Chenchen Guo,
Huiqun Wang,
Bo-Zhen Chen* and
Zhiyuan Tian
School of Chemistry and Chemical Engineering, University of Chinese Academy of Sciences, No. 19A, YuQuan Road, Beijing 100049, P. R. China. E-mail: bozhenchen@hotmail.com; Fax: +86 10 88256092; Tel: +86 10 88256129
First published on 18th November 2014
Density functional theory calculations have proven the polar nature of the crossed intermolecular radical anion cycloadditions of various enones. The substituent effects on the chemo- and stereoselectivity of the cycloadditions have been elucidated. The electronic structures of the substituents strongly influence the formation of the radical anion and the reactivity of cycloaddition. The amino and nitryl substituents are both unfavorable for the cycloaddition. The cycloaddition is sensitive to the substituents on the C atoms which form a σ bond in the first cycloaddition step by both steric hindrance and electronic effect. To improve the chemoselectivity, one of these C atoms should be unsubstituted. The stereoselectivity mainly caused by the difference in steric interaction between the trans and cis transition states is benefited by the bulky substituents on the carbonyl.
The intermolecular radical cation cycloaddition of styrenes has been found to have low activation barrier and excellent stereoselectivity.8–11 Thereafter, a variety of intramolecular radical anion cycloadditions of bis(enones) were carried out using electrocatalysis12 and chemically induced13 methods. However, the development of the intermolecular radical anion cycloaddition is limited by the initiation methods. Recently, the T. P. Yoon's laboratory have reported that Ru(bipy)32+ serves as an excellent visible light photocatalyst for initiating the inter-/intramolecular anion/cation [2 + 2] cycloaddition,14–17 representing a considerable advance in construction of cyclobutane-containing structures. In our previous studies, we have investigated the intramolecular cycloadditions of bis(enones) and bis(styrenes) and the intermolecular cycloaddition between phenyl vinyl sulfone and enone by theoretical methods.18–21 The investigation gave an insight into the origin of the stereoselectivity of intramolecular cycloadditions and the regioselectivity of intermolecular cycloaddition. However, the origin of the chemo- and stereoselectivity of intermolecular cycloaddition is still unclear.
The experimental investigation of the intermolecular cycloadditions of enones (reactions 1–3 and 6–9 shown in Table 1(b)) showed that the substituents had a dramatic effect on the reactivity and stereoselectivity of the cycloaddition.15 Reactions 1–3 and 6 show good yield and excellent stereoselectivity to form the trans products. The yields of reactions 7 and 8 are relative low, but the stereoselectivity was kept. The stereoselectivity of reaction 9 substituted by methoxyl on carbonyl is not so excellent as other reactions. To avoid the undesired homodimerization, the researchers used two dissimilar enone substrates in all the reactions. One of the reactants must be aryl enone to initiate the radical anion reaction. The other is acting as a Michael acceptor. All the reactions except reaction 8 gave excellent chemoselectivity to form the crossed cycloaddition products. However, in reaction 8, the yield of the homodimerization product of the aryl enone is higher than that of the crossed cycloaddition products. In this paper, we not only calculated these above reactions 1–3, and 6–9, but also designed and calculated reactions 4, 5, and 10–16 (see Table 1(b)), to investigate the substituent effect on the chemo- and stereoselectivity of the intermolecular cycloaddition. We hope that our investigations can provide important information for further designing new novel intermolecular [2 + 2] cycloadditions.
