Hsu-Cheng Huaa and
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 19th September 2017
The molecular properties and reactive activities of the d-π conjugated (E)-Tip(Fc)E14E14(Fc)Tip (1-C, 1-Si, 1-Ge, 1-Sn, and 1-Pb) systems possessing the E14E14 unit were explored using density functional theory (M06-2X/Def2-SVPD). The theoretical investigations on the basis of several physical properties (the bonding analysis, UV-vis and Raman spectra) indicate that a coupling occurs between the double bonded moiety, E14E14, and the ferrocenyl groups. Moreover, the present theoretical findings strongly suggest that the chemical reactivity of such d-π conjugated molecules increase in the order as follows: 1-C ≪ 1-Si < 1-Ge < 1-Sn < 1-Pb. Specifically, the larger the atomic radius of the group 14 element involved in such d-π conjugated compounds, the smaller its π bond strength and more facile its [1 + 4] or [1 + 2] cycloaddition with either a butadiene or a selenium atom, respectively. The singlet–triplet energy splittings, based on the VBSCD model, have been used as a guide to interpret the reactivity.
This study, therefore, pursues the first systematic theoretical inspection of the d-π-conjugated molecules, (E)-Tip(Fc)E14E14(Fc)Tip (1-C, 1-Si, 1-Ge, 1-Sn, and 1-Pb), using density functional theory (DFT). From the present work, it is hoped that the computed molecular properties, as well as the chemical reactivity, can provide a guide for any future experimental studies of unknown d-π-conjugated compounds possessing a E14E14 unit.
1-C | 1-Si | 1-Ge | 1-Sn | 1-Pb | |
---|---|---|---|---|---|
1 | 1.364 | 2.166 | 2.251 | 2.635 | 2.863 |
[2.173] | [2.332] | ||||
(1.500) | (2.323) | (2.416) | (2.743) | (2.906) | |
2 | 1.503 | 1.824 | 1.934 | 2.142 | 2.262 |
[1.880] | [1.981] | ||||
(1.545) | (1.893) | (1.958) | (2.156) | (2.273) | |
3 | 1.492 | 1.824 | 1.903 | 2.090 | 2.204 |
[1.848] | [1.935] | ||||
(1.501) | (1.851) | (1.928) | (2.121) | (2.229) | |
4 | 125.9° | 121.8° | 119.7° | 113.9° | 114.0° |
[116.3°] | [114.6°] | ||||
(125.8°) | (115.9°) | (116.5°) | (115.0°) | (114.6°) | |
5 | 120° | 118.9° | 105.6° | 96.48° | 95.31° |
[117.0°] | [116.5°] | ||||
(117.3°) | (115.9°) | (116.5°) | (115.0°) | (114.6°) | |
θ | 6.8° | 29.3° | 46.5° | 64.2° | 68.4° |
[27.9°] | [43.7°] | ||||
(7.4°) | (49.1°) | (52.0°) | (61.9°) | (63.4°) |
Firstly, we compared the geometries of 1-Si and 1-Ge with the M06-2X computational results, since only these structures have been determined by X-ray crystal analyses.1 The calculated SiSi and GeGe bond lengths of 1-Si and 1-Ge are 2.166 and 2.251 Å, which are somewhat shorter than the experimental data, 2.173 (ref. 1 and 6) and 2.332 Å,1b respectively, as shown in Table 1. Moreover, it is found that the calculated Si–C and Ge–C (ipso-ferrocenyl) bond distance of 1-Si (1.824 Å) and 1-Ge (1.903 Å) are shorter than those of the Si–C and Ge–C (ipso-Tip) bonds (1.885 Å for 1-Si and 1.934 Å for 1-Ge), whose trend is similar to the experimental observations.1 The reasons for such short values are probably due to conjugative interactions between the π-electrons of the SiSi and GeGe units and those of the ferrocenyl units in both 1-Si and 1-Ge, respectively.1 Additionally, the M06-2X results shown in Table 1 indicate that 1-Si and 1-Ge exhibit a characteristic trans-bent structure with a trans-bent angle (θ) of 29.4° and 46.5°, which are analogous to the reported X-ray analyses, 27.9° (ref. 1a) and 43.7°,1b respectively.7 From the above comparisons, the reasonably good agreement between the experimental data and the computational results is quite encouraging.8,9 It is, therefore, certain that the theoretical method (M06-2X/Def2-SVPD) used in this work should be reliable for any further investigations of their molecular properties as well as energetic features of the chemical reactions, for which experimental values are not attainable.
