How does non-covalent Se⋯Se[double bond, length as m-dash]O interaction stabilize selenoxides at naphthalene 1,8-positions: structural and theoretical investigations

Satoko Hayashia, Waro Nakanishi*a, Atsushi Furutaa, Jozef Drabowiczb, Takahiro Sasamoric and Norihiro Tokitohc
aDepartment of Material Science and Chemistry, Faculty of Systems Engineering, Wakayama University, 930 Sakaedani, Wakayama 640-8510, Japan. E-mail: nakanisi@sys.wakayama-u.ac.jp; Fax: +81 73 457 8253; Tel: +81 73 457 8253
bCenter of Molecular and Macromolecular Studies, Polish Academy of Science, Sienkiewicza, 112, 90-363, Lodz, Poland
cInstitute for Chemical Research, Kyoto University, Gokasho, Uji, Kyoto 611-0011, Japan

Received (in Montpellier, France) 9th June 2008, Accepted 25th September 2008

First published on 17th November 2008


Abstract

Bis-selenides[thin space (1/6-em)](LL), such as 8-[MeSe(X)]-1-[MeSe(Z)]C10H6 (1[thin space (1/6-em)](LL)), 8-[EtSe(X)]-1-[EtSe(Z)]C10H6 (2[thin space (1/6-em)](LL)), 8-[p-YC6H4Se(X)]-1-[MeSe(Z)]C10H6 (3[thin space (1/6-em)](LL)) and 8-[p-YC6H4Se(X)]-1-[p-YC6H4Se(Z)]C10H6 (4[thin space (1/6-em)](LL)) were oxidized with ozone at 0 °C, where (X, Z) = (lone pair, lone pair) for LL. Bis-selenoxides, 1[thin space (1/6-em)](OO), 3[thin space (1/6-em)](OO) and 4[thin space (1/6-em)](OO) where (X, Z) = (oxygen, oxygen), were obtained in the oxidation of 1[thin space (1/6-em)](LL), 3[thin space (1/6-em)](LL) and 4[thin space (1/6-em)](LL), respectively, via corresponding selenide-selenoxides, 1[thin space (1/6-em)](LO), 3[thin space (1/6-em)](LO) and 4[thin space (1/6-em)](LO), respectively. A facile Se–C bond cleavage was observed in 2[thin space (1/6-em)](LL). The structures of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) were determined by the X-ray analysis. Three Se⋯Se[double bond, length as m-dash]O atoms in 1[thin space (1/6-em)](LO) and four O[double bond, length as m-dash]Se⋯Se[double bond, length as m-dash]O atoms in 1[thin space (1/6-em)](OO) align linearly. While the non-covalent Se⋯Se[double bond, length as m-dash]O 3c–4e interaction operates to stabilize 1[thin space (1/6-em)](LO), the non-covalent O[double bond, length as m-dash]Se⋯Se[double bond, length as m-dash]O 4c–4e interaction would not stabilize 1[thin space (1/6-em)](OO). The 3c–4e interaction must play an important role to control the stereochemistry of selenoxides. The 8-G-1-[MeSe(OH)2]C10H6 (n[thin space (1/6-em)](OH·OH)) are the key intermediates in the racemization of 8-G-1-[MeSe(O)]C10H6 (n[thin space (1/6-em)](O)) in solutions, where G = SeMe (1), H (5), F (6), Cl (7) and Br (8). Energies of n[thin space (1/6-em)](OH·OH), relative to n[thin space (1/6-em)](O), are evaluated based on the theoretical calculations. G of SeMe is demonstrated to operate most effectively to protect from racemization of selenoxides among n = 1 and 5–8, since the relative energies for G of cis- and trans-SeMe are largest.