(a) | |||||||||
---|---|---|---|---|---|---|---|---|---|
(b) Reactions | R1 | R2 | R3 | R4 | Reactions | R1 | R2 | R3 | R4 |
1 (R1a + R2a) | Ph | Me | Me | H | 9 (R1a + R2c) | Ph | Me | MeO | H |
2 (R1b + R2a) | ClPh | Me | Me | H | 10 (R1a + R2d) | Ph | Me | NO2 | H |
3 (R1c + R2a) | MeOPh | Me | Me | H | 11 (R1a + R2e) | Ph | Me | Me | NH2 |
4 (R1d + R2a) | NO2Ph | Me | Me | H | 12 (R1a + R2f) | Ph | Me | Me | NO2 |
5 (R1e + R2a) | NH2Ph | Me | Me | H | 13 (R1a + R1a) | Ph | Me | Ph | Me |
6 (R1f + R2a) | Ph | Et | Me | H | 14 (R1b + R1b) | ClPh | Me | ClPh | Me |
7 (R1g + R2a) | Ph | t-Bu | Me | H | 15 (R1c + R1c) | MeOPh | Me | MeOPh | Me |
8 (R1a + R2b) | Ph | Me | Et | Me | 16 (R1f + R1f) | Ph | Et | Ph | Et |
Frequency analysis calculations at the B3LYP level at 298 K were performed to confirm each stationary point along the reaction pathway to be either a minimum (no imaginary frequencies) or a transition-state (only one imaginary frequency). The intrinsic reaction coordinate (IRC)26–28 pathways have been traced to confirm whether the transition state connects the reactant, intermediate, or product. The energies presented in this paper were corrected with zero-point energies (ZPEs) calculated at the B3LYP/6-311+G(d,p) level. Gibbs free energies and enthalpies in gas phase at 298 K and 1 atm were calculated at the same level. The single-point solvation Gibbs free energies were calculated by using SMD solvation model in CH3CN solvent (used in the experiment) at the same level as well.29
All of the quantum chemical calculations were performed using the Gaussian 09 program.30 The 〈S2〉 values for the doublet states of all the reactants, transition states, intermediates, and products along the reaction pathways at the (U)B3LYP/6-311+G(d,p) level were less than 0.78, where the double state is expected to be 0.75.
As shown in Table 2, the order of the EAad in solvent is the same to that in gas phase, but the EAad values in solvent are considerably lower than those in gas phase, indicating that the radical anion could be stabilized by the solvent. The order of the calculated EAad values is R1d > R1b > R1a > R1c > R1e, which is consistent with the electron-withdrawing capacity of the substituents: NO2Ph > ClPh > Ph > MeOPh > NH2Ph. Thus, strong electron-withdrawing substituents are beneficial for the formation of radical anion reactant. It is noted that the EAad value of R1e is the lowest, indicating the disadvantage for R1e to afford the radical anion over other reactants. Similarly, the EAad of R2d and R2f with electron-withdrawing substituents are much larger than those of R2a, R2b, R2c and R2e with electron-donating substituents. In the cycloadditions of R1a–g and R2a, as the EAad values of R1a–g are all larger than that of R2a, the formed radial anions should be R1a–g•−. It is noted that, in the cycloadditions of R1a and R2a–c, R2e, the formed radical anion should be R1a•−, while in the cycloadditions of R1a and R2d, R2f, the formed radical anions should be R2d•−, R2f•−. The above analysis shows that in reactions 1–3 and 6–9, the radical anions are formed by the aryl enones indeed, which confirms the prediction by the experimentalist.
Species | EAada (vacuum) | EAada (CH3CN) | Species | EAada (vacuum) | EAada (CH3CN) |
---|---|---|---|---|---|
a EAad = E(optimized neutral) − E(optimized anion).31,32 | |||||
R1a | 17.9 | 58.9 | R2a | 7.5 | 49.8 |
R1b | 23.1 | 60.7 | R2b | 4.1 | 48.9 |
R1c | 14.5 | 55.3 | R2c | 2.8 | 41.7 |
R1d | 46.3 | 81.7 | R2d | 46.3 | 89.4 |
R1e | 11.7 | 53.2 | R2e | −6.9 | 38.2 |
R1f | 18.8 | 59.1 | R2f | 50.8 | 134.5 |
R1g | 16.2 | 56.9 |
Species | ω [ev] | μ [a.u.] | η [a.u.] | ΔNmax [e] | Species | ω [ev] | μ [a.u.] | η [a.u.] | ΔNmax [e] |
---|---|---|---|---|---|---|---|---|---|
R1a•− | 0.85 | 0.0679 | 0.0733 | −0.9255 | R2a | 2.03 | −0.1701 | 0.1847 | 0.9209 |
R1b•− | 0.64 | 0.0611 | 0.0797 | −0.7675 | R2b | 1.73 | −0.1569 | 0.1939 | 0.8094 |
R1c•− | 1.02 | 0.0618 | 0.0508 | −1.2152 | R2c | 1.86 | −0.1763 | 0.2274 | 0.7751 |
R1d•− | 0.04 | 0.0154 | 0.0720 | −0.2134 | R2d•− | 0.27 | 0.0457 | 0.1062 | −0.4300 |
R1e•− | 1.09 | 0.0641 | 0.0510 | −1.2553 | R2e | 1.26 | −0.1330 | 0.1914 | 0.6947 |
R1f•− | 0.77 | 0.0619 | 0.0675 | −0.9170 | R2f•− | 0.20 | 0.0438 | 0.1279 | −0.3425 |
R1g•− | 0.74 | 0.0577 | 0.0611 | −0.9448 | R1a | 2.21 | −0.1699 | 0.1780 | 0.9545 |
