Raghu Nath
Behera
* and
Arunashree
Panda
*
Department of Chemistry, Birla Institute of Technology & Science, Pilani-K. K. Birla Goa Campus, Zuarinagar, 403726, Goa, India. E-mail: rbehera@bits-goa.ac.in; panda_arunashree@yahoo.com
First published on 25th May 2012
The intramolecular Se⋯N interactions between the selenium and the nitrogen atom in three series of o-substituted organoselenium compounds has been studied using density functional theory (DFT). The nature and the strength of these interactions and their dependence on substituents, the chelate ring size as well as the rigidity are predicted using a B3LYP/6-31G(d)/LanL2DZ method. The strength of the Se⋯N interactions is found to be dependent on the nature of Se–X (X = Cl, Br, I, SPh, CH2Ph; Ph: Phenyl) acceptor orbitals and follow the order I > Br > Cl > SPh > CH2Ph. The natural bond orbital (NBO) analysis using DFT methods points to nN→σ*Se–X electron delocalization as the key contributing factor towards Se⋯N nonbonding interactions. Both NBO and atoms in molecules (AIM) methods suggest that the intramolecular interaction in the organoselenium compounds is dominantly covalent in nature. Studies on the effect of solvent on the Se⋯N interaction show that a polar solvent stabilizes the Se⋯N interactions by shortening the Se⋯N distances.
The main evidence for such intramolecular nonbonding E⋯Y interactions is the distance between the two heteroatoms determined by X-ray crystallography1 and 77Se/125Te NMR.9 Computational methods based on electronic structure calculations have also been proved to be very useful in understanding the nature and magnitude of such intramolecular interactions.10 The detailed studies on such systems suggest that the interaction between a heteroatom Y (Y = N, O, S, halogens etc.) lone pair orbital and a σ*E–X orbital (E = Se/Te) leads to a weak unsymmetrical hypervalent bond. The collinear geometry between the donor atom (Y) and the E–X σ* acceptor orbital helps in maximizing the orbital interaction between the donor lone pair and the E–X anti bonding orbital and the geometry around the divalent selenium/tellurium is distorted T-shaped. The Y⋯E–X angle ranges from 165 to 180° depending on the strength of the Y⋯E interaction. The stronger the interaction, the more linear the Y⋯E–X angle. The bonding scheme of this interaction is described as three-centre four-electron [3c–4e] bonding. A pair of electrons occupies the nonbonding orbital and another pair of electrons occupies the bonding orbital of the molecular orbital. As a result, the E–X bonds get elongated and Y⋯E length shortens. Thus, one of the reasons of the origin of the Y⋯E interaction is due to the hypervalent nature of E. Although the hypervalency in divalent chalcogens increases in the order O < S < Se < Te, the basic factors responsible for the origin and the strength of such interactions are not completely understood.
In view of this, we will present results for intramolecular Se⋯N nonbonding interactions in a series of ortho substituted arylchalcogenides as studied using DFT, NBO and the quantum theory of AIM analysis. The effect of factors like substituent, chelate ring and rigidity on these interactions will also be discussed.
