Open Access Article
Ming-Der Su
*ab
aDepartment of Applied Chemistry, National Chiayi University, Chiayi 60004, Taiwan. E-mail: midesu@mail.ncyu.edu.tw
bDepartment of Medicinal and Applied Chemistry, Kaohsiung Medical University, Kaohsiung 80708, Taiwan
First published on 3rd February 2017
The mechanisms for photochemical isomerization reactions are studied theoretically using the model systems, cyclotetrasilene and cyclobutene, both of which feature one four-membered-ring and one double bond, using the CAS(6,6)/6-311G(d) and CAS-MP2-(6,6)/6-311++G(3df,3pd) methods. The mechanisms, which are governed by the conical intersection concept, play a crucial role in these photorearrangement reactions, and explain the reaction pathways. The model computations demonstrate that the preferred reaction path for the photoisomerization reactions for both cyclotetrasilene and cyclobutene is as follows: four-membered-ring reactant → Franck–Condon region → conical intersection → butterfly-like photoproduct. These results allow a number of predictions to be made.
About 15 years ago, Kira and co-workers reported a distinctive photochemical reaction that rearranges hexakis(tert-butyldimethylsilyl)cyclotetrasilene (I) to its corresponding isomer, hexakis(tert-butyldimethylsilyl)-bicyclo[1,1,0]tetrasilane (II), as shown in Scheme 1.4 After heating, (II) is isomerized back to the initial reactant (I). However, to the best of the author's knowledge, there has been no theoretical study of the mechanism for this photo-isomerization reaction for cyclotetrasilene (I).4c This may be because the computational methods for studying photochemistry were not so mature at that time. The author uses a simplified cyclotetrasilene (Si-Rea-S0) as a model to study its photochemical mechanism for the isomerization reaction to bicyclo[1,1,0]tetrasilane (Si-Pro-S0) using modern theoretical methods, i.e., CASSCF (the complete-active-space SCF)5 and the multi-reference Møller–Plesset (CAS-MP2) algorithm.6 For the purposes of comparison, a similar mechanistic study is also made of a four-carbon system, C-Rea-S0, as represented in Scheme 2.7
Conical intersection (CI) points8 can occur on the potential surfaces, from which the excited state decays to the ground state surface at the same multiplicity (usually from singlet to singlet). Therefore, the CI mechanism is used in this work to interpret the reaction trajectories for the photochemistry of both Si-Pro-S0 and C-Pro-S0 molecules. This paper shows that the CIs8 play a decisive role in the photo-rearrangement reactions for cyclotetrasilene and cyclobutene molecules, which have a four-membered-ring.
E) + 1π*(E
E) + 2σ(E–E) + 2σ*(E–E) orbitals. The state-averaged CASSCF(6,6) method was adopted to verify geometry on the intersection space (i.e., root = 2). Moreover, the excited state gradient was obtained by using the CSASSCF method. The harmonic frequencies are computed analytically at the CAS(6,6)/6-311G(d) level of theory and are used to characterize either minima or transition states. Unless otherwise stated, the relative energies that are shown in this study are those that are ascertained at the CAS-MP2(6,6)/6-311++G(3df,3pd) level, using the CAS(6,6)/6-311G(d) geometry. These are designated CAS-MP2 and CASSCF, respectively. The Cartesian coordinates and the energies that are computed for the various points are available as ESI.†
In order to determine possible excited-state reaction paths that lead to CIs, a molecular orbital representation of the relationship between the likely reaction pathway and intersection is schematically illustrated in Scheme 3 (E = C and Si),13 which is a foundation for these theoretical studies. Upon irradiation with light, a singlet four-membered-ring molecule (1) is moved up to a singlet excited species (2), succeeding an intramolecular double bond (E
E) rotation. Then, as shown in (3), this excited molecule 1 can be considered as a composition of four kinds of carbenes (>E), existing four spin-up σ orbitals and four spin-down σ orbitals.13 Consequently, through the conical intersection, a two-three-membered-ring photoproduct (4) can be obtained.
Using the molecular orbital analysis that is given in Scheme 3, since the narrow energy gap between S0 and S1 energy surfaces strongly implies the existence of a CI point, Si-Rea-S0 and C-Rea-S0 are used as examples to determine whether there is a low-lying S1/S0 surface crossing. Fig. 1 shows the potential energy profiles for the rotational angle, θ, as shown in Scheme 3.14 Fig. 1(A) and (B) show that the reaction pathways all terminate at a very similar S1–S0 energy gap at around 75° and 60°, respectively. These energy profile results suggest that a CI point occurs in the intramolecular rotation for the four-membered-ring geometries. In the next section, these findings are used to explain the mechanisms for the photochemical isomerization reactions of Si-Rea-S0 and C-Rea-S0.