The electronic structures of (E)-Tip(Fc)E14E14(Fc)Tip were analyzed using the natural bond orbital (NBO)10 partitioning scheme in combination with the Wiberg bond indices (WBI),11 which are summarized in Table 2. It is apparent that the order of WBI for the E14E14 doubly bonded species decreases from carbon to lead. In particular, only the WBI of 1-Pb is 0.77, being less than 1.0, implying that the bonding between the two lead atoms is best described as a single bond. About the NBO10 analysis given in Table 2, our theoretical findings indicate that there exists a 1:1 p orbital contribution to the π bond in the case of 1-C. On the other hand, the heavier the group 14 element (E14) involved, the higher the asymmetric contributions to the π bond. However, since the 1-C, 1-Sn, and 1-Pb molecules have not been experimentally reported yet and the study of the bonding characters is beyond the scope of the present work, we thus consider the theoretical results collected in Table 2 is a prediction.
E14E14 | Bond length (Å) | WBI | Occupancy | NBO analysis | BDE (kcal mol−1) |
---|---|---|---|---|---|
a All are computed at the M06-2X/Def2-SVPD level of theory.b Wiberg bond index (WBI).c Occupancy of the corresponding σ and π bonding NBO.d Bonding dissociation energy (BDE), units: kcal mol−1. BDE = 2E[(E)-Tip(Fc)E14:] − E[(E)-Tip(Fc)E14E14(Fc)Tip]. | |||||
1-C | 1.364 | 1.71 | σ = 1.96 | 0.707 C(sp1.61) + 0.707 C(sp1.61), where C = 50.00%, C = 50.00% | 132.7 |
π = 1.88 | 0.707 C(sp99.99) + 0.707 C(sp99.99), where C = 49.99%, C = 50.01% | ||||
1-Si | 2.116 | 1.62 | σ = 1.93 | 0.707 Si(sp1.83) + 0.707 Si(sp1.83), where Si = 50.01%, Si = 49.99% | 13.64 |
π = 1.85 | 0.706 Si(sp17.25) + 0.708 Si(sp17.67), where Si = 49.86%, Si = 50.14% | ||||
1-Ge | 2.251 | 1.53 | σ = 1.89 | 0.707 Ge(sp2.02) + 0.707 Ge(sp2.03), where Ge = 49.99%, Ge = 50.01% | −3.08 |
π = 1.83 | 0.708 Ge(sp9.56) + 0.706 Ge(sp9.56), where Ge = 50.17%, Ge = 49.83% | ||||
1-Sn | 2.635 | 1.21 | σ = 1.77 | 0.708 Sn(sp2.20) + 0.706 Sn(sp2.24), where Sn = 50.16%, Sn = 49.84% | −30.23 |
π = 1.73 | 0.709 Sn(sp4.26) + 0.705 Sn(sp4.22), where Sn = 50.26%, Sn = 49.74% | ||||
1-Pb | 2.863 | 0.77 | σ = 1.97 | 0.699 Pb(sp1.66) + 0.715 Pb(sp1.81), where Pb = 48.82%, Pb = 51.18% | −30.45 |
π = 1.64 | 0.716 Pb(sp99.99) + 0.699 Pb(sp1.00), where Pb = 51.20%, Pb = 48.80% |
Specifically, the larger the atomic radius of E14 involved in the (E)-Tip(Fc)E14E14(Fc)Tip species, the longer the E14E14 double bond length, and the smaller the bond order of the E14E14 bond, the weaker the E14E14 double bond strength. Indeed, from the viewpoint of the bond dissociation energy (BDE; kcal mol−1) of the E14E14 double bond, i.e., (E)-Tip(Fc)E14E14(Fc)Tip → 2 × Tip(Fc)E14 (BDE = 2E(Tip(Fc)E14:) − E((E)-Tip(Fc)E14E14(Fc)Tip)), the M06-2X calculations shown in Table 2 reveal that the BDE decreases in the order: CC (133) > SiSi (14) > GeGe (−3.1) > SnSn (−30) > PbPb (−31). From these results, one may readily anticipate that the double bonds for both 1-Sn and 1-Pb can be relatively easily broken, whereas the 1-C π-bonded compound is quite stable in both the solution phase and the solid phase. However, the M06-2X studies show that the BDEs of 1-Si and 1-Ge are roughly equal to zero, demonstrating that the two species can dissociate in solution. These predictions are in good agreement with the available experimental evidence (vide infra).1