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Fig. 1 The organoselenium compounds 1a–e, 2a–e and 3a–e investigated in this study. |
Compounds | r Se–C (Å) | r Se⋯N (Å) | r Se–X (Å) | θ N⋯Se–X (°) | θ C–Se–X (°) | Remark |
---|---|---|---|---|---|---|
1c | 1.965 | 2.204 | 2.907 | 178.2 | 99.1 | This work |
(1.896) | (1.971) | (2.983) | (179.7) | (97.2) | (Ref. 20) | |
0.069 | 0.033 | −0.076 | −1.5 | 1.9 | Difference | |
1d | 1.946 | 2.476 | 2.277 | 177.2 | 100.7 | This work |
(1.937) | (2.458) | (2.25) | (176.4) | (100.4) | (Ref. 20) | |
0.009 | 0.018 | 0.027 | 0.8 | 0.3 | Difference | |
1e | 1.924 | 2.653 | 2.014 | 176.4 | 99.7 | This work |
(1.909) | (2.686) | (1.975) | (174) | (100.2) | (Ref. 20) | |
0.015 | −0.033 | 0.039 | 2.4 | −0.5 | Difference | |
2c | 1.977 | 2.259 | 2.881 | 178.3 | 99.4 | This work |
(1.945) | (2.133) | (2.777) | (177.7) | (97.4) | (Ref. 21) | |
0.032 | 0.126 | 0.104 | 0.6 | 3.0 | Difference | |
2e | 1.923 | 2.756 | 2.005 | 175.3 | 99.9 | This work |
(1.916) | (2.798) | (1.966) | (175.4) | (100.2) | (Ref. 21) | |
0.007 | −0.042 | −0.039 | −0.1 | 0.3 | Difference | |
3c | 1.983 | 2.2 | 2.908 | 178.2 | 99.5 | This work |
(—) | (2.059) | (2.83) | (175.3) | (97.5) | (Ref. 19) | |
— | 0.141 | 0.078 | 2.9 | 2.0 | Difference | |
3e | 1.926 | 3.26 | 1.987 | 151.9 | 99.8 | This work |
(1.916) | (3.384) | (1.979) | (—) | (98) | (Ref. 19) | |
0.01 | 0.124 | 0.008 | — | 1.8 | Difference |
Compounds | r Se–X (Å) | r Se⋯N (Å) | θ N⋯Se–X (°) | ω X–Se–C–C(C) (°) | ω N–C–C–C(Se) (°) |
---|---|---|---|---|---|
1a | 2.362 | 2.204 | 176.4 | 178.7 | 1 |
1b | 2.487 | 2.229 | 177.3 | 178.7 | 1.1 |
1c | 2.907 | 2.204 | 178.2 | 179 | 0.5 |
1d | 2.277 | 2.476 | 177.2 | 178.4 | 3.5 |
1e | 2.014 | 2.653 | 174 | 174.5 | 5.5 |
2a | 2.339 | 2.259 | 176.2 | −179.4 | −0.8 |
2b | 2.462 | 2.294 | 177.2 | −179.4 | −0.8 |
2c | 2.881 | 2.259 | 178.3 | −180 | 0 |
2d | 2.25 | 2.608 | 177.5 | −179.8 | 1.9 |
2e | 2.005 | 2.756 | 175.3 | −178.3 | −1.3 |
3a | 2.358 | 2.211 | 175.9 | 178.5 | 2.1 |
3b | 2.481 | 2.236 | 176.9 | 178.6 | 2.6 |
3c | 2.908 | 2.2 | 178.2 | 179.9 | −0.1 |
3d | 2.254 | 2.585 | 174.7 | 165.3 | 26.2 |
3e | 1.987 | 3.26 | 151.9 | 133.6 | 70.1 |
It has been suggested that the Se⋯Y (Y = O, N, F) interactions consist of an electrostatic and a covalent contribution.10d,f Thus, to estimate (approximately) the extent of electrostatic contributions to Se⋯N interactions, we calculated the electrostatic interaction energy between Se and N atoms from their charges obtained by natural population analysis (NPA). In this calculation, we assumed a point charge model so that the charge is located at the respective nuclei.10d The calculated electrostatic contribution to the Se⋯N interaction (Eel) and the NPA charges on Se and N atoms (qSe and qN, respectively) are given in Table 3.The values of Eel follow the order SPh < CH2Ph < Br < I < Cl for series 1 and 2 and CH2Ph < SPh < Br < I < Cl for 3. For a given X, the order is 2 < 3 < 1 (for X = Cl, Br, I) and for X = SPh, CH2Ph the trend is 3 < 2 < 1. This trend is nearly according to the electronegativity of X attached to the Se atom. The NPA charge on the Se atom also increases with the Eel. We observe quite good correlation (R = 0.904) of Eel with qSe (Fig. 2). However, qN does not correlate so well with Eel. These observations are very similar to those of other intramolecular chalcogen interactions.10d,e