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Fig. 1 The scans for finding a CI pathway using a E E (E = C and Si) rotation in the reactants ((A) Si-Rea-S0 and (B) C-Rea-S0; R = SiH3) for the angle, θ, optimized for the S0 and S1 states at the CAS(6,6)/6-311G(d) level of theory. See the text and ESI.† | ||
A comparison with the CASSCF-optimized geometry for the silicon reactant (Si-Rea-S0), as shown in Fig. 2, shows that the theoretical values for the bond lengths and the bond angles in these four-membered-ring species are in good agreement with the experimental values.4 The bond lengths and the bond angles are within 0.07 Å and 5.9°, respectively. Therefore, CASSCF and CAS-MP2 computations should be satisfactory for a theoretical study of the photochemical and thermal reactions.
Initially, cyclotetrasilene (Si-Rea-S0) with a four-silicon-membered-ring is irradiated by visible light and is promoted to the Franck–Condon region at the first excited singlet state (Si-FC-S1), which is shown on the left side of Fig. 2. Subsequently, this species relaxes to the conical intersection point (Si-CI), from which it can go to either the final photoproduct (Si-Pro-S0) or the initial reactant (Si-Rea-S0). These CAS-MP2 computations show that the relative energies for Si-FC-S1, Si-CI, and Si-Pro-S0 with respect to Si-Rea-S0 are 68, 42, and 21 kcal mol−1, respectively. The theoretical evidence strongly suggests that when cyclotetrasilene (Si-Rea-S0) is irradiated by visible light, it easily undergoes a Si
Si double bond rotation to produce either the reactant (Si-Rea-S0) or the corresponding bicyclo[1,1,0]tetrasilane (Si-Pro-S0). The photochemical isomerization mechanism for Si-Rea-S0 that is shown in Fig. 2 is represented as follows:
| Cyclotetrasilene (photo): Si-Rea-S0 + hν → Si-FC-S1 → Si-CI → Si-Pro-S0 |
The thermal (dark) reaction on the ground singlet state energy surface that is shown in Fig. 2 is also studied. Fig. 2 shows that the Si-TS-S0 point combines Si-Rea-S0 and Si-Pro-S0 on the ground singlet surface and that its energy lies 15 kcal mol−1 below the energy of the Si-CI point. It is worthy of note that the CAS-MP2 calculations give barrier heights for Si-Rea-S0 → Si-TS-S0 and Si-Pro-S0 → Si-TS-S0 that are approximately 34 and 12 kcal mol−1, respectively. This theoretical evidence points to the fact that cyclotetrasilene (Si-Rea-S0) is thermodynamically more stable than bicyclo[1,1,0]tetrasilane (Si-Pro-S0) and producing the latter from the former using the thermal reaction would be difficult, which is in good agreement with the experimental results.4 Fig. 2 also predicts that the thermal reversion from Si-Pro-S0 to Si-Rea-S0 is relatively easily accomplished, since the energy that is required to surmount the reverse barrier (12 kcal mol−1) is less than that which is required to surmount forward barrier (34 kcal mol−1). This theoretical prediction is again in good agreement with the available experimental results.4
The photochemical conversion of C-Rea-S0 to C-Pro-S0 and its thermal reversion are studied. The computational results are all listed in Fig. 3. Similarly to the model for cyclotetrasilene (Si-Rea-S0), the singlet photo-rearrangement reaction for C-Rea-S0 that is studied in this work follows similar reaction paths to those that are shown in Fig. 2. The CAS-MP2 computations suggest that the photo-isomerization reaction for C-Rea-S0 proceeds as follows:
| Cyclobutene (photo): C-Rea-S0 + hν → C-FC-S1 → C-CI → C-Pro-S0 |
However, the CAS-MP2 results demonstrate that much higher energy (117 kcal mol−1) of C-FC-S1 than that of the irradiating light (420 nm = 68 kcal mol−1) makes this photo-rearrangement reaction energetically unfeasible,15 so the energy of photo-irradiation is insufficient to generate the butterfly-like product, C-Pro-S0 via radiation-less decay (i.e., the CI channel). Consequently, no photo-isomerization reaction should be observed in these cyclobutene systems for irradiation with visible light. However, the thermal reversion (C-Pro-S0 → C-Rea-S0) is predicted to be easily achieved, since the energy that is required to surmount the reverse barrier (C-Pro-S0 → C-TS-S0) is calculated to be 10 kcal mol−1 less than that which is required to surmount the forward barrier (C-Rea-S0 → C-TS-S0), using the CAS-MP2 calculations. To the best of the author's knowledge, no experimental reports of the photochemical reactions of cyclobutenes have been published so the CAS-MP2 computational results that are shown in Fig. 3 remain a prediction.
CH2) and silene (H2Si
SiH2). The energy gap for the HOMO (π) and the LUMO (π*) for ethylene is much larger than that for silene. Silene also has a higher HOMO (π) and a lower LUMO (π*) than ethylene. For details, see ref. 2.Footnote |
| † Electronic supplementary information (ESI) available. See DOI: 10.1039/c7ra00506g |
| This journal is © The Royal Society of Chemistry 2017 |