Introduction

Selonoxides1–4 [RSe(O)R′] afford optically active enantiomers, as well as sulfoxides,5,6 if R and R′ are not the same, since Se in each selenoxide is three-coordinated containing a lone pair. However, it is usually difficult to utilize optical active selenoxides to introduce the optical activity in a target molecule,1,2,4,7 since the racemization of optical active selenoxides is usually very fast. Nevertheless, some efforts have been made to stabilize the stereochemistry of selenoxides, by taking advantage of non-covalent coordination by the neighboring groups (G) of the G⋯Se[double bond, length as m-dash]O type.2,4,7

Naphthalene 1,8-positions supply a good system to investigate such interactions, since the non-bonded distances between heteroatoms at the positions are close to the sum of the van der Waals radii minus 1 Å.8,9 Various types of non-covalent interactions are detected in naphthalene 1,8-positions.8–11 The σ-type three center-four electron interactions (σ(3c–4e)),12–14σ(2c–4e),12π(2c–4e),12 distorted π(2c–4e),12 and Z4 4c–6e13 are typical examples. Such non-covalent interactions are demonstrated to control the fine structures of molecules.15 Recently, we investigated fine structures of 8-G-1-(arylseleninyl)naphthalene with G = H, F, Cl and Br, together with the factors to control the structures, as the first step to control the stereochemistry of selenoxides.16 The factors are called G, O and Y dependences, which originate from the np(G)⋯σ*(Se–O), np(O)⋯π(Nap) and np(O)⋯π(Ar) interactions, respectively.16

We paid much attention to G = MeSe and ArSe in 8-G-1-(arylseleninyl)naphthalenes, since many conformers are plausible around the two Se–CNap bonds, relative to the case of G = H and halogens. Scheme 1 shows the orbitals taking part in the non-covalent Se⋯Se[double bond, length as m-dash]O interaction. A bis-selenide contains double ns(Se), np(Se), σ(Se–C) and σ*(Se–C) orbitals. However, ns(O), np(O), np′(O), σ(Se–O) and σ*(Se–O) appear newly with the quit of an np(Se), when a selenide-selenoxide is formed from the bis-selenide.

The oxidation and formation of 8-[2RSe(X)]-1-[1RSe(Z)]C10H6 (1 (1R = 2R = Me), 2 (1R = 2R = Et), 3 (1R = Me, 2R = p-YC6H4: Y = H (a), MeO (b) and NO2 (d)) and 4 (1R = 2R = p-YC6H4: Y = H (a) and tBu (c)) are investigated for LL where (X, Z) = (lone pair, lone pair), LO (lone pair, oxygen) and OO (oxygen, oxygen) (Chart 1). The reactions are easily controlled and each process is followed by the spectroscopic method. Non-bonded O[double bond, length as m-dash]Se⋯Se[double bond, length as m-dash]O interactions are also the subject of interest.

The structures around the naphthyl group (Nap) in 8-G-1-RSeC10H6 are well explained by three types, type A (A), B and C.8c,d,f–h,17,18 The combined notation are used to specify the structures of 1–4 with G = RSe, where the notation, such as AA, BA or CA, shows the conformers around the two CNap–Se bonds. Scheme 2 draws the notations employed in this work, exemplified by 1[thin space (1/6-em)](LO).

The structures of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) are determined by X-ray crystallographic analysis. Quantum chemical (QC) calculations are performed on 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO), to elucidate the role of the Se⋯Se[double bond, length as m-dash]O interaction in 1[thin space (1/6-em)](LO) and the O[double bond, length as m-dash]Se⋯Se[double bond, length as m-dash]O interaction in 1[thin space (1/6-em)](OO) as the factor to control the fine structures. Orbitals of two Se atoms in 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) must overlap directly with each other, which would stabilize the fine structures. QC calculations are also performed on 8-G-1-[MeSe(X)]C10H6 [G = MeSe (1), H (5), F (6), Cl (7) and Br (8) with X = lone pair (L), O (O), OH+ (OH+) and O2H2 (OH·OH)], where OH·OH must be the key intermediate in the racemization of 1 and 5–8, in the presence of a trace of water. The relative energy [ΔE = E(n[thin space (1/6-em)](OH·OH)) − (E(n[thin space (1/6-em)](O)) + E(H2O)) (n = 1 and 5–8)] is evaluated: that for G = MeSe is largest among them. The larger value must correspond to a selenoxide with the stronger resistance for racemization, although n[thin space (1/6-em)](OH·OH) is not the transition state. The G⋯Se[double bond, length as m-dash]O interactions containing the Se⋯Se[double bond, length as m-dash]O and O[double bond, length as m-dash]Se⋯Se[double bond, length as m-dash]O interactions are also analyzed with the natural orbital (NBO)19,20 and atoms-in-molecules (AIM)21,22 analyses.