Compounds | q N (e) | q Se (e) | E el (kcal mol−1) | E Se…N (kcal mol−1) | E del (kcal mol−1) | △q(σ*) (e) | △q(N) (e) | Covalency factor (χ) |
---|---|---|---|---|---|---|---|---|
1a | −0.557 | 0.555 | 46.58 | 63.63 | 77.26 | −0.199 | 0.203 | 0.814 |
1b | −0.552 | 0.486 | 39.97 | 59.08 | 73.73 | −0.189 | 0.194 | 0.798 |
1c | −0.596 | 0.457 | 41.04 | 72.95 | 97.57 | −0.177 | 0.224 | 0.814 |
1d | −0.545 | 0.358 | 26.17 | 22.85 | 27.92 | −0.105 | 0.1 | 0.637 |
1e | −0.536 | 0.449 | 30.13 | 11.58 | 13.32 | −0.051 | 0.05 | 0.521 |
2a | −0.555 | 0.544 | 44.39 | 50.96 | 64.62 | −0.185 | 0.189 | 0.778 |
2b | −0.552 | 0.472 | 37.72 | 45.28 | 59.22 | −0.173 | 0.177 | 0.756 |
2c | −0.603 | 0.437 | 38.74 | 58.97 | 82.74 | −0.18 | 0.214 | 0.778 |
2d | −0.541 | 0.352 | 24.25 | 13.44 | 17.05 | −0.074 | 0.072 | 0.55 |
2e | −0.53 | 0.452 | 28.87 | 7.5 | 9.12 | −0.036 | 0.037 | 0.454 |
3a | −0.555 | 0.534 | 44.52 | 59.41 | 74.28 | −0.194 | 0.202 | 0.81 |
3b | −0.551 | 0.465 | 38.05 | 54.83 | 70.67 | −0.183 | 0.192 | 0.793 |
3c | −0.608 | 0.444 | 40.75 | 71.42 | 98.04 | −0.177 | 0.227 | 0.817 |
3d | −0.539 | 0.327 | 22.64 | 11.89 | 14.75 | −0.064 | 0.064 | 0.565 |
3e | −0.511 | 0.358 | 18.64 | — | — | — | — | 0.124 |
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Fig. 2 Plot of the magnitude of the ionic contribution, Eel (calculated by considering point charges for Se and N atoms), with the charge on the selenium atom, (qSe). |
To estimate the covalent contribution to the Se⋯N interactions, we used NBO second order perturbation and NBO deletion analysis. The NBO method, based on local block eigenvectors of a one-particle density matrix, predicts bonds and lone pairs of an optimized Lewis structure of a molecule from ab initio wavefunctions.12 Delocalization of electron density between occupied (bond or lone pair) NBOs and formally unoccupied (antibonding or Rydberg) NBOs corresponds to a stabilizing interaction. In the NBO deletion technique, a selected set of NBOs from a donor–acceptor pair is deleted and the energy change (loss of delocalization energy) associated with this process provides information on the interaction between the respective orbitals.
We studied the orbital interactions between the lone pairs of the nitrogen atom (nN) and the antibonding orbital of the Se–X bond (σ*Se⋯X). Our NBO study indicated the absence of nN→σ*Se⋯X orbital interaction for the compound 3e. The NBO second order perturbation energies for nN→σ*Se⋯X orbital interactions (ESe⋯N) are presented in Table 3. The values of ESe⋯N range from 11.58 to 72.95 kcal mol−1 for 1a–e, 7.5 to 58.97 kcal mol−1 for 2a–e and 11.89 to 71.42 kcal mol−1 for 3a–d. Also, these interaction energies increase in the order CH2Ph < SPh < Br < Cl < I for all series and for a given X, the order is 2 < 3 < 1 (except for X = SPh where it is 3 < 2 < 1). This trend is more or less according to the electrophilicity of the Se–X bond and the nucleophilicity of the N atom for the Se⋯N interactions. The NBO deletion energies (Edel), which provide information on the orbital interaction energies associated with the Se atom and the chelating N atom, follow the same trend as those of the ESe⋯N. These factors clearly suggest that the nN→σ*Se⋯X orbital interactions contribute significantly to the stability of Se⋯N interactions in these compounds.
