Weiliang
Shi
a,
Jianzheng
Ma
b,
Chenwei
Jiang
*b and
Tetsuya
Taketsugu
*cd
aGraduate School of Chemical Sciences and Engineering, Hokkaido University, Sapporo 060-0810, Japan
bMinistry of Education Key Laboratory for Nonequilibrium Synthesis and Modulation of Condensed Matter, Shaanxi Province Key Laboratory of Quantum Information and Quantum Optoelectronic Devices, School of Physics, Xi’an Jiaotong University, Xi’an 710049, China. E-mail: jiangcw@xjtu.edu.cn
cDepartment of Chemistry, Faculty of Science, Hokkaido University, Sapporo 060-0810, Japan. E-mail: take@sci.hokudai.ac.jp
dInstitute for Chemical Reaction Design and Discovery (WPI-ICReDD), Hokkaido University, Sapporo 001-0021, Japan
First published on 14th May 2024
In this study, we have advanced the field of light-driven molecular rotary motors (LDMRMs) by achieving two pivotal goals: lowering the thermal helix inversion (THI) barrier and extending the absorption wavelength into the visible spectrum. This study involves the structural reengineering of a second-generation visible LDMRM, resulting in the synthesis of a novel class, specifically, 2-((2S)-5-methoxy-2-methyl-2,3-dihydro-1H-cyclopenta[a]naphthalen-1-yl)-3-oxo-2,3-dihydro-1H-dibenzo[e,g]indole-6,9-dicarbonitrile. This redesigned motor stands out with its two photoisomerization stages and two thermal helix inversions, featuring exceptionally low THI barriers (4.00 and 2.05 kcal mol−1 at the OM2/MRCI level for the EM → EP and ZM → ZP processes, respectively). Moreover, it displays absorption wavelengths in the visible light range (482.98 and 465.76 nm for the EP and ZP isomers, respectively, at the TD-PBE0-D3/6-31G(d,p) level), surpassing its predecessors in efficiency, as indicated by the narrow HOMO–LUMO energy gap. Ultrafast photoisomerization kinetics (approximately 0.8–1.6 ps) and high quantum yields (around 0.3–0.6) were observed through trajectory surface hopping simulations. Additionally, the simulated time-resolved fluorescence emission spectrum indicates a significantly reduced “dark state” duration (0.09–0.26 ps) in these newly designed LDMRMs compared to the original ones, marking a substantial leap forward in the design and efficiency of LDMRMs.
Most LDMRMs traditionally rely on ultraviolet (UV, 100–400 nm) or visible (400–750 nm) light for their excitation. This approach comes with several drawbacks: UV light is undesirable for constructing nodular photoresponsivity systems;3 UV light is less than ideal for constructing compact photoresponsive systems, and it can be detrimental to materials prone to degradation, while also posing a risk to cell health due to photoreactions in some cellular components.8 Consequently, shifting the absorption band of the chromophore to the visible or near-infrared region of the electromagnetic spectrum has become a central concern within the LDMRM field. Various strategies have been explored to achieve a redshift of the excitation wavelength for well-established LDMRMs. Among these approaches, the most effective is believed to be the fine-tuning of the highest occupied molecular orbital (HOMO)–lowest unoccupied molecular orbital (LUMO) band gap through structural modifications of the molecular motor. In 2003, the Feringa group introduced a groundbreaking concept by proposing a donor–acceptor functionalized LDMRM, enabling the absorption of photons at 430 nm through the introduction of a push–pull system in the lower half of the molecular motor, facilitating photoisomerization.9 More recently, Leeuwen and colleagues10 introduced a class of LDMRMs based on the push–pull system. The incorporation of a benzofluorenyl moiety into a standard molecular motor resulted in a considerable bathochromic shift, with λmax transitioning from 395 nm of the parent motor to 420 nm due to enhanced π-conjugation. Pfeifer et al.11 further delved into the structural redesign of the second-generation LDMRM based on a push–pull system, achieving an even more pronounced redshift in the maximum absorption wavelength by altering substituents in the stator and rotor. In their study, three push–pull motors and a tricyano-substituted motor (1s, 2s, 6s refer to Fig. 1) were prepared, allowing for a comparative analysis of the impact of push–pull substitution on π-system extension by the CN-group in 6s.11 The results revealed maximum absorption wavelengths of 422 nm (1s), 453 nm (2s), and 421 nm (6s), with quantum yields ranging from approximately 0.3–0.11. These findings underscore the potential for achieving a redshift in absorption wavelength through strategic structural design, such as the introduction of substituent groups.12,13