Oxidation of 1,8-bis(selanyl)naphthalenes[thin space (1/6-em)](LL) with ozone is well controlled and monitored, which gives 1,8-bis(seleninyl)naphthalenes (OO) via 8-selanyl-1-seleninylnaphthalenes (LO). Factors to control the fine structures of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) are clarified based on QC calculations, after determination of the structures. The Se⋯Se[double bond, length as m-dash]O interaction is demonstrated to control the fine structure of 1[thin space (1/6-em)](LO), whereas the role of the O[double bond, length as m-dash]Se⋯Se[double bond, length as m-dash]O interaction in 1[thin space (1/6-em)](OO) is critically discussed. The role of G in 1 and 5–8 in the racemization process is also evaluated.


Orbitals taking part in the non-bonded Se⋯SeO interactions in naphthalene 1,8-positions.
Scheme 1 Orbitals taking part in the non-bonded Se⋯Se[double bond, length as m-dash]O interactions in naphthalene 1,8-positions.

Structures around naphthyl group in 8-G-1-[RSe(X)]C10H6, exemplified by 1 (LO).
Scheme 2 Structures around naphthyl group in 8-G-1-[RSe(X)]C10H6, exemplified by 1[thin space (1/6-em)](LO).

Bis(selanyl)naphthalenes, 1–4, together with 5–8.
Chart 1 Bis(selanyl)naphthalenes, 1–4, together with 5–8.

Results and discussion

Survey of oxidation

Bis-selenides (n[thin space (1/6-em)](LL): n = 1–4) were oxidized with ozone in the methylene dichloride solution of each bis-selenide at 0 °C. The bis-selenides (n[thin space (1/6-em)](LL)) gave corresponding bis-selenoxides (n[thin space (1/6-em)](O)) via corresponding selenide-selenoxides (n[thin space (1/6-em)](LO)), except for 2[thin space (1/6-em)](LL). While 1[thin space (1/6-em)](LL) gave 1[thin space (1/6-em)](LO), followed by the quantitative formation of 1[thin space (1/6-em)](OO), a facile Se–C bond cleavage occurred on the oxidation of 2[thin space (1/6-em)](LL), resulting in the formation of naphtho-1,8-[c,d]-1,2-diselenole (9).23β-Elimination of the selenoxide may be responsible for the facile Se–C bond cleavage. In the case of 3[thin space (1/6-em)](LL), the methylselanyl Se atoms were attacked exclusively. 3[thin space (1/6-em)](LO) were consumed to produce the corresponding 3[thin space (1/6-em)](OO) with more ozone. 4[thin space (1/6-em)](LO) were also produced from the corresponding 4[thin space (1/6-em)](LL) with ozone, followed by the formation of the corresponding 4[thin space (1/6-em)](OO), respectively. The results are summarized in Chart 1. The reactions are well followed by NMR.