As shown in Table 3, according to the scale proposed by Domingo et al.,36 the radical anion reactants are moderate electrophiles except those with strong electron-withdrawing substituents which can be considered as nucleophiles (marginal electrophiles). The neutral reactants are all strong electrophiles. The maximum charges ΔNmax of the neutral reactants are positive, and the values decrease with the global electrophilicity, which is consistent with the previous work.36 The radical anion reactants are all negative, indicating that the electron may transfer from the radical anion towards the environment. However, the trend that the absolute values decrease with the global electrophilicity is conserved. Since the two reactants are classified as a strong and a moderate electrophile or a strong and a marginal electrophile, respectively, the [2 + 2] cycloaddition will present a charge transfer pattern. The chemical potential of the neutral reactants are lower than that of the radical anion reactants, indicating that the charge will take place from the radical anion towards the neutral reactants. To evaluate this charge transfer, we calculated the index ΔN0 according to the formula:37 ΔN0 = (μ1 − μ2)/(η1 + η2). As shown in Table 4, the value of ΔN0 also confirms the charge transfer from the radical anion towards the neutral reactants. The large difference in electrophilicity (Δω) within the two reactants (see Table 4) suggests the polar character of the cycloaddition, which is consistent with the charge transfer analysis.
Reactions | Δω [ev] | ΔN0 [e] | Reactions | Δω [ev] | ΔN0 [e] |
---|---|---|---|---|---|
1 (R1a•− + R2a) | 1.18 | 0.90 | 9 (R1a•− + R2c) | 1.01 | 0.81 |
2 (R1b•− + R2a) | 1.39 | 0.85 | 10 (R1a + R2d•−) | 1.94 | 0.76 |
3 (R1c•− + R2a) | 1.01 | 0.96 | 11 (R1a•− + R2e) | 0.41 | 0.76 |
4 (R1d•− + R2a) | 1.99 | 0.70 | 12 (R1a + R2f•−) | 2.01 | 0.70 |
5 (R1e•− + R2a) | 0.94 | 0.96 | 13 (R1a•− + R1a) | 1.36 | 0.95 |
6 (R1f•− + R2a) | 1.26 | 0.89 | 14 (R1b•− + R1b) | 1.75 | 0.93 |
7 (R1g•− + R2a) | 1.29 | 0.90 | 15 (R1c•− + R1c) | 0.94 | 1.00 |
8 (R1a•− + R2b) | 0.88 | 0.84 | 16 (R1f•− + R1f) | 1.42 | 0.94 |
The relative free energies of the main structures along reactions 1–16 are shown in Table 5. Take reaction 1 for instance, as shown in the potential energy profile (see Fig. 1), the formation of PC-1 is associated with a slight decrease of the enthalpy and a positive relative free energy in gas phase, indicating the impossibility as stable intermediate. According to our calculational results, the PC-1 valley in the energy profiles disappears in the solvent, and the activation barriers are also decreased by the solvent (see Table 5 and Table S2†). We use PC-1 as the start of the cycloaddition and the free energies in solvent at 298 K to discuss the reaction process. From PC-1, the activation barrier to form the acyclic intermediate IM-1 is predicted to be 3.2 kcal mol−1. The TS1-1 and IM-1 are all polar, confirmed by the dipole moments (μ > 4D) and charge transfer indexes (t = 0.43e, t = 0.52e) shown in Table S1.† Subsequently, there is a bifurcation from IM-1, which leads to the trans product with lower polarity and cis product with higher polarity, respectively. The charge transfer indexes show that the charge transfer increased in the second transition states and decreased when the products are formed. The activation barrier to form P-trans-1 is 3.8 kcal mol−1, and the activation barrier to form P-cis-1 is 6.8 kcal mol−1. It is obvious that the barrier to form P-cis-1 is much higher than that to form P-trans-1, indicating that the reaction pathway to form P-trans-1 is more dynamically favorable. Additionally, P-trans-1 is more thermodynamically stable than P-cis-1. Therefore, the cycloaddition to form P-trans-1 has an absolute advantage over that to form P-cis-1, which is in agreement with the experimental result that P-trans-1 is the mainly observed product for the cycloaddition of R1a and R2a. The cycloaddition processes of the rest reactions 2–16 are analogous to that of reaction 1. Thus, we won't discuss these processes in detail again. Considering that the relative free energies of TS2-trans are lower than those of TS1 for all the reactions, we only use the relative free energy of TS1 to discuss the reactivity of the cycloaddition in the following.