Besides these, the M06-2X computational data given in Table 2 reveal that there exists substantially more σ-character within the π bond of the diplumbylene in relation to the other dimetallenes. As a result, this feature should relate to the presence of a weak slipped π-interaction in the 1-Pb species.12
In order to gain a better understanding of the chemical bonding of the (E)-Tip(Fc)E14E14(Fc)Tip compounds, their frontier molecular orbitals (MOs) based on the M06-2X/Def2-SVPD method are schematically illustrated in Fig. 1. In principle, the HOMO and LUMO of these double bonded species predominantly consist of E14E14 p-π and p-π* orbitals, respectively. As shown in Fig. 1, after the replacement of two E14 atoms at the (E)-Tip(Fc)E14E14(Fc)Tip center, the energy of LUMO (the π* orbital) decreases from 1-C to 1-Pb, whereas the energy of HOMO increases in the order: Eπ(1-C) < Eπ(1-Pb) < Eπ(1-Sn) < Eπ(1-Ge) < Eπ(1-Si). As a result, on the basis of M06-2X calculations, the energy gaps (kcal mol−1) between HOMO and LUMO for the (E)-Tip(Fc)E14E14(Fc)Tip molecules are estimated to be 154 (1-C) > 109 (1-Si) > 107 (1-Ge) > 99 (1-Sn) > 98 (1-Pb), whose trend is consistent with that of its singlet–triplet energy splitting (ΔEst = Etriplet − Esinglet),13 i.e., 46 (1-C) > 36 (1-Si) > 34 (1-Ge) > 24 (1-Sn) > 21 (1-Pb). That is to say, the heavier the group 14 atoms (E14E14) involved, the smaller the ΔEst of E14E14 appears to be. Supposing the chemical reactions are “frontier-controlled”, then the ΔEst of the E14E14 systems can be considered as a criterion regarding their reactivity. From the calculations shown above, the M06-2X data indicate that the ΔEst of the 1-Sn and 1-Pb are smaller than those of the other three compounds (1-C, 1-Si, and 1-Ge). This theoretical evidence strongly suggests that the (E)-Tip(Fc)E14E14(Fc)Tip (E14 = C, Si, and Ge) compounds are stable enough to be detected, while 1-Sn and 1-Pb molecules are kinetically unstable and easily react with the other species (such as the solvent molecules). Again, these findings agree well with the theoretical data given in Table 2 as well as the available experimental observations.1
Fig. 1 Calculated frontier molecular orbitals for the (E)-Tip(Fc)E14E14(Fc)Tip (1-C, 1-Si, 1-Ge, 1-Sn, and 1-Pb) species at the M06-2X/Def2-SVPD level of theory. For more information see the text. |
UV spectroscopy may be one of the most valuable methods for detecting the double-bond character of dimetallenes.14 The UV-vis spectra of E14E14 (1-C, 1-Si, 1-Ge, 1-Sn, and 1-Pb), investigated by using the M06-2X/Def2-SVPD level of theory, are summarized in Table 3, accompanied by available experimental findings.1 In the case of 1-Si, the M06-2X spectrum contains two intense absorption peaks at 427 nm (ε = 14312, SiSi π(HOMO) → SiSi π*(LUMO)) and 227 nm (ε = 31720, SiSi π(HOMO) → d-π* orbitals of metallocenyl moiety). In addition, a weak and broadened absorption peak is seen at 308 nm (ε = 2531, SiSi π(HOMO) → d-π*orbitals of metallocenyl moiety and d-π orbitals of metallocenyl unit → SiSi π*(LUMO)). In the case of 1-Ge, the same level computations show that there are two strong absorption peaks at 449 nm (ε = 14692, GeGe π(HOMO) → GeGe π*(LUMO)) and 223 nm (ε = 33570, d-π orbitals of metallocenyl moiety → GeGe π*(LUMO)). As there are no relevant experimental or theoretical data for the UV-vis absorption spectra regarding the (E)-Tip(Fc)E14E14(Fc)Tip (E14 = C, Sn, and Pb) systems, the data given in Table 3 are predictions.