Structures of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO)

Single crystals of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) were obtained via slow evaporation of methylene dichloride-hexane solutions and one of suitable crystals was subjected to X-ray crystallographic analysis for each compound.24 Only one type of structure corresponds to each of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) in the crystals. Table 1 shows the crystallographic data of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO). Fig. 1 shows the structures of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO).25 The packing structure of 1[thin space (1/6-em)](OO) is shown in Fig. S1 of the Electronic Supplementary Information (ESI). Selected interatomic distances, angles and torsional angles of the compounds 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) are collected in Table 2, together with those of 1[thin space (1/6-em)](LL), which contains two types, 1[thin space (1/6-em)](LL)A and 1[thin space (1/6-em)](LL)B.26

The structures of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) are all AA for two methyl groups (Fig. 1 and Table 2).15 The planarity of the naphthyl (Nap) planes is very good. All Se–O bonds are placed in the naphthyl plane. The superior tendency of the Se–O bonds to stay on the naphthyl plane (O dependence)16 must be the driving force for the structures of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO). Three Se⋯Se–O atoms align linearly (∠SeSeO = 173.31(15)°) and the Se–O bond is almost perpendicular to another CNapSeCMe plane in 1[thin space (1/6-em)](LO). The non-covalent np(Se)⋯σ*(Se–O) 3c–4e interaction operates effectively to keep the Se–O bond on the naphthyl plane in 1[thin space (1/6-em)](LO) (G dependence).16 These results show that the structure of 1[thin space (1/6-em)](LO) is well stabilized by the O and G dependences observed in 1-naphthyl selenoxides.16

On the other hand, there is no np(Se) in 1[thin space (1/6-em)](OO). Therefore, the G dependence of the np(Se)⋯σ*(Se–O) type cannot operate in 1[thin space (1/6-em)](OO). Consequently, the driving force for the structure must come from the O dependence for both Se–O bonds. Namely, the non-covalent O–Se⋯Se–O σ(4c–4e) interaction must be carefully examined as a factor to stabilize the fine structure of 1[thin space (1/6-em)](OO), although the non-bonded Se⋯Se distances are less than the sum of van der Waals radii by ca. 0.65 Å.27 The σ(4c–4e) interaction seems not so important.

How does G of MeSe control the fine structure and the behavior? QC calculations are performed on 1 and 5–8.


Structures of 1 (LO) (a) and 1 (OO) (b) with atomic numbering scheme for selected atoms (thermal ellipsoids are shown at the 50% probability level).
Fig. 1 Structures of 1[thin space (1/6-em)](LO) (a) and 1[thin space (1/6-em)](OO) (b) with atomic numbering scheme for selected atoms (thermal ellipsoids are shown at the 50% probability level).
Table 1 Crystallographic data for 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO)
 1[thin space (1/6-em)](LO)1[thin space (1/6-em)](OO)
Empirical formulaC12H12OSe2C12H12O2Se2·2.5H2O
Formula weight330.14391.18
Temperature/K298(2)103(2)
Crystal systemMonoclinicMonoclinic
Space groupP21/n (#14)C2/c (#15)
a5.8460(19)25.549(9)
b14.473(3)5.8653(18)
c14.1490(16)20.850(8)
β97.660(17)117.329(4)
V31186.5(5)2775.6(16)
Z48
Dc/g cm−31.8481.872
F(000)6401544
Reflections observed [I > 2σ(I)]22002435
Parameters136190
R1 [I > 2σ(I)]0.0320.021
R1 [all data]0.0820.022
ωR2 [I > 2σ(I)]0.0650.053
ωR2 [all data]0.0770.054
Goodness-of-fit on F21.0291.109


Table 2 Selected interatomic distances (Å), angles (°) and torsional angles (°) around Se atom in 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO), together with those of 1[thin space (1/6-em)](LL)
 1[thin space (1/6-em)](LL)Aa1[thin space (1/6-em)](LL)Ba1[thin space (1/6-em)](LO)1[thin space (1/6-em)](OO)
a Ref. 26.
Interatomic distances
Se1–Se23.051(4)3.064(4)3.1587(10)3.1512(8)
Se1–C11.929(4)1.932(3)1.983(5)1.959(2)
Se1–C111.944(4)1.953(4)1.954(5)1.940(2)
Se1–O1  1.653(4)1.6771(15)
Se2–C91.926(4)1.932(4)1.928(5)1.970(2)
Se2–C121.944(4)1.949(4)1.938(6)1.934(2)
Se2–O2   1.680(15)
 