It is known that a strong Se⋯N interatomic distance causes shortening of the Se⋯N interatomic distance and an increase in the linearity of the N⋯Se–X alignment.18 This indeed is observed from the present calculations. However, the X-ray study of selenenyl halides shows that the bond angles N⋯Se–X (X = Cl, Br or I) deviate from 180° as the Se⋯N interaction increases (e.g.1b: Se⋯N = 2.052 Å and N⋯Se–Br = 175.15°; 1c: Se⋯N = 2.059 Å, N⋯Se–I = 175.26°).19–21 This is probably due to the presence of intermolecular interactions between Se and X (X = Cl, Br or I). The intermolecular interaction increases when the electronegativity of the halogen atom decreases and hence is greatest for X = I. The weakest Se⋯N interaction is observed in all the aryl benzyl selenides compared to the selenenyl halides and selenenyl sulphides, maybe due to the presence of the benzyl group, which cannot accept electron density from the selenium. This is in agreement with the experimental observations (Se⋯N; 1e: 3.3842 Å; 3e: 2.798 Å).19,21
The value of ESe⋯N depends on at least two factors: (a) the distance between the Se and N atom (rSe⋯N) and (b) the donor ability of the N atom. To find out the contribution of each of these factors, we reoptimized the geometries of the compounds at the fixed Se⋯N distances and then calculated the ESe⋯N of all the compounds (see Table 4). It is clear from Table 4 that the values of ESe⋯N are highly dependent on rSe⋯N and almost comparable ESe⋯N values were obtained for a fixed Se⋯N distance for series 1, 2 and 3 (for a given X). The relatively higher ESe⋯N values of compound 1, compared to those of 3 and 2, may be due to the difference in the size of chelate rings containing a donor nitrogen atom.
X | r Se⋯N (Å) | E Se⋯N (kcal mol−1) | ||
---|---|---|---|---|
1 | 2 | 3 | ||
Cl | 2.211 | 62.4 | 59.04 | 59.41 |
Br | 2.236 | 57.93 | 54.43 | 54.83 |
I | 2.2 | 73.7 | 70.35 | 71.42 |
SPh | 2.585 | 16.43 | 14.48 | 11.89 |
CH2Ph | 3.26 | 0.81 | 0.85 | — |
The values for ESe⋯N (and Edel) decrease with an increase in Se⋯N distance (rSe⋯N) for all the compounds. The single correlation curve between ESe⋯Nversus rSe⋯N (Fig. 3) and Edelversus rSe⋯N (Fig. 4) clearly show that the nature of the interactions in all the studied compounds are the same. The changes in orbital occupancies of the lone pair of nitrogen (nN) and σ*Se⋯X orbitals (△q = qdel−q) during NBO deletion analysis are displayed in Table 3. The significant decrease of charge of the σ*Se⋯X orbitals and a similar increase of charge for the nN orbitals upon NBO deletion suggest that the nature of orbital interaction is electron delocalization from the lone pair of the N atom to the anti-bonding orbital of Se–X (i.e. nN→σ*Se⋯X). This dominant contribution of nN→σ*Se⋯X charge transfer in the intramolecular Se⋯N bonding is supported by relatively high values (up to 81%) of covalency factor χ for the intramolecular coordination Se⋯N bond (Table 3). The values of χ follow the same trend as ESe⋯N and Edel (CH2Ph < SPh < Br < Cl < I for all series and for a given X, the order is 2 < 3 < 1) and show a single correlation curve (Fig. 5) for all the compounds.