Molecular | Wavelength (nm) molar absorptivity (M−1 cm−1) | Transition |
---|---|---|
a All are computed at the M06-2X/Def2-SVPD level of theory.b Experimental data are shown in the square bracket. Experimental data see: ref. 1b.c Experimental data are shown in the square bracket. Experimental data see: ref. 1b. | ||
1-C | 276.4 (ε = 25617) | CC π(HOMO) → CC π*(LUMO) |
191.1 (ε = 59353) | d(Fe) + π(CC) → d(Fe) + π*(CC) | |
1-Si | 427.3 (ε = 14312) | SiSi π(HOMO) → SiSi π*(LUMO) |
[427 (ε = 24000)]b | ||
308.2 (ε = 2531)b | d(Fe) + π(SiSi) → SiSi π*(LUMO) | |
[332 (ε = 5900)] | SiSi π(HOMO) → d(Fe) + π*(SiSi) | |
227.1 (ε = 31720) | SiSi π(HOMO) → d(Fe) + π*(SiSi) | |
1-Ge | 449.0 (ε = 14692) | GeGe π(HOMO) → GeGe π*(LUMO) |
[430 (ε = 17000)]c | ||
[500 (sh)]c | ||
222.5 (ε = 33570) | d(Fe) + π(GeGe) → GeGe π*(LUMO) | |
1-Sn | 508.4 (ε = 13437) | SnSn π(HOMO) → SnSn π*(LUMO) |
232.9 (ε = 28889) | SnSn π(HOMO) → d(Fe) + π*(SnSn) | |
d(Fe) + π(SnSn) → SnSn π*(LUMO) | ||
1-Pb | 465.2 (ε = 11231) | PbPb π(HOMO) → PbPb π*(LUMO) |
208.2 (ε = 24592) | d(Fe) + π(PbPb) → d(Fe) + π*(PbPb) |
Table 4 displays the computed Raman spectra of E14E14 (1-C, 1-Si, 1-Ge, 1-Sn, and 1-Pb) using the M06-2X/Def2-SVPD method, compared with the reported experimental Raman data. However, the M06-2X calculations indicate that the νSiSi vibrational frequencies of 1-Si are estimated to be 648 and 724 cm−1, which are slightly higher than the experimentally observed νSiSi value (595 and 665 cm−1).1,15 Their vibrational motions are given in Fig. A and B (ESI†), respectively. Again, since to date no Raman spectra of other species (1-C, 1-Ge, 1-Sn, and 1-Pb) have been evaluated and reported, the theoretical data given in Table 4 can be a guide for further experimental studies.
Molecular | Frequency (cm−1) |
---|---|
a All are computed at the M06-2X/Def2-SVPD level of theory.b Experimental data are shown in the square bracket. Experimental data see: ref. 1b. | |
1-C | 1513.1 (C–C stretch) |
1681.2 (CC stretch) | |
3043.8 (C–H stretch) | |
3130.5 (C–H stretch) | |
3031.8 (C–H stretch) | |
1-Si | 648.4 (SiSi stretch) |
[595]1d | |
723.7 (SiSi stretch) | |
[665]1d | |
1248.6 (C–C stretch) | |
2950.7 (C–H stretch) | |
3046.5 (C–H stretch) | |
1-Ge | 1231.4 (C–C stretch) |
2977.5 (C–H stretch) | |
3045.1 (C–H stretch) | |
3141.3 (C–H stretch) | |
3272.6 (C–H stretch) | |
1-Sn | 1413.7 (C–H band) |
2951.5 (C–H stretch) | |
3043.9 (C–H stretch) | |
3138.3 (C–H stretch) | |
3275.0 (C–H stretch) | |
1-Pb | 1688.2 (CC stretch) |
3019.9 (C–H stretch) | |
3044.1 (C–H stretch) | |
3131.3 (C–H stretch) | |
3266.1 (C–H stretch) |
The cycloaddition addition of 2,3-dimethyl-1,3-butadiene with 1 studied in this work follows the general reaction paths (path I, path II, and path III) as represented in Scheme 3. That is to say, 1 would first produce both two equivalent heavy carbene analogues ((Tip)(Fc)E14:, 2)16 and one corresponding 1,2-migration intermediate ((Tip)2(Fc)E14–E14(Fc), 3). Subsequently, these then react with butadiene to yield two types of [1 + 4] cycloproducts (4 and 5), instead of the [2 + 4] cycloformation (6). Theoretical studies regarding the potential energy surfaces for the d-π electron systems containing the E14E14 double bond are shown in the following sections.