Angles
Se2–Se1–C11164.47(3)146.46(3)85.93(16)88.26(7)
Se2–Se1–O1  173.31(15)167.54(5)
Se1–Se2–C12150.34(3)159.73(3)85.65(18)89.41(7)
Se1–Se2–O2   167.51(5)
Se1–C1–C10122.9(3)123.9(3)126.9(4)124.33(16)
C1–Se1–C1199.29(16)98.41(16)96.0(2)94.73(9)
C1–Se1–O1  101.1(2)102.69(8)
C11–Se1–O1  100.7(2)102.85(9)
Se2–C9–C10123.9(3)122.9(3)124.1(4)124.67(16)
C9–Se2–C1299.27(16)98.50(16)98.1(2)93.38(9)
C9–Se2–O2   102.21(8)
C12–Se2–O2   102.29(9)
C1–C10–C9126.4(3)127.2(3)127.0(4)128.1(2)
 
Torsional angles
Se1–C1–C10–C5173.5(2)−176.0(2)−177.6(4)179.19(15)
C10–C1–Se1C11−154.1(3)136.8(3)82.8(4)−86.49(19)
C10–C1–Se1–O1  −175.0(4)169.19(17)
Se2–C9–C10–C5172.2(2)−170.2(2)178.8(4)178.90(15)
C10–C9–Se2–C12−138.8(3)148.0(3)84.6(4)−87.10(19)
C10–C9–Se2–O2   169.54(18)
O1–Se1–Se2–O2   140.3(3)


QC calculations

QC calculations were performed on 1[thin space (1/6-em)](LO) with the B3LYP/6-311+G(d) method of the Gaussian 98 program.28–30 QC calculations revealed energy profiles of the compounds.31Table 3 collects the results of the QC calculations. The NBO analysis19,20 were performed on 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) with the B3LYP/6-311+G(d) method. The results are shown in Table 4. The AIM parameters21,22 are calculated for 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) with the Gaussian 03 program32 employing the 6-311+G(3df) basis sets for Se with the 6-311+G(3d,2p) basis sets for C and H at the B3LYP level. They are analyzed employing the AIM 2000 program.33Table 5 collects the results of AIM calculations.

Indeed, the results of QC calculations essentially correspond to those in the gas phase, but the factors to control and/or stabilize the structures in gas phase must also operate in solid states and in solutions. Therefore, it must be instructive to consider those predicted by QC calculations, although we must be careful for the crystal packing effect in crystals and the solvent effect in solutions, since such effects often larger than the predicted factors.

The effect of G to stabilize 8-G-1-[MeSe(X)]C10H6 [G = MeSe (1), H (5), F (6), Cl (7) and Br (8) with X = lone pair (L), O (O), OH+ (OH+) and O2H2 (OH·OH)] will be discussed in detail, here. The results clarified the factors for the racemization of selenoxides. n[thin space (1/6-em)](OH·OH) (n = 1 and 5–8) must be the key intermediates in the racemization of n[thin space (1/6-em)](O), in the presence of (a trace of) water in solutions.