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Fig. 3 Variation of NBO second order perturbation energies (ESe⋯N) with the Se⋯N distances (rSe⋯N). |
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Fig. 4 Variation of NBO deletion energies (Edel) with the Se⋯N distances (rSe⋯N). |
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Fig. 5 Plot of covalency factor (χ) with the NBO second order perturbation energies (ESe⋯N). |
The strength of the Se⋯N interactions has been observed in the order CH2Ph < SPh < Br < Cl ≈ I. The ionic contribution (Eel) decreases in the order Cl > I > Br > SPh > CH2Ph and the covalent contribution (ESe⋯N) decreases in the order I > Cl > Br > SPh > CH2Ph (Table 3). However, the total strength (ionic + covalent) decreases in the order I ≈ Cl > Br > SPh > CH2Ph. The observed trend for halides may be due to the negligence of intermolecular interaction during our theoretical calculations. These interactions, which are often present in the organoselenenyl halides in the solid state, have a significant affect on the Se⋯N interactions. However, the Se⋯N bond distances of organoselenenyl halides 1a [1.9695 Å(av.)],201b (1.975 Å)20 and 1c (1.971 Å)20 from the X-ray studies follow the trend Br > Cl ∼ I. These halides either have very weak or no intermolecular interactions. Also for organoselenenyl halides 3b (2.052 Å)19 and 3c (2.059 Å)19 (absence of intermolecular interactions due to the presence of a sterically more demanding group), Se⋯N bond distances are very close. Furthermore, for organoselenenyl halides of 2 (where the intermolecular interaction is greatest among the three series studied here), the trend of Se⋯N distances is Cl (2a, 2.052 Å) < Br (2b, 2.063 Å) < I (2c, 2.133 Å).
In summary, introduction of rigidity (for 3) onto the backbone of 2, or replacing the five membered oxazoline ring in 2 by a six membered oxazine ring in 1, enhances the strength of Se⋯N nonbonding interactions; the latter effect seems to be more dominant. This is in accordance with the experimental findings. For example, the Se–N distances in 1a, 1b and 1c are 1.9695 (average), 1.975 (average) and 1.971 Å, respectively, whereas for 2a, 2b and 2c they are 2.052(2), 2.063(3) and 2.133 Å, respectively. Similar trends have also been observed for similar organotellurium compounds.22
The presence of BCP between Se and N atoms and the ring critical point (RCP) for the five membered ring formed with the phenyl ring due to Se⋯N interaction was observed for all the studied compounds, except 3e. The electron density at RCP (ρrcp), along with the other AIM parameters (ρSe⋯N, ∇2ρSe⋯N and HSe⋯N) for the Se⋯N interaction, are given in Table 5. The values of ρSe⋯N for the studied compounds range from 0.0237 to 0.0736 e Å−3, which are in between a typical covalent bond (e.g. ρC–C ≈ 0.24 e Å−3) and that of hydrogen bond (ρH–Bond ≈ 0.002–0.04 e Å−3). Similar values were reported for Se⋯N interactions by Sharma et al.10d The values of ρSe⋯N follow the trend CH2Ph < SPh < Br < Cl < I for all series, and 2 < 3 < 1 for a given X. This trend is similar to that for ESe⋯N and Edel. This is not surprising because a covalent interaction in AIM theory is related to orbital interactions in NBO analysis. The values of ESe⋯N and Edel correlate nicely with ρSe⋯N (Fig. 6 and 7, respectively), indicating a dominant covalent contribution in the Se⋯N interactions. The values of ρrcp lie in the range 0.014 to 0.0248 e Å−3 and increase in the order CH2Ph < SPh < I < Br < Cl for all three series, and for a given X: 2 < 3 < 1. The values of ∇2ρSe⋯N obtained (Table 5) are all positive (range: 0.07 to 0.138 e Å−5) and follow the overall trend CH2Ph < SPh < I < Br < Cl for series 2, 3 and CH2Ph < SPh < Br < Cl ≈ I for series 1; and for a given X: 1 < 2 < 3. All positive values indicate a dominant electrostatic character, which is in contrast to “dominant covalent contribution” as predicted by NBO analysis. Thus, we analyze the total energy density at the critical point (HSe⋯N), which is known to be more reliable in identifying the type of interactions (electrostatic or covalent).23,10d The calculated values of HSe⋯N (Table 5) are mostly negative (except 1d, 1e, 2d and 2e) indicating dominant covalent interaction, as predicted by NBO analysis. The values of HSe⋯N become more negative for stronger Se⋯N interactions (shorter rSe⋯N) and are positive with weaker Se⋯N interactions. This correlation is quite evident from Fig. 8.