Reaction | 1-C | 1-Si | 1-Ge | 1-Sn | 1-Pb |
---|---|---|---|---|---|
a The Gibbs free energies.b ΔEst = Etriplet − Esinglet; see ref. 13 and 17. | |||||
1 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 |
2 (ΔH1) | +132.7 | +13.6 | −3.1 | −30.2 | −30.5 |
2 (ΔEst)b | −11.2 | +27.2 | +29.0 | +32.7 | +39.6 |
TS2 (ΔE2) | +10.1 | +16.5 | +17.1 | +19.0 | +25.7 |
4 (ΔH3) | −72.2 | −56.1 | −39.6 | −12.6 | +20.6 |
(i) As discussed earlier, due to the relative weakness of the heavier E14E14 double bond, the 1 d-π electron species should, presumably, produce the heavy carbene analogue (Tip(Fc)E14:; 2). As discussed earlier, from a chemical bonding viewpoint where the π bond strength of a double bond decreases from CC to PbPb, the reason is that when heavier group 14 elements (E14) are involved, it can lead to longer double bond distances.18 As a result, the greater the atomic mass of E14 involved in the double bond of a 1 compound, the weaker its π bond and the smaller the singlet–triplet energy splitting (ΔEst). In fact, as shown earlier, on the basis of both BDE (Table 1 and ΔH1 in Table 5) and ΔEst (Table 1)13,17 analysis of the reactant molecule, one may readily obtain the conclusion that the ease of breaking the E14E14 double bond of 1 should decrease in the order: 1-Pb > 1-Sn > 1-Ge > 1-Si > 1-C.
(ii) Fig. 2 presents the relative energies of the valence molecular orbitals in the series of the 2 molecules (2-C, 2-Si, 2-Ge, 2-Sn, and 2-Pb) based on the M06-2X/Def2-SVPD calculations. As seen in Fig. 2, the replacement of a single E14 atom at the center of 2 greatly decreases the energy of the HOMO (sp-σ orbital) when going from 2-C to 2-Pb for the sake of the relativistic effect.9 However, this substitution keeps the energy of the LUMO (p-π orbital) roughly constant along the group 14 elements. It is, therefore, anticipated that the energy gap between the HOMO and LUMO of 2 should increase from 2-C to 2-Pb. Indeed, this prediction is consistent with the trend of the calculated ΔEst (kcal mol−1) for the 2 species, as already shown in Table 4.
Fig. 2 Calculated frontier molecular orbitals for the 2 (Tip(Fc)E14:; 2-C, 2-Si, 2-Ge, 2-Sn, and 2-Pb) species at the M06-2X/Def2-SVPD level of theory. For more information see the text. |
(iii) Considering both the calculated activation energies and the reaction enthalpies based on the M06-2X computational results given in Table 5, it is concluded that, for the [1 + 4] cycloaddition reaction of 2, the reactivity decreases in the order: 2-C > 2-Si > 2-Ge > 2-Sn ≫ 2-Pb. In order to verify the important factor that determines the general feature of path I, a valence bond state correlation diagram (VBSCD) model13,16 was used to obtain a deeper understanding of the reactivity of 2. From Table 5, it is apparent that the smaller the value of ΔEst of 2, the lower its barrier height the more exothermic the reaction, and thus the faster the [1 + 4] reaction with a butadiene.
