts from 2 to 3, the R value increased to ∼4 Å and the SOC reduced to 30 cm−1. When R exceeded 5 Å, with Br positioned between 4 and 11, the SOC sharply decreased to a low value ranging from 4 to 8 cm−1. In 12-BAP, the Br atom is closer to N, with R below 3 Å. Consequently, the SOC is the highest among all the systems, approaching 89 cm−1. Since Ĥso ∝ Z4 (Z is the nuclear charge), a heavy Br atom near the n-orbital of pyridinic-N (at the site of ΔL) can induce strong 〈1ππ*|Ĥso|3nπ*〉 through the HAE. When comparing 2-BAP and 12-BAP, the R value of 2-BAP (2.75 Å) is lower than that of 12-BAP (2.95 Å), while the SOC is higher for 12-BAP. This contrasting behaviour can be rationalized using the NTO plot shown in Fig. 5. In AP, the n-orbital is localized on the pyridinic N, whereas in 2-BAP, the n-orbital extends in-plane with mutual alignment of the p-orbital of Br. This extension is weaker in 3-BAP and absent in 4-BAP to 11-BAP (see Fig. S3). In 12-BAP, the n-orbital exhibited greater spatial extension due to its side-wise association with the in-plane p-orbital of Br. Fig. 5 illustrates that this p-orbital of Br contributed prominently to the hole NTO of the 3nπ* state, in conjunction with the n-orbital of N. This cooperative orbital mixing leads to an expanded hole NTO for the 3nπ* state, which is orthogonal to the hole NTO of the 1ππ* state. Consequently, the SOC matrix element (〈1ππ*|Ĥso|3nπ*〉) is significantly enhanced in 12-BAP.
![]() | ||
| Fig. 4 Distance between Br and N (R in Å) in n-BAP and the SOC between the 1ππ* and 3nπ* states (〈1ππ*|Ĥso|3nπ*〉 in cm−1). | ||
![]() | ||
| Fig. 5 Natural transition orbitals of the 1ππ* and 3nπ* states for AP, 2-BAP, 3-BAP, 11-BAP and 12-BAP. | ||
Furthermore, we computed the ISC rates for the nearby 3ππ* state and the 3nπ* state of n-BAP, as summarized in Table S8. The S1 → T2 ISC channel in n-BAP corresponds to the 1ππ* → 3ππ* transition. Despite the weak SOC, the ISC remained energetically favourable (ΔG < 0), yielding kisc in the 105–7 s−1 range. For the alternative ISC channel (1ππ* → 3nπ*), kisc was quite low (∼103 s−1) for 2-BAP and varied between 105–6 s−1 for the other derivatives, except for 12-BAP (where it reached 1012 s−1). Although the SOC was higher for 1ππ* → 3nπ* than for 1ππ* → 3ππ*, the ISC for 1ππ* → 3nπ* remained inefficient across 2-BAP to 11-BAP due to the unfavourable driving force (ΔG > 0) and substantial barrier height (220–480 meV). While strong SOC allows spin-forbidden transitions, it alone does not ensure rapid ISC. In the Marcus framework (refer to eqn (3)), the ISC rate constant scales quadratically with SOC but decays exponentially with ΔG. An uphill singlet–triplet energy gap (ΔG > 0) can therefore outweigh the benefit of large SOC, so both strong coupling and favourable energetic alignment are required for efficient triplet formation. In 12-BAP, the 1ππ* → 3nπ* transition was significantly more efficient, surpassing the 1ππ* → 3ππ* by four orders of magnitude, which was driven by remarkably high SOC (〈1ππ*|Ĥso|3nπ*〉 = 89 cm−1), and an energetically favourable process (ΔG < 0) with a low activation barrier (5.5 meV). Table 4 summarizes the kisc values for the dominant ISC channel in AP and several bromo-substituted derivatives. Notably, Br proximal to the pyridinic N facilitated an ultrafast triplet population via ISC in 12-BAP owing to the enhanced SOC and the optimized energy alignment between the 1ππ* and 3nπ* states.
| Molecule | |Vsoc| | ΔG | E r | E a | k isc |
|---|---|---|---|---|---|
| AP | 0.20 | −42.5 | 114.3 | 11.3 | 1.96 × 107 |
| 2-BAP | 0.13 | −10.3 | 109.0 | 22.3 | 5.55 × 106 |
| 3-BAP | 0.23 | −16.3 | 109.5 | 19.8 | 1.91 × 107 |
| 11-BAP | 0.18 | −32.5 | 116.2 | 15.1 | 1.37 × 107 |
| 12-BAP | 88.92 | −436.5 | 546.4 | 5.5 | 2.22 × 1012 |
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