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Fig. 1 The geometry of rotary motor 1s, 2s, 6s, and the newly designed Xs, as well as DDPYM. Some atoms are labelled by red numbers. |
Feringa-type molecular motors exist in two main configurations: 4-stroke (involving two steps of photoisomerization coupled with two steps of thermal helix inversion (THI)),12,13 and 2-stroke (consisting of two photoisomerization steps only).14 The timescales for the photoisomerization and THI steps span from nanoseconds to days and femtoseconds to picoseconds, respectively.15,16 The rotation speed of a designed LDMRM is influenced by all the constituent steps in its rotation cycle, and the high energy barrier associated with the THI step hinders the overall rotation speed of LDMRMs. Hence, there exists considerable potential for enhancing the rotation speed by reducing the THI barrier.3 Recently, a new family of fulgide-based LDMRMS was reported by Filatov et al.17 They investigated the dynamics properties of these prototype molecules using a combination of quantum chemical calculations and trajectory surface hopping (TSH) simulations with Tully's fewest switches algorithm.18 The TSH method is a highly effective technique for exploring the elementary processes of excited-state dynamics by calculating potential gradients through electronic structure calculations to determine the forces acting on atoms, deriving classical trajectories through numerical solutions of Newton's equations of motion, and considering transitions between electronic states due to non-adiabatic couplings.19,20 Theoretical simulations predicted a quantum efficiency of 0.55–0.68 for these prototype molecules, an ultrafast dynamics timescale of 200 to 300 fs, and a thermal helix potential barrier of 13.6 kcal mol−1.
Several new designs of LDMRMs have been theoretically proposed to augment the rotation speed by minimizing the THI step. Filatov et al.21 reported a new class of 2-stroke LDMRM capable of 360° rotation by reengineering the rotor blades and combining two photoisomerization steps. The TSH simulations predicted a photoisomerization process taking place within a timescale of 200 to 300 fs, demonstrating a notably high quantum yield of approximately 0.91–0.97. García-Iriepa et al.22 proposed a 2-stroke photoreaction-only LDMRM that eliminates the THI step and achieves rapid rotation by introducing a chiral hydrogen bond environment. More recently, Ma et al.23 introduced a new 3-stroke LDMRM capable of a full 360° rotation in two photoisomerization steps and one THI step, named DDIYs. TSH simulations at the semi-empirical OM2/MRCI level predicted ultrafast timescales (0.1 to 0.3 fs) for the two photoisomerization steps. They also designed an oxindole-based LDMRM, DDPYM,24 with a push–pull character and minimal steric hindrance near the rotation axis, leading to faster and more concentrated electronic decay of the S1 excited state compared to its parent molecule.
Consequently, significant research endeavors have been dedicated to shifting the absorption wavelength of molecular motors into the visible spectrum while upholding rotation speed and quantum yield. Drawing inspiration from the oxindole-based LDMRM, we introduce a new category of 4-stroke light-driven molecular motors, denoted as 2-((2S)-5-methoxy-2-methyl-2,3-dihydro-1H-cyclopenta[a]naphthalen-1-yl)-3-oxo-2,3-dihydro-1H-dibenzo[e,g]indole-6,9-dicarbonitrile, or simply “Xs” (Fig. 1). Our molecule design draws from the second-generation LDMRMs established by Pfeifer et al.,11 focusing on tuning the HOMO–LUMO energy gap and minimizing the THI barrier. This adaptation enables a 360° rotation that encompasses two-step photoisomerization (EP to ZM and ZP to EM) and two-step thermal helix inversion. The primary aim was to conduct a comprehensive assessment of key attributes, including the UV-visible (UV-vis) spectrum, time-resolved fluorescence emission spectrum, the THI barrier, quantum yield, and average lifetime. These comparative analyses allowed us to evaluate and validate the performance of the designed LDMRM. Furthermore, we conducted a detailed comparative analysis with a recently conceived oxindole-based LDMRM named “DDPYM” (Fig. 1). We believe that this innovatively designed LDMRM will serve as a catalyst for further experimental and theoretical research in this domain.