Reaction | 1-C | 1-Si | 1-Ge | 1-Sn | 1-Pb |
---|---|---|---|---|---|
a The Gibbs free energies.b ΔEst = Etriplet − Esinglet; see ref. 13 and 17. | |||||
1 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 |
TS1 (ΔE1) | +234.1 | +44.6 | +33.4 | +7.1 | −8.0 |
3 (ΔH2) | +110.3 | −10.3 | −18.8 | −25.9 | −38.4 |
3 (ΔEst)b | −13.5 | −6.1 | +2.3 | +13.1 | +14.7 |
TS3 (ΔE3) | +39.1 | +45.6 | +52.5 | +61.9 | +63.7 |
5 (ΔH4) | −59.5 | −43.8 | −18.9 | +2.1 | +19.8 |
(i) In path II, the first step of reaction (1 → TS1 → 3) is that 1 undergoes a 1,2-Tip migration before it reacts with 2,3-dimethyl-1,3-butadiene, in which the Tip substituent migrates from one E14 atom to the other E14 atom. From Table 6, taking activation energy and reaction enthalpy into consideration, it can be readily seen that the greater the atomic mass of the group 14 element (E14) involved in the 1 species, the smaller the migration barrier and the larger the exothermicity of the 1,2-shift. The reason for such a phenomenon can be attributed to the bond strength of the E14E14 double bond. As mentioned earlier, due to the examination of both BDE (Table 2 and ΔH1 in Table 5) and ΔEst (Table 1) for the 1 systems,13,17 one can easily obtain the conclusion that the E14E14 π bond strength of 1 decreases in the order: 1-C > 1-Si > 1-Ge > 1-Sn > 1-Pb. It is therefore expected that 1 ((E)-Tip(Fc)E14E14(Fc)Tip) with two heavier E14 centers greatly favors the 1,2-Tip shift to form carbene analogue 3 ((Tip)2(Fc)E14–E14(Fc)). This prediction has been confirmed by examining the migration barriers (ΔE1) as well as the corresponding enthalpies (ΔH2), as already shown in Table 5.
(ii) Fig. 3 shows the relative energies of HOMO and LUMO in the series of the 3 molecules (3-C, 3-Si, 3-Ge, 3-Sn, and 3-Pb) at the M06-2X/Def2-SVPD level of theory. Again, it can be readily seen that the substitution of two E14 atoms in 3 can result in the decrease of both HOMO and LUMO energies owing to the relativistic effect,9 as already stated earlier. The M06-2X/Def2-SVPD computations given in Table 6 indicate that the ΔEst (kcal mol−1) for the 3 compounds increases rapidly from 3-C down to 3-Pb.
Fig. 3 Calculated frontier molecular orbitals for the 3 ((Tip)2(Fc)E14–E14(Fc); 3-C, 3-Si, 3-Ge, 3-Sn, and 3-Pb) species at the M06-2X/Def2-SVPD level of theory. For more information see the text. |
(iii) As seen in Scheme 3, the next step of path II is that 3 reacts with 2,3-dimethyl-1,3-butadiene to encounter the [1 + 4] cycloaddition reaction to produce another cycloproduct 5. Again, from Table 6, taking both the activation barrier and reaction enthalpy into account, it is obvious that the larger the atomic number of the group 14 element (E14) contained in the 3 species, the higher the [1 + 4] barrier height (ΔE3), the less exothermicity (ΔH4), and a higher barrier [1 + 4] cycloaddition is obtained. In fact, these phenomena can be interpreted by using the VBSCD model,13,17 as shown earlier. In other words, the present theoretical investigations demonstrate that the heavier the group 14 elements occupying the heavy 3 system, the larger its singlet–triplet energy splitting (ΔEst), the larger its activation energy (ΔE3), and the smaller its reaction enthalpy (ΔH4), which, in turn, results in a slower [1 + 4] cycloaddition reaction with a butadiene.