Reactions | R1 + R2 | PC | TS1 | IM | TS2-trans | P-trans | TS2-cis | P-cis |
---|---|---|---|---|---|---|---|---|
1 (R1a + R2a) | 0 | 0.8 | 4.0 | −2.5 | 1.3 | −5.2 | 4.3 | −2.3 |
(0) | (−7.2) | (−3.9) | (−9.0) | (−5.5) | (−10.6) | (−0.7) | (−6.5) | |
2 (R1b + R2a) | 0 | −0.8 | 5.0 | −1.5 | 1.9 | −5.7 | 4.8 | −2.8 |
(0) | (−6.4) | (−2.0) | (−7.1) | (−4.2) | (−10.4) | (0.6) | (−6.4) | |
3 (R1c + R2a) | 0 | −0.7 | 2.0 | −4.5 | 0.1 | −4.0 | 3.4 | −1.0 |
(0) | (−8.2) | (−5.4) | (−10.5) | (−6.6) | (−10.0) | (−1.5) | (−5.9) | |
4 (R1d + R2a) | 0 | −0.7 | 21.4 | 16.0 | 16.7 | −9.5 | 18.6 | −5.8 |
(0) | (−4.5) | (12.0) | (8.7) | (8.8) | (−11.1) | (12.5) | (−7.5) | |
5 (R1e + R2a) | 0 | −1.0 | 1.2 | −5.3 | −0.4 | −3.8 | 3.0 | −0.7 |
(0) | (−9.6) | (−6.3) | (−11.4) | (−7.2) | (−10.2) | (−2.1) | (−6.0) | |
6 (R1f + R2a) | 0 | 1.6 | 5.9 | −0.2 | 1.8 | −4.9 | 4.8 | −1.9 |
(0) | (−5.9) | (−2.4) | (−7.2) | (−4.9) | (−10.0) | (0.0) | (−5.9) | |
7 (R1g + R2a) | 0 | −1.3 | 13.1 | −0.1 | 3.0 | −3.9 | 10.3 | −0.9 |
(0) | (−7.9) | (1.1) | (−2.9) | (−4.1) | (−9.3) | (0.9) | (−5.2) | |
8 (R1a + R2b) | 0 | 1.9 | 12.8 | 6.1 | 7.5 | 1.9 | 13.3 | 9.0 |
(0) | (−5.8) | (2.0) | (−3.6) | (−2.1) | (−6.4) | (4.7) | (1.8) | |
9 (R1a + R2c) | 0 | 0.4 | 7.2 | 1.6 | 5.3 | −4.0 | 7.5 | −0.4 |
(0) | (−6.5) | (−1.6) | (−5.7) | (−1.8) | (−7.0) | (2.5) | (−4.4) | |
10 (R1a + R2d) | 0 | 0.1 | 18.6 | 10.4 | 16.1 | −5.0 | 18.2 | −3.5 |
(0) | (−16.4) | (4.5) | (−0.5) | (5.7) | (−7.1) | (6.7) | (−4.0) | |
11 (R1a + R2e) | 0 | −6.4 | 21.2 | 17.8 | 17.8 | 11.0 | 20.0 | 14.6 |
(0) | (−19.5) | (8.0) | (5.6) | (5.7) | (1.9) | (9.2) | (3.6) | |
12 (R1a + R2f) | 0 | 0.0 | 25.7 | 22.5 | 23.8 | 16.6 | 29.3 | 23.5 |
(0) | (−10.1) | (16.9) | (9.5) | (12.8) | (8.1) | (18.9) | (17.2) | |
13 (R1a + R1a) | 0 | 3.5 | 10.9 | 1.9 | 3.6 | −1.5 | 10.1 | 5.9 |
(0) | (−8.9) | (−0.5) | (−7.4) | (−6.7) | (−12.2) | (1.7) | (−2.4) | |
14 (R1b + R1b) | 0 | 3.3 | 10.5 | 1.4 | 3.6 | −0.5 | 10.0 | 7.7 |
(0) | (−9.1) | (−1.1) | (−8.1) | (−8.1) | (−14.0) | (0.2) | (−4.9) | |
15 (R1c + R1c) | 0 | 3.4 | 11.1 | 2.1 | 2.2 | −2.3 | 9.5 | 4.0 |
(0) | (−7.3) | (0.1) | (−7.6) | (−6.6) | (−11.2) | (2.1) | (−0.8) | |
16 (R1f + R1f) | 0 | 3.8 | 12.2 | 3.7 | 4.9 | −0.4 | 11.5 | 7.1 |
(0) | (−8.3) | (−0.3) | (−6.7) | (−6.5) | (−11.9) | (1.9) | (−2.5) |
![]() | ||
Fig. 1 Free energy profiles for the reaction 1 leading to the stereoisomers. Enthalpies are displayed in parentheses. All the energies are given in kcal mol−1 in gas phase. |
As shown in Table 5, the first activation barriers of reactions 1–3 and 5 are 3.2, 5.8, 2.7 and 2.2 kcal mol−1, respectively; the second activation barriers to form the trans products are no more than 4.9 kcal mol−1. The moderate activation barriers indicate that both electron-withdrawing and electron-donating substituted enones could undergo cycloadditions. However, the first activation barrier of reaction 4 with nitryl on the phenyl is predicted to be 22.1 kcal mol−1, which is 18.9 kcal mol−1 higher than that of reaction 1, indicating that too strong electron-withdrawing is unfavorable for the cycloaddition. Considering that all the stereo structures along these reactions are similar, the difference in reactivity must be caused by the electronic effect. It is subjected to further investigation into the electronic structures. Therefore, we performed NBO calculations to get the NBO charges on the moiety of the key structures.