The OM2/MRCI method, recognized for its computational efficiency and accuracy in exploring excited state dynamics, has been widely used in the investigation of photochemical reactions,26–37 as evident in benchmark papers.38–42 In this study, the OM2/MRCI method, implemented in the MNDO99 program,43 was utilized for excited-state calculations and dynamics simulations of LDMRMs 1s, 2s, 6s, and Xs. The Lagrange–Newton approach44 facilitated the identification of S1/S0 minimum energy conical intersections (MECIs) along the photoisomerization pathways. Multireference configuration interaction (MRCI) calculations were conducted for three reference states, encompassing the closed-shell ground-state, and single and double excitations from HOMO to LUMO. Considering the characteristics of ππ* electronic excitations and the convergence of the optimizations for MECIs, we selected active spaces (8,9), (10,10), (8,8), and (8,8) for the three substituent molecular motors, 1s, 2s, 6s, and Xs, respectively, in the OM2/MRCI calculations. To ensure the persistence of π orbitals within the active space throughout the calculation process, we identified and tracked the π-type population (PIPOP) using a threshold of 0.4.
The TSH simulations were conducted for molecular motors within the framework of the OM2/MRCI method utilizing Tully's fewest-switches algorithm.18 Initial conditions were generated by the ground state equilibrium structure, with atomic velocities randomly distributed according to a Wigner distribution at 300 K. Geometries were selectively chosen using the filtering approach integrated into the MNDO program.43 In this filtering approach, transition probabilities are calculated for structures generated via Wigner sampling, and structures are then selected as initial conditions based on a comparison between these transition probabilities and random numbers.45 Wigner sampling is based on harmonic normal modes, and when it includes low-frequency modes, it samples structures that deviate from the equilibrium configuration. This can be problematic because in the actual potential energy surfaces of molecular systems, the effects of anharmonicity and mode coupling contribute, which reduces the accuracy of structural sampling along low-frequency modes. A simple workaround is to exclude these low-frequency modes from the sampling. However, more precise methods such as the quantum thermostat technique have been devised recently, and comparisons between these methods and experimental data are being made.46 Although the molecular system in the current study includes low-frequency modes, the purpose of the TSH simulations using OM2/MRCI is qualitative rather than quantitative, so we used conventional Wigner sampling to set the initial conditions. To enhance accuracy, the empirical decoherence correction proposed by Granucci et al.47 (0.1 a.u.) was applied. The Newton equation of motion was resolved employing a time step of 0.1 fs through the velocity-Verlet algorithm,48 while the time-dependent electronic Schrödinger equation was solved with a time step 100 times smaller.
Fig. 2 and 3 illustrate schematic diagrams of potential energy profiles for the rotation cycle of the molecular motors 1s and Xs, respectively. Table 1 presents the calculated energy barriers for 1s, 2s, 6s (between M and P), and Xs (between ZM and ZP and between EM and EP) in the ground state, calculated using the OM2/MRCI method. The optimized transition state geometries are depicted in Fig. S1, S3, S5 and S6 (ESI†), and corresponding structural parameters are provided in Tables S1, S4, S7 and S10 (ESI†). The OM2/MRCI results align well with those obtained through DFT calculations. As depicted in Fig. 2 and 3, the molecular motor undergoes photoexcitation to the FC region (P isomer for 1s and EP and ZP isomers for Xs). Subsequently, the molecular motor rotates counterclockwise around the CC double bond, decaying to the ground state via S1/S0 CIs, and eventually reaching stable M isomers for 1s and ZM or EM isomers for Xs. Over time, the stable M isomers of 1s and ZM or EM isomers of Xs traverse the THI barrier and isomerize to P′ of 1s and ZP of EP isomers for Xs. Table 1 reveals that the relative values of THI barriers for 1s, 2s, 6s, and Xs are consistent regardless of the method used. The THI barriers of the newly designed molecular motor Xs are notably lower than those of 1s, 2s, and 6s, suggesting a potentially higher rotational speed for Xs compared to 1s, 2s, and 6s. In comparison to DDPYM, the THI barriers of Xs are higher than DDPYM between ZM and ZP, while THI barriers between EM and EP are lower. This implies that the rotational speed of Xs may differ from DDPYM depending on the specific isomerization pathway, with Xs being faster for EM to EP and potentially slower for ZM to ZP. Fig. S2 and S4 (refer to ESI†) provide a similar schematic diagram of potential energy profiles for 2s and 6s.