(iv) When comparing the computational data for the mechanisms of path I and path II (Scheme 3, Tables 5 and 6), it is evident to see that both the activation energies and exothermicities for path I (ΔE2 and ΔH3) are smaller and larger, respectively, than those for path II (ΔE3 and ΔH4). It is thus predicted that the cycloproduct (4) produced by path I should be in a larger yield than the other cycloproduct (5) formed by path II. This anticipation is in good agreement with the experimental evidence for the 1-Ge system.1b
Reaction | 1-C | 1-Si | 1-Ge | 1-Sn | 1-Pb |
---|---|---|---|---|---|
a The Gibbs free energies.b ΔEst = Etriplet − Esinglet; see ref. 13 and 17. | |||||
1 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 |
1 (ΔEst)b | +43.0 | +32.9 | +30.3 | +18.2 | +15.5 |
TS4 (ΔE4) | +193.4 | +44.6 | +39.9 | +17.5 | −6.5 |
6 (ΔH5) | +122.3 | +40.1 | −18.5 | −45.3 | −51.7 |
(i) As illustrated in Table 7, considering both the activation energies and reaction enthalpies for the path III mechanism, it is convenient to see that the reactivity of 1 increases in the order: 1-C ≪ 1-Si < 1-Ge ≪ 1-Sn < 1-Pb. In particular, it is interesting to find that the activation barrier (193 kcal mol−1) for path III of the 1-C molecule is the highest. The subsequent higher barrier heights are the 1-Si (45 kcal mol−1) and 1-Ge (40 kcal mol−1) compounds, which are still higher than the 1-Sn (18 kcal mol−1) and 1-Pb (−6.5 kcal mol−1) species. Consequently, one can easily foresee that the [2 + 4] cycloaddition reactions for the 1-C, 1-Si, 1-Ge with a butadiene are unlikely to occur, whereas the [2 + 4] cycloproducts through the reactions of 1-Sn and 1-Pb with a butadiene should be effortlessly observable. This prediction agrees with the experimental findings for the 1-Ge case.7c
(ii) According to the VBSCD model13,16 mentioned earlier, from Fig. 1 and Table 7, it is simple to see that the greater the atomic number of E14 atoms contained in 1, the smaller the E14E14 π bond strength, the smaller the HOMO–LUMO energy gap, the smaller the value of ΔEst of 1, the lower its barrier height, the greater its exothermicity, and the faster the [2 + 4] reaction with a butadiene.
(iii) One may ask why the (E)-Tip(Fc)E14E14(Fc)Tip (1) species undergoes the [1 + 4] addition reaction rather than the [2 + 4] cycloaddition reaction as shown in Scheme 1 (ref. 1) and Scheme 3. The reason for this can be attributed to the steric effects between the 2,3-dimethyl-1,3-butadiene and the d-π conjugated systems ((E)-Tip(Fc)E14E14(Fc)Tip) bearing an E14E14 double bond (Scheme 4). Since 2,3-dimethyl-1,3-butadiene contains two methyl groups, which can lead to steric overcrowding with the Fc and Tip bulky substituents of 1, this would thus result in large barrier heights (Table 7) when 1 and 2,3-dimethyl-1,3-butadiene undergo the [2 + 4] cycloaddition. In addition, as discussed earlier, the bonding strength of E14E14 for the heavier group 14 elements are rather weak. Consequently, 1 and 2,3-dimethyl-1,3-butadiene prefer to undergo a [1 + 4] addition rather than to proceed to a [2 + 4] cycloaddition.
Reaction | 1-C | 1-Si | 1-Ge | 1-Sn | 1-Pb |
---|---|---|---|---|---|
a The Gibbs free energies.b ΔEst = Etriplet − Esinglet; see ref. 13 and 17. | |||||
1 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 |
1 (ΔEst)b | +43.0 | +32.9 | +30.3 | +18.2 | +15.5 |
7 (ΔH6) | −20.2 | −61.3 | −76.4 | −129.2 | −145.0 |
(i) As seen in Table 9, the optimized geometrical parameters of 7-Si and 7-Ge are reasonably in agreement with those observed experimentally,1 strongly suggesting that the method (M06-2X/Def2-SVPD) used in this work should give meaningful information on the bonding properties of 7 (vide infra). Moreover, it is obvious from Table 9 that both the Si–Si and Ge–Ge bond distances of 7-Si and 7-Ge are 2.286 (exp. 2.288)1a and 2.385 (exp. 2.370)1b Å, which are slightly shorter than the traditional Si–Si and Ge–Ge single bond lengths (2.33–2.37 Å)20 and (2.43–2.52 Å),21 respectively. The reason for such shorter bond distances is due to the π-complex characters of selenadisilirane and selenadigermirane.1 As a result, the two three-membered cyclic products (7-Si and 7-Ge) were thought to exhibit considerable π-coupling characteristics between E14E14 π bonds and ferrocenyl groups. Nevertheless, repeated attempts to find the transition state for the cycloaddition reaction of 1 with a selenium atom using the M06-2X method were always unsuccessful. Accordingly, the present theoretical investigations indicate that no transition states exist on the M06-2X/Def2-SVPD surface for the [1 + 2] cycloaddition reaction of 1 with a selenium atom.