As we have declared in our previous investigation for the intramolecular cycloaddition of bis(enone),19 the cycloaddition reactivity is influenced by the charges on the reaction centre (RC) including C1, C2, C3 and C4 atoms (see notations in Fig. 2). We only present the NBO charges on these four atoms in this work. As shown in Table 6, the NBO charges on RC of the key structures are almost −1e, suggesting that the additional electron mainly focuses on the reaction centre along the cycloaddition.
![]() | ||
Fig. 2 Optimized geometries of the important transition states with selected bond distances given in angstrom. |
Reactions | Atom | TS1 | IM | TS2-trans | P-trans | TS2-cis | P-cis |
---|---|---|---|---|---|---|---|
1 (R1a + R2a) | C1 | −0.177 | −0.243 | −0.249 | −0.218 | −0.253 | −0.225 |
C2 | −0.342 | −0.290 | −0.221 | −0.242 | −0.220 | −0.240 | |
C3 | −0.345 | −0.416 | −0.393 | −0.374 | −0.394 | −0.379 | |
C4 | −0.389 | −0.264 | −0.298 | −0.313 | −0.306 | −0.293 | |
RC | −1.253 | −1.213 | −1.161 | −1.147 | −1.173 | −1.137 | |
2 (R1b + R2a) | C1 | −0.117 | −0.240 | −0.250 | −0.216 | −0.254 | −0.223 |
C2 | −0.338 | −0.299 | −0.220 | −0.242 | −0.219 | −0.241 | |
C3 | −0.344 | −0.419 | −0.395 | −0.373 | −0.396 | −0.379 | |
C4 | −0.384 | −0.249 | −0.294 | −0.312 | −0.302 | −0.293 | |
RC | −1.183 | −1.207 | −1.159 | −1.143 | −1.171 | −1.136 | |
3 (R1c + R2a) | C1 | −0.175 | −0.243 | −0.246 | −0.219 | −0.251 | −0.226 |
C2 | −0.351 | −0.290 | −0.226 | −0.241 | −0.225 | −0.239 | |
C3 | −0.348 | 0.415 | −0.390 | −0.374 | −0.393 | −0.380 | |
C4 | −0.390 | −0.270 | −0.299 | −0.312 | −0.307 | −0.294 | |
RC | −1.264 | −1.218 | −1.161 | −1.146 | −1.176 | −1.139 | |
4 (R1d + R2a) | C1 | −0.190 | −0.240 | −0.260 | −0.205 | −0.265 | −0.219 |
C2 | −0.281 | −0.283 | −0.227 | −0.265 | −0.221 | −0.260 | |
C3 | −0.349 | −0.428 | −0.413 | −0.370 | −0.412 | −0.377 | |
C4 | −0.345 | −0.203 | −0.237 | −0.312 | −0.246 | −0.286 | |
RC | −1.165 | −1.154 | −1.137 | −1.152 | −1.144 | −1.142 | |
5 (R1e + R2a) | C1 | −0.175 | −0.244 | −0.245 | −0.219 | −0.250 | −0.226 |
C2 | −0.352 | −0.286 | −0.233 | −0.241 | −0.225 | −0.230 | |
C3 | −0.348 | −0.413 | −0.389 | −0.375 | −0.392 | −0.380 | |
C4 | −0.392 | −0.279 | −0.299 | −0.311 | −0.308 | −0.294 | |
RC | −1.267 | −1.222 | −1.166 | −1.146 | −1.175 | −1.130 | |
9 (R1a + R2c) | C1 | −0.190 | −0.239 | −0.253 | −0.224 | −0.256 | −0.226 |
C2 | −0.340 | −0.310 | −0.222 | −0.223 | −0.216 | −0.227 | |
C3 | −0.349 | −0.416 | −0.389 | −0.371 | −0.389 | −0.377 | |
C4 | −0.408 | −0.285 | −0.329 | −0.318 | −0.335 | −0.297 | |
RC | −1.287 | −1.250 | −1.193 | −1.136 | −1.196 | −1.127 | |
10 (R1a + R2d) | C1 | −0.160 | −0.262 | −0.245 | −0.209 | −0.257 | −0.222 |
C2 | −0.330 | −0.187 | −0.239 | −0.285 | −0.252 | −0.292 | |
C3 | −0.344 | −0.385 | −0.393 | −0.372 | −0.387 | −0.353 | |
C4 | −0.391 | −0.366 | −0.273 | −0.270 | −0.283 | −0.291 | |
RC | −1.225 | −1.200 | −1.150 | −1.136 | −1.179 | −1.158 |