Table 3 Energies and relative energies for 8-G-1-[MeSe(OiHj)]C10H6 (i, j = 0, 1 and 2)a
FormO: A/AAbOH+: A/AAbOH·OH: AC
a Calculated with the B3LYP/6-311+G(d) method.b A for 5–8 and AA for 1.c Evaluated based on the values of E(H2O2) = −151.5891 au, E(H2O) = −76.4438 au and E(OH) = −75.8181 au calculated with the same method.d Relative to that of the corresponding n[thin space (1/6-em)](O): A.e Relative to the same structure derived from 5 (G = H) being given in parenthesis.f 7.1 kJ mol−1 from the corresponding species of 1 (G = trans-MeSe; O): AA.
5 (G = H)−2902.0303−2902.4017−2978.4686
 Qn(Se)1.3091.3071.324
 Qn(O)−0.968−0.837−0.996, −0.993
 Qn(H) 0.4970.433, 0.433
 +Wc−2978.4741−2978.2198−2978.4686
 Δdeas 0.0667.7 (as 0.0)14.4 (as 0.0)
6 (G = F)−3001.3000−3001.6744−3077.7371
 +Wc−3077.7438−3077.4925−3077.7371
 Δdeas 0.0659.8 (−7.9)17.6 (3.2)
7 (G = Cl)−3361.6478−3362.0250−3438.0833
 +Wc−3438.0916−3437.8431−3438.0833
 Δdeas 0.0652.4 (−15.2)21.8 (7.4)
8 (G = Br)−5475.5651−5475.9442−5552.0007
 +Wc−5552.0089−5551.7623−5552.0007
 Δdeas 0.0647.4 (−20.2)21.5 (7.1)
1 (G = trans-MeSe)−5342.8896−5343.2854−5419.3241
 +Wc−5419.3334−5419.1035−5419.3241
 Δdeas 0.0603.6 (−64.1)24.4 (10.0)
1 (G = cis-MeSe)−5342.8869−5343.2821−5419.3214
 +Wc−5419.3307−5419.1002−5419.3214
 Δdeas 0.0f612.3 (−55.4)31.5 (17.1)


Table 4 Second order perturbation energies in the donor (D)–acceptor (A) interactions of the n(G)⋯σ*(Se–O) type in 8-G-1-[MeSe(O)]C10H6 and 8-G-1-[MeSe+(OH)]C10H6, calculated with the NBO methodab
D; Anp(G); σ*(Se–O)np(G): σ*(Se+–OH)
a The 6-311+G(d) basis sets being employed.b In kcal mol−1.c Corresponding to the ns(G)⋯σ*(Se+–OH) interaction.d 0.76 kcal mol−1 for the ns(Se)⋯σ*(Se–O) type interaction.e The 6-311+G(3df) basis sets being employed for Se with the 6-311+G(3d,2p) basis sets for C and H.f Corresponding to the ns(Se)⋯σ*(Se–O) interactions.
G = F1.449.15 (0.87)c
G = Cl3.2913.65 (1.09)c
G = Br3.7327.95 (1.19)c
G = cis-SeMe4.77d34.99 (1.76)c
G = trans-SeMe5.5241.86 (2.69)c
G = trans-SeMee5.86 
G = trans-Se(O)Mee1.53 (×2)f 


Table 5 Second order perturbation energies in the donor–acceptor interactions of the n(G)⋯σ*(Se–O) type at the naphthalene 1,8-positions in 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO), calculated with the NBO methoda
Compoundro(Se, Se)/Åρb(rc)/eao−3Δρb(rc)/eao−5Hb(rc)/au
a The 6-311+G(3df) basis sets being employed for Se and the 6-311+G(3d,2p) basis sets for C and H.
1[thin space (1/6-em)](LO)3.25210.01950.0420−0.0005
1[thin space (1/6-em)](OO)3.28510.01600.03930.0002


Effect of G in 1 and 5–8

Racemization of an optically active selenoxide is believed to proceed via a selenide dihydroxide (n[thin space (1/6-em)](OH·OH)).4a–dScheme 3 shows a hypothetical racemization process of optically active n[thin space (1/6-em)](O*) vian[thin space (1/6-em)](OH·OH).

Protonation of n[thin space (1/6-em)](O*) occurs at O of an optically active isomer of n[thin space (1/6-em)](O*: R) to give n[thin space (1/6-em)](O*H+: R) at the initial stage of the reaction. n[thin space (1/6-em)](OH·OH) will form in the reaction of n[thin space (1/6-em)](O*H+: R) with water followed by the deprotonation to yield n[thin space (1/6-em)](OH·OH). Elimination of water from n[thin space (1/6-em)](OH·OH) results in the racemization, since of n[thin space (1/6-em)](OH·OH) is not optically active as a whole. Similar reactions occur starting from n[thin space (1/6-em)](O*: S) to yield n[thin space (1/6-em)](OH·OH) vian[thin space (1/6-em)](O*H+: S), which also leads to racemization. Water may originate from the solvent and the racemization would proceed under the neutral conditions. The stability of n[thin space (1/6-em)](OH·OH) must affect on the rates of racemization for the optical active selenoxides.