OM2/MRCI | B3LYP-D3 | CAMB3LYP-D3 | M062X | ωB97XD | ||
---|---|---|---|---|---|---|
1s | M → P′ | 19.80 | 22.06 | 21.52 | 21.80 | 21.52 |
2s | M → P′ | 20.59 | 23.50 | 22.95 | 23.13 | 22.92 |
6s | M → P′ | 20.01 | 22.95 | 22.51 | 22.75 | 22.46 |
Xs | ZM → ZP | 4.00 | 5.74 | 5.33 | 4.66 | 4.87 |
EM → EP | 2.05 | 6.26 | 6.35 | 7.17 | 6.47 | |
DDPYM24 | ZM → ZP | 2.00 | — | — | — | — |
EM → EP | 8.80 | — | — | — | — |
TDDFT | OM2/MRCI | Exp. | ||
---|---|---|---|---|
1s | P | 445.28/2.78 | 364.5/3.40 | 422/2.94 |
2s | P | 422.21/2.94 | 362.5/3.42 | 453/2.74 |
6s | P | 425.22/2.92 | 353.0/3.51 | 421/2.95 |
Xs | EP | 482.98/2.57 | 395.0/3.14 | |
ZP | 465.76/2.66 | 382.5/3.24 | ||
DDPYM | EP | 385.99/3.21 | ||
ZP | 383.00/3.23 |
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Fig. 4 (a) UV-Vis spectra and equilibrium structures of 1s, 2s, 6s, Xs, and DDPYM determined in the gas phase by TDDFT calculations at the PBE0-D3/6-31G(d,p) level. (b) The experimental spectra for 1s, 2s, and 6s (Solid lines: UV-vis spectra of 1s, 2s, and 6s in dichloromethane solvent. Dashed lines: UV-vis spectra after irradiation to photo-stationary states (PSS) with 420 nm (1s, 6s) and 455 nm (2s) light) (Reproduced from ref. 11 with permission from the Royal Society of Chemistry). |
The overall UV-vis spectra generated from Wigner sampling and absorption spectra at the OM2/MRCI level were also calculated and are shown in Fig. S7(a) and (b) (ESI†), respectively, with maximum absorption wavelengths listed in Table 2. The absorption spectra of 1s, 2s, 6s, and Xs span from 250 to 550 nm, qualitatively alligning with TDDFT calculations. Notably, the maximum absorption wavelength of Xs (EP and ZP) is greater than that observed for 1s, 2s, and 6s, which can also be shown in Fig. S7(b) (ESI†). The consistency between the several sets of results indicates that the newly designed motors exhibit a significant redshift in the UV-vis absorption spectrum. To further elucidate the reason for the redshift of Xs, we examined the relevant frontier molecular orbitals. As illustrated in Fig. 5, the HOMO–LUMO energy gap of molecular motor Xs is notably low compared to the substituent motors 1s, 2s, and 6s. The structural modification of Xs has reduced the HOMO–LUMO energy gap by altering the HOMO and LUMO charge distribution. Consequently, the maximum wavelengths of the UV-vis absorption spectra of the newly designed molecular motor Xs were red-shifted to 482.98 and 465.76 nm.
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Fig. 5 The HOMO and LUMO of motor 1s-P, 2s-P, 6s-P, Xs-EP, and Xs-ZP, calculated at the PBE0-D3/6-31G(d,p) level, with HOMO–LUMO gap in eV. |
For 1s, 2s, 6s, Xs (EP), and Xs (ZP), 400 structures were generated, respectively, using Wigner sampling. Through the filtering approach, about 70% of these structures were selected. From the chosen structures, 175, 242, 233, 220, and 179 structures, respectively, were selected as initial conditions for trajectory calculations, and we conducted TSH simulations from the S1 excited state. The simulation times were 5.0, 2.5, 5.0, 1.5, and 3.0 ps for each molecular species. Isomerization to M was achieved for 1s, 2s, and 6s by counterclockwise rotation around the central CC double bond, with quantum yields of approximately 0.78, 0.6, and 0.67, respectively. For Xs, the photoisomerization process was investigated for EP and ZP starting from the S1 excited state, with quantum yields of approximately 0.55 and 0.37 for EP → ZM and ZP → EM, respectively. In the case of DDPYM, the quantum yield for the transition from EP to ZM is 0.52, and for the transition from ZP to EM is 0.36. Which is comparable to Xs. Fig. 6 illustrates the time evolution of the S0 and S1 state populations for 1s, 2s, 6s, Xs-EP, and Xs-ZP. The average lifetimes of the S1 state for each molecular species are calculated to be 2.56, 1.16, 2.40, 0.85, and 1.85 ps, respectively. Table 3 presents the number of trajectories, quantum yields, and lifetimes. The newly designed molecular motor Xs exhibits a slight decrease in the quantum yield of the photoisomerization reaction compared to 1s, 2s, and 6s. The time evolution of the population reveals that the average lifetime of the EP → ZM isomerization of Xs is extremely short compared to 1s, 2s, and 6s, and the ZP → EM isomerization reaction is also significantly shorter than that of 1s and 6s. Indeed, when comparing the simulated average lifetimes of DDPYM for the EP → ZM (0.27) and ZP → EM (0.44), it becomes evident that the lifetimes in DDPYM are significantly shorter than those in Xs. This suggests that Xs may exhibit longer-lived excited states compared to DDPYM.