The additional negative charges on RC should be advantageous for the first step of the cycloaddition, as the electron on the π* antibonding orbital could weaken the CC bond. This is confirmed by the calculational results that the reaction with a more negative RC would have the lower first activation barrier. As shown in Table 6, the NBO charges on RC are strongly affected by the electronic structure of the substituents. The electron-donating substituent is helpful for the formation of a more negative RC, which is beneficial for the first step of the cycloaddition. Thereby, the electron-withdrawing substituent would increase the first activation barrier. However, according to the relationship between the NBO charges on RC and the first activation barrier, the first activation barrier of reaction 4 should not be so significantly high as the NBO charges on RC in TS1-4 are not dramatic decreased. By comparing the distribution of the NBO charges we find that the Coulombic repulsion between C1 and C3 also has effect on the first activation barrier. The NBO analysis shows that the Coulombic repulsion between C1 and C3 in TS1-2 is the smallest and that in TS1-4 is the largest among TS1-1 to TS1-5, making the energy of TS1-2 decrease and the energy of TS1-4 increase. Therefore, although the difference in NBO charges on RC between TS1-2 and TS1-4 is not considerable, the first activation barrier of reaction 2 is moderate, while that of reaction 4 is significantly high.
After the C1–C3 bond is formed, the NBO charges on C1 and C3 atoms increase, and the NBO charges on C2 and C4 atoms decrease, which is favorable for weakening the Coulombic repulsion between C2 and C4, benefiting the formation of C2–C4 bond. In the second cycloaddition step, the NBO charges on RC are decreased. The reaction 4, with less negative NBO charges on RC and weak Coulombic repulsion between C2 and C4 in the second transition states, has the lowest second activation barrier comparing to reactions 1–3 and 5, indicating that the electron-withdrawing substituent is beneficial for the second cycloaddition step.
To investigate the electronic effect of the reacting partner on the cycloaddition, we also performed NBO analysis on the key structures of reactions 9 and 10 with methoxyl and nitryl substituents at R3-position. The effect of the methoxyl on RC is strong, as the NBO charges on RC in TS1-9 are the most negative shown in Table 6. With the increasing of the charges on RC, the NBO charges on C1 and C3 become more negative as well, leading to the stronger Coulombic repulsion between C1 and C3. Therefore, although the NBO charges on RC in TS1-9 are more negative than those in TS1-1, the first activation barrier of reaction 9 is 3.6 kcal mol−1 higher. The NBO charges on RC in TS1-10 are a little less negative than those in TS1-1 caused by the effect of the nitryl at R3-position. However, this insignificant effect on the NBO charges on RC could not explain the significant higher in the free energy of TS1-10 than TS1-1. Then, we check the structure of TS1-10 and find that the C–N bond is 1.61 Å, which is much longer than that in PC-10 (1.45 Å). The elongation of the C–N bond may be caused by the increasing Coulombic repulsion between the C and N atoms, as the NBO charges on C and N atoms in TS1-10 are 0.525 and 0.418e, which are more positive than those in PC-10 (0.498e, 0.342e). This strong Coulombic repulsion weakens the C–N σ bond interaction, increasing the energy of TS1-10.