The effect of G on the stability of 8-G-1-[MeSe(OiHj)]C10H6 [1 and 5–8: L (i = j = 0), O (i = 1, j = 0), OH+ (i = j = 1) and OH·OH (i = j = 2)] are examined based on the QC calculations. The results of QC calculations performed with the B3LYP/6-311+G(d) method are collected in Table 3. Table 3 also contains natural charges (Qn) of Se and O calculated employing the natural population analysis.20Scheme 4 shows optimized structures of the global minimum for each of 1[thin space (1/6-em)](LL), 1[thin space (1/6-em)](LO) and 1 (LOH+), together with the three types, AA′, BB and AC, for 1 (LOH·OH). The values for AC of n[thin space (1/6-em)](LOH·OH) are given in Table 3, since AC is most stable among the three for each.34


Mechanism for racemization of n (O*) vian (OH·OH) (n = 1 and 5–8).
Scheme 3 Mechanism for racemization of n[thin space (1/6-em)](O*) vian[thin space (1/6-em)](OH·OH) (n = 1 and 5–8).

Optimized structures for 1 (G = SeMe) and the derivatives.
Scheme 4 Optimized structures for 1 (G = SeMe) and the derivatives.

Energy differences of the reactions in Scheme 3 are examined based on the values shown in Table 3. The energy of n[thin space (1/6-em)](O) + H2O (E(n[thin space (1/6-em)](O) + H2O)) is taken as the standard for each, for convenience of comparison. How are the selenoxides stabilized by G at the 8-position? The effect of G on the stabilization of selenoxides is examined before discussion the energy profile shown in Scheme 3.

Eqn (1) shows the energies of n[thin space (1/6-em)](L) + H2O2 (E(n[thin space (1/6-em)](L) + H2O2)) relative to E(n[thin space (1/6-em)](O) + H2O) [ΔE(n[thin space (1/6-em)](LO) = E(n[thin space (1/6-em)](L) + H2O2) −E(n[thin space (1/6-em)](O) + H2O)) (see Table S1 in the ESI). Similarly, eqn (2) and (3) exhibit ΔE(n[thin space (1/6-em)](OH+)) and ΔE(n[thin space (1/6-em)](OH·OH)),35 respectively, which are defined as [E(n[thin space (1/6-em)](OH+) + HO) −E(n[thin space (1/6-em)](O) + H2O)] and [E(n[thin space (1/6-em)](OH·OH)) −E(n[thin space (1/6-em)](O) + H2O)], respectively.36

 
ΔE(n[thin space (1/6-em)](LO)) = E(n[thin space (1/6-em)](L) + H2O2) −E(n[thin space (1/6-em)](O) + H2O)

G = H (121.8 kJ mol−1) < F (131.3) < cis-MeSe (133.9) < Cl (136.8) ≤ Br (137.6) < trans-MeSe (141.0)

(1)
 
ΔE(n[thin space (1/6-em)](OH+)) = E(n[thin space (1/6-em)](OH+) + HO) −E(n[thin space (1/6-em)](O) + H2O)

G = H (667.7 kJ mol−1) > F (659.8) > Cl (652.4) > Br (647.4) ≫cis-MeSe (605.2) > trans-MeSe (603.6)

(2)
 
ΔE(n[thin space (1/6-em)](OH·OH)) = E(n[thin space (1/6-em)](OH·OH)) −E(n[thin space (1/6-em)](O) + H2O)

G = H (14.4 kJ mol−1) < F (17.6) < Cl (21.8) ≈ Br (21.5) < trans-MeSe (24.4) < cis-MeSe (31.5)

(3)

The order in eqn (1) corresponds the energy lowering effect by the G⋯Se–O interactions in the formation selenoxides relative to the G⋯Se–C interactions in selenides. However, we must be careful to examine the values for G = cis-MeSe and trans-MeSe, since the structure of the corresponding selenide is commonly CC (see Table S1 in the ESI).