Compounds | ρ Se⋯N (e Å−3) | ρ rcp (e Å−3) | ∇2ρSe⋯N (e Å−5) | H Se⋯N (e Å−4) |
---|---|---|---|---|
1a | 0.0736 | 0.0248 | 0.123 | −0.0076 |
1b | 0.0706 | 0.0242 | 0.115 | −0.0059 |
1c | 0.0752 | 0.0237 | 0.124 | −0.0121 |
1d | 0.043 | 0.0193 | 0.076 | 0.0006 |
1e | 0.0302 | 0.0163 | 0.07 | 0.0012 |
2a | 0.0641 | 0.023 | 0.133 | −0.0112 |
2b | 0.0602 | 0.022 | 0.127 | −0.0092 |
2c | 0.0659 | 0.0223 | 0.127 | −0.0179 |
2d | 0.0319 | 0.016 | 0.087 | 0.0002 |
2e | 0.0237 | 0.0139 | 0.085 | 0.0004 |
3a | 0.0706 | 0.0242 | 0.141 | −0.015 |
3b | 0.0677 | 0.0236 | 0.137 | −0.0132 |
3c | 0.0738 | 0.0234 | 0.132 | −0.0171 |
3d | 0.0338 | 0.0178 | 0.089 | −0.0001 |
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Fig. 6 Correlation plot of the NBO second order perturbation energies (ESe⋯N) with the electron density (ρSe⋯N) at the bond critical point of the Se⋯N interaction. ρSe⋯N is in units of e Å−3. |
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Fig. 7 Correlation plot of the NBO deletion energies (Edel) with the electron density (ρSe⋯N) at the bond critical point of the Se⋯N interaction. ρSe⋯N is in units of e Å−3. |
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Fig. 8 Variation of AIM total energy density (HSe⋯N) at the bond critical point with the Se⋯N distances (rSe⋯N). HSe⋯N are given in units of e Å−4. |
The AIM dual-parameter analysis (plot of HSe⋯Nversus ∇2ρSe⋯N) for weak to strong interaction is shown in Fig. 9. Most of the points fall in the fourth quadrant (HSe⋯N < 0, ∇2ρSe⋯N > 0; more shared-shell character) indicating strong Se⋯N interaction. A few points lie on first quadrant (HSe⋯N > 0, ∇2ρSe⋯N > 0), indicating that the electron density at BCP is neither stabilized nor concentrated, i.e. weak Se⋯N interactions.
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Fig. 9 Variation of AIM total energy density (HSe⋯N in units of e Å−4) with the Laplacian of the electron density (in units of e Å−5) at the bond critical point. |
Detailed inspection of the AIM analysis reveals some interesting facts. Several intramolecular interactions have been observed for all the systems discussed in the present study (Fig. 1) from the AIM analysis through BCP and RCP.24 These interactions have not been reported for the solid state structures of these compounds19–21 and are discussed below.