In conclusion, the first cycloaddition step needs a more negative RC, while the second cycloaddition step needs a less negative RC. Both of the electron-donating and electron-withdrawing substituents are amenable to cycloaddition, which is consistent with the experimental result. However, too strong electron-withdrawing substituents at either of the two dissimilar enones significantly increase the first activation barrier, indicating that the nitryl is unfavorable for the cycloaddition. This conclusion confirms our previous conjecture in the investigation of the bis(enones) again.19
As we talked above, the cycloaddition is sensitive to the steric bulk at R2- and R4-position, but the methyl is amenable. Considering that the R2-position is equal to the R4-position in influencing the cycloaddition, we only change the substituents at R4-position to discuss the effect on the reaction reactivity. In order to check the possibility of constructing other full-substituted cyclobutanes by the radical anion cycloaddition, we tried to add the amino and nitryl to the R4-position. As shown in Table 5, the first activation barriers of reactions 11 and 12 are significantly higher than that of reaction 1, which should be caused by both of the electronic effect and steric effect. Considering that the steric hindrance caused by the amino and nitryl has no big difference to the methyl, the energy difference between TS1-11, TS1-12 and TS1-8 should be attributed to the electronic effect.
The NBO charges on RC in TS1-11 and TS1-12 are −0.901 and −0.936e, respectively, which are considerably less negative than the reactions shown in Table 6, explaining the significant high first activation barriers of reactions 11 and 12. Specially, the NBO charges on C3 in TS1-11 and TS1-12 are 0.015 and −0.080e, respectively, notably influenced by the substituents on C3 atom, while those on C1 atom are −0.198 and −0.101e, respectively. The stronger Coulombic repulsion between C1 and C3 in TS1-12 may just explain why the relative free energy of TS1-12 is 4.6 kcal mol−1 higher than that of TS1-11. For that the energy difference between TS1-11, TS1-12 and TS1-8 is similar to that between TS1-8 and TS1-1, the contribution of electronic effect and steric effect on the reaction reactivity should be equivalent.
Additionally, it should be mentioned that the relative free energy of PC-11 are considerably lower than those in other reactions, which is caused by the formation of the hydrogen bond between the H atom of amino and the O atom of carbonyl in the complexes as we talked above. The stabilization of the complex is unfavorable for the cycloaddition, since it will need more energy to break the hydrogen bond and undergo the following reaction.
As shown in Table 5, the fist activation barriers for the crossed cycloadditions (reactions 1, 2, 3, 6 and 9) are 3.2, 5.8, 2.7, 4.3 and 6.8 kcal mol−1, respectively; the fist activation barriers for the corresponding self cycloadditions (reactions 13, 14, 15, 16 and 13) are 7.4, 7.2, 7.7, 8.4 and 7.4 kcal mol−1, respectively. The first activation barriers of the crossed cycloaddition above are all lower than their corresponding self cycloadditions, indicating the chemoselectivity to form the crossed cycloaddition products as the main product. As we talked above, the first activation barrier is strongly affected by the steric hindrance at R2- and R4-position. This well explains the predomination of the crossed cycloaddition with substituents only at R2-position over the self cycloaddition with substituents at both of R2- and R4-positions. Therefore, considering the bulky substituents at R2-position in R1g, the self cycloaddition of R1g should be extremely unfavorable.
The first activation barrier of reaction 8 is 0.8 kcal mol−1 higher than that of reaction 13, suggesting the self cycloaddition of R1a has slight advantage over its crossed cycloaddition with R2b, which is in agreement with the experimental result. It is obvious that the difference of the steric hindrance in the first step of these two reactions is ignorable. Thus, we tried to explain the predomination of the self cycloaddition from the NBO analysis. However, the NBO charges on RC in TS1-8 are more negative than those in TS1-13, which indicates that the relative free energy of TS1-8 even should be lower than that of TS1-13. Nonetheless, the important feature of TS1-13, that is the strong conjugation effect caused by the two existing phenyl substituents, may contribute to reduce the energy of TS1-13. Although the chemoselectivity is not good as the difference in the first activation barrier between reactions 8 and 13 is small, the stereoselectivity for each cycloaddition is still excellent, which will be discussed in the following part.