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Fig. 6 The average population of electronic states S0 and S1 over simulation time in the photoisomerization process starting from (a) 1s-P, (b) 2s-P, (c) 6s-P, (d) Xs-EP, and (e) Xs-ZP isomers. |
Number of trajectories | Quantum yields | Average lifetime (ps) | ||
---|---|---|---|---|
1s | P–M | 175 | 0.78 | 2.56 |
2s | P–M | 242 | 0.60 | 1.16 |
6s | P–M | 233 | 0.67 | 2.40 |
Xs | EP–ZM | 220 | 0.55 | 0.85 |
ZP–EM | 179 | 0.37 | 1.58 | |
DDPYM24 | EP–ZM | 238 | 0.52 | 0.27 |
ZP–EM | 221 | 0.36 | 0.44 |
To provide further insight into the reduced lifetime of Xs-EP and Xs-ZP compared to 1s, 2s, and 6s, we conducted nonadiabatic dynamics simulations of the photoisomerization process to compute the “dark state” duration. The dark state duration was determined based on the obtained average lifetime and the time-dependent fluorescence emission spectrum presented in Fig. S12a, S13a, S14a, S15a, and S16a (ESI†), with the corresponding data listed in Table S15 (ESI†). It is important to note that the term “dark state” in this context does not refer to a new electronic state but rather signifies a “dark region” with low oscillator strength on the excited state.27 The computational details of the time-dependent fluorescence emission spectrum and a more comprehensive description of the computational results can be found in the ESI.† As indicated in Table S15 (ESI†), the “dark state” durations for 1s, 2s, and 6s are 1.86, 0.90, and 2.06 ps, respectively, which are significantly longer than those for Xs-EP and Xs-ZP at 0.09 and 0.26 ps. This observation may elucidate why the average lifetime of the EP → ZM process for XS is extremely shorter than that for 1s, 2s, and 6s, and the ZP → EM process is also significantly shorter than that for 1s and 6s. The slightly higher average lifetime of ZP → EM process for Xs compared to 2s may be attributed to the steric bulkiness in the fjord region of Xs-ZP (C40–C2–C1–C15 is −4.4°, C2–C1–C15–C17 is 33.0° based on OM2/MRCI level), which is less than that of 2s-P (C40–C2–C1–C15 is 12.9° and C2–C1–C15–C17 is 39.3° based on OM2/MRCI level). This difference in steric hindrance implies that the rotation from Xs-ZP to the CIs will take more time than for 2s, even though the “dark state” duration is significantly reduced for Xs-ZP compared to 1s-P.
TSH simulations at the OM2/MRCI level were employed to investigate the photoisomerization process of 1s, 2s, 6s, and Xs. Remarkably, it was observed that the average lifetime of EP → ZM for Xs is shorter than that of 1s, 2s, and 6s molecular motors. Similarly, ZP → EM is shorter than for 1s and 6s but slightly longer than 2s, with no significant impairment in the quantum yield of the newly designed molecular motor. Calculated time-dependent fluorescence emission spectrum results demonstrated that the “dark state” duration of 1s, 2s, and 6s is significantly longer than that of Xs-EP and Xs-ZP.
In summary, the computational results indicate that the newly proposed light-driven molecular rotary motor Xs exhibits a low thermal helix potential barrier and a simultaneous red-shift in visible light absorption wavelength. In comparison to DDPYM, improvements have been observed in both the UV-visible absorption spectrum and the THI barrier. This work is anticipated to stimulate further research into the design and synthesis of new families of molecular rotary motors.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4cp00037d |
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