(ii) The chemical bonding properties of the [1 + 2] products (7) can be readily explained in terms of the Dewar–Chatt–Duncanson model.22 On the basis of this model, their bonding schemes are categorized into two representations: one is a π-complex (8), with the E14E14-to-selenium σ-donation making the greater contribution, and the other is a selenacyclopropane (9), with major selenium-to-E14E14 π-back-donation, as shown in 8 and 9, respectively. In order to identify which pattern is predominant in such three-membered ring products (7), it is better to examine the molecular orbital pictures of their HOMO and LUMO. As seen in Fig. 4, all the computed HOMOs of the 7 species are composed of the σ-orbital of the selenium atom and the p-π orbitals of the E14E14 unit, presenting the π-complex in character. In consequence, the bonding schemes in such [1 + 2] molecules (7) are better characterized as the π-complex bonding (8), rather than the three-membered ring bonding (9). This theoretical finding is consistent with the earlier theoretical examinations by Tokitoh and co-workers.1
Fig. 4 Calculated HOMO and LUMO for the 7 (three-membered cyclic product) molecules at the M06-2X/Def2-SVPD level of theory. For more information see the text. |
(iii) The M06-2X computational results shown in Table 8 reveal that the order of the reactivity for producing cyclic products (7) increases as follows: 1-C ≪ 1-Si < 1-Ge < 1-Sn < 1-Pb. Again, this trend is quite similar to those species shown in Scheme 3 discussed earlier. That is to say, using the VBSCD model,13,17 it is easy to anticipate that the longer the atomic radius of group 14 element (E14) involved in the 1 molecule, the smaller its singlet–triplet energy splitting ΔEst, and the easier the formation of a [1 + 2] three-membered ring product with a selenium atom.
(1) The present computed UV-vis and Raman spectra, as well as several molecular properties, reveal that there exist coupling interactions between the E14E14 double bond and the ferrocenyl groups in the d-π conjugated (E)-Tip(Fc)E14E14(Fc)Tip molecules.
(2) The theoretical findings demonstrate that the greater the atomic radius of the group 14 element E14 contained in such d-π conjugated systems, the longer the E14E14 double bond distance, the weaker its π bond strength, the smaller its WBI bond order, the smaller its BDE to produce two equivalent carbene analogues (Tip(Fc)E14:), and the larger the yields of the formations of either [1 + 4] or [1 + 2] cyclo adducts. That is to say, the heavier the atomic mass of the group 14 element involved in the d-π conjugated compounds studied in this work, the smaller its π bond strength and more facile its [1 + 4] or [1 + 2] cycloadditions with either a butadiene or a selenium atom, respectively. In short, the order of the chemical reactivity increases as follows: 1-C ≪ 1-Si < 1-Ge < 1-Sn < 1-Pb.
(3) The theoretical evidence reveals that the steric congestions between (E)-Tip(Fc)E14E14(Fc)Tip and 2,3-dimethyl-1,3-butadiene would make these reactants undergo the [1 + 4] addition reactions rather than the [2 + 4] cycloaddition reactions.
(4) On the basis of the VBSCD model,13,17 one can use the singlet–triplet energy gap (ΔEst) of the (E)-Tip(Fc)E14E14(Fc)Tip compound as a diagnostic tool to anticipate its chemical reactivity.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c7ra04935h |
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