According to the NBO charges displayed in Table 6, the NBO charges on RC in TS2-trans are less negative than those in TS2-cis. As we talked above, the less negative RC is beneficial for the second cycloaddition step, suggesting that the energy of TS2-trans should be lower than that of TS2-cis. Additionally, the Coulombic repulsion between C2 and C4 in TS2-trans is a little weaker than that in TS2-cis, which also contributes to reduce the energy of TS2-trans. However, the energy difference between the TS2-trans and TS2-cis changes slightly for reactions 1–5 with significant different electronic structures, indicating that the electronic effect on the stereoselectivity is restricted. Thus, we predict that the stereoselectivity is primarily influenced by the steric hindrance.
As shown in Fig. 2, in TS2-cis-1, the carbonyl substituents on C2 and C4 are in the same side. The distance between the two O atoms is 4.10 Å, showing the stronger steric interaction. While in TS2-trans-1, the carbonyl substituents on C2 and C4 are in the different side. The distance between the two O atoms is 5.64 Å, showing the weaker steric interaction. The difference in steric interactions contributes to the excellent stereoselectivity. The experimental results show that the stereoselectivity of reaction 9 is not so excellent as other reactions (reactions 1–3 and 6–8), which is confirmed by our calculational result that the energy difference between TS2-trans-9 and TS2-cis-9 is smaller than that in reactions 1–3 and 6–8. To understand the origin of the unusual stereoselectivity, we herein examine the structures of diastereomeric TS2-trans-9 and TS2-cis-9 (Fig. 2). In TS2-trans-9, although the steric hindrance between the carbonyl substituents on C2 and C4 are weaker than that in TS2-cis-9, the steric hindrance between the phenyl and the methyl on O atom is much stronger than that in TS2-cis-9. The cooperation of these two factors decreases the energy difference between TS2-trans-9 and TS2-cis-9. Therefore, the stereoselectivity of reaction 9 is not excellent.
The reason causing the decrease of the energy difference between TS2-trans-4 and TS2-cis-4 is analogous to that in reaction 9. Furthermore, the distances between C2 and C4 in TS2-trans-4 and TS2-cis-4 are the longest among those in all reactions, suggesting that the steric effect on the stereoselectivity of reaction 4 becomes weak. This could explain that the energy difference between TS2-trans-4 and TS2-cis-4 is smaller than that in reaction 9. The energy of TS2-trans-10 is 2.1 kcal mol−1 lower than that of TS2-cis-10, which is little smaller than the energy difference between TS2-trans-9 and TS2-cis-9, indicating that the stereoselectivity is not good either. The distance between the H atom on phenyl and the O atom on nitryl in TS2-cis-10 is shorter than that in TS2-trans-10, indicating the stronger Coulombic attraction between the H and O atoms in TS2-cis-10. Thus, the energy difference between TS2-trans-10 and TS2-cis-10 is decreased, which is unfavorable for keeping the stereoselectivity.
The reaction 8 with ethyl R3-position is predicted to demonstrate excellent stereoselectivity since the TS2-trans-8 is favored by 5.8 kcal mol−1 to TS2-cis-8. It is interesting to discover the similar improving trend in stereoselectivity in reaction 13–16 substituted by phenyl at R3-position, where the TS2-trans-(13–16) is 6.5, 6.4, 7.3 and 6.6 kcal mol−1 lower in free energy than TS2-cis-(13–16), respectively. The origin of much lower energies of TS2-trans-(13–16) can be understood on the basis of the strong steric interaction between the two phenyl substituents in the cis structure. Therefore, we can speculate that the steric hindrance at R1- and R3-positions could increase the energy difference between the trans and cis transition states. To improve the stereoselectivity, it is better to introduce bulky substituents at R1- and R3-positions.
The cycloaddition is sensitive to the substituents at R2- and R4-positions by both steric hindrance and electronic effect. To improve the chemoselectivity, it is better to keep the R4-position unsubstituted. The stereoselectivity is mainly caused by the steric hindrance, and the electronic effect only has slight influence on the stereoselectivity. Therefore, in order to improve the stereoselectivity, it is better to introduce bulky substituents at R1- and R3-positions to increase the difference in steric interaction between the trans and cis transition states.
Our investigation shows that the electronic and stereo structures of the substituents have dramatic effect on the radical anion cycloadditions. Especially, the amino and nitryl could be hardly endured. This work provides useful information for choosing substituents to design novel intermolecular [2 + 2] cycloadditions with excellent chemo- and stereoselectivity.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c4ra13816c |
This journal is © The Royal Society of Chemistry 2014 |