(A) The common features that have been observed for all cases i.e. for 1–3 (except 3e) are; (1) the presence of Se⋯N interactions and (2) the presence of interaction between the substituents X and the aryl hydrogen ortho to the Se–X group. Similar observations have been made by Sunoj et al. earlier.10e A representative diagram of 1a showing both Se⋯N and Se⋯H interactions is given in Fig. 10.24
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Fig. 10 Molecular plot of 1a (X = Cl) showing Se⋯N and Se⋯H bond critical points (small red spheres) and the corresponding ring critical points (yellow spheres) arising due to intramolecular interactions. |
(B) Besides these above interactions, the existence of an additional interaction between the Se atom and the aryl hydrogen ortho to the S atom from the SPh group could be identified through Se⋯H BCPs and the corresponding RCPs for compounds 1d, 2d and 3d. One of the representative cases is shown in Fig. 11.
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Fig. 11 Molecular plot of 2d (X = SPh) showing the Se⋯N, S⋯H and Se⋯H bond critical points (small red spheres) and the corresponding ring critical points (yellow spheres) arising due to intramolecular interactions. |
(C) Furthermore, another interaction in addition to (A) between oxygen and aryl hydrogen ortho to the oxazoline ring is predicted for the compound 1e.24
(D) Interestingly, along with the interactions described in (A), interactions between the oxygen and carbon atom (of the phenyl ring attached to the naphthyl ring) have been observed for the sterically hindered compounds 3a–d.24
(E) More interestingly, although compound 3e (Fig. 12) does not have a Se⋯N interaction, existence of several other intramolecular interactions have been predicted by our AIM studies. (1) The interaction between the hydrogen atom of the methyl group of the oxazoline ring and the hydrogen atom of the methyl group of the phenyl ring perpendicular to the naphthyl ring results in the formation of a 12 membered chelate ring. (2) The hydrogen atom of the other methyl group of the oxazoline ring interacts with the selenium atom forming a eight membered chelate ring. (3) A 6-membered chelate ring arises from the interaction of the aryl hydrogen ortho to the –CH2– group and the oxygen atom of the oxazoline ring. (4) Additionally, another 5-membered chelate ring results from the interaction of the same aryl hydrogen ortho to the –CH2– group and the selenium atom.
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Fig. 12 Molecular plot of 3e (X = CH2Ph) showing the H⋯H, O⋯H, Se⋯H bond critical point (small red spheres) and the corresponding ring critical points (yellow spheres) arising due to intramolecular interactions. |
To sum up, the AIM analysis reveals that the electron density at the Se⋯N BCP shows a very good correlation with the computed intramolecular interaction energies (from NBO analysis) and hence suggests a dominant covalent nature of the intamolecular interactions. Also, several types of intramolecular interactions other than Se…N are predicted.
Compounds | r Se⋯N (Å) | r Se⋯N (CHCl3) (Å) | E Se⋯N (kcal mol−1) | E Se⋯N (CHCl3) (kcal mol−1) |
---|---|---|---|---|
1a | 2.204 | 2.092 | 63.63 | 93.36 |
1b | 2.229 | 2.13 | 59.08 | 82.02 |
1c | 2.204 | 2.088 | 72.95 | 105.48 |
1d | 2.476 | 2.409 | 22.85 | 28.31 |
1e | 2.653 | 2.665 | 11.58 | 11.16 |
2a | 2.259 | 2.123 | 50.96 | 81.62 |
2b | 2.294 | 2.171 | 45.28 | 68.85 |
2c | 2.259 | 2.103 | 58.97 | 97.63 |
2d | 2.608 | 2.574 | 13.44 | 15.06 |
2e | 2.756 | 2.776 | 7.5 | 7.05 |
3a | 2.211 | 2.092 | 59.41 | 90.52 |
3b | 2.236 | 2.132 | 54.83 | 78.25 |
3c | 2.2 | 2.074 | 71.42 | 108.15 |
3d | 2.585 | 2.536 | 11.89 | 14.32 |
3e | 3.26 | 3.151 | — | 0.68 |
Footnote |
† Electronic supplementary information (ESI) available: B3LYP/6-31G(d)/LanL2DZ optimized geometries and AIM molecular plots of all the studied compounds. See DOI: 10.1039/c2ra20591b |
This journal is © The Royal Society of Chemistry 2012 |