Eqn (2) exhibits that the protonation on the seleninyl O atom occurs more easily in the order of G = H < F < Cl < Br ≪cis-MeSe < trans-MeSe. The results show that the protonation occurs more easily when G become better donors, especially for G = MeSe. The evaluated ΔE(n[thin space (1/6-em)](OH+)) values are very large in magnitudes, however, they do not mean that the process is very difficult to occur. The large magnitudes are the results of the calculations for the charge separated species of the n[thin space (1/6-em)](OH+) + HO type. Only the relative values are important, since protonation will occur easily in solutions. Resulting hypervalent np(G)⋯σ*(Se–OH+) interactions stabilize further the species in the order shown in eqn (2), relative to the case of the selenoxides.

The activation energies for the racemization of optically active selenoxides are closely related to the values shown in eqn (3), although they are the energies for the intermediates, n[thin space (1/6-em)](OH·OH). The activation energies are expected to increase in this order. The activation energy for G = cis-MeSe is predicted to be larger than that with trans-MeSe. However, cis-MeSe and trans-MeSe isomers interconvert with each other. Therefore, it may be better to evaluate the value by G = trans-MeSe under the experimental conditions: The activation energy of 1[thin space (1/6-em)](LO) with G = MeSe is estimated to be about 10 kJ mol−1 larger than that of 5 (L) with G = H and the former is also larger than the case of G = Br by ca. 3 kJ mol−1. Fig. 2 summarizes the effect of G given in eqn (2).


Energies of n (OH·OH), relative to n (O) for n = 1 and 5–8.
Fig. 2 Energies of n[thin space (1/6-em)](OH·OH), relative to n[thin space (1/6-em)](O) for n = 1 and 5–8.

G at the 8-position will protect sterically from the racemization of an optical active n[thin space (1/6-em)](O*). G must stabilize the optical active n[thin space (1/6-em)](O*) and the protonated n[thin space (1/6-em)](O*H+) whereas G would destabilize n[thin space (1/6-em)](OH·OH). The steric congestion at the backside of the Se+–OH bond in n[thin space (1/6-em)](O*H+) by G will block the space for H2O to attack to produce n[thin space (1/6-em)](OH·OH) (Scheme 4). We must be careful, since G could also stabilize n[thin space (1/6-em)](OH·OH) in some cases. The calculated values might correspond to the total effects of the electronic and steric effects. Energy profiles for the racemization evaluated by above calculations must contain main factors. The energies for the transition states must be close to those of the intermediates, n[thin space (1/6-em)](OH·OH).

NBO analysis for n(G)⋯σ*(Se–O) interactions

Table 4 summarizes the second order perturbation energies (E(2)) for the charge transfer (CT) interactions of the n(G)⋯σ*(Se–O) type in 8-G-1-[MeSe(O)]C10H6 and 8-G-1-[MeSe+(OH)]C10H6 evaluated with the NBO method.37 The B3LYP/6-311+G(d) method is employed for the calculations. The E(2) values becomes larger in an order shown in eqn (4).
 
E(2): G = F (1.44) < Cl (3.29) < Br (3.73) < cis-MeSe (4.77) < trans-MeSe (5.52)(4)

The E(2) values are also evaluated for 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO), employing the 6-311+G(3df) basis sets for Se and the 6-311+G(3d,2p) basis sets for C and H at the B3LYP level.38Table 4 also contains the values. The np(G)⋯σ*(Se–O) interaction are evaluated to be 5.9 kcal mol−1 for 1[thin space (1/6-em)](LO)39 and as 1.5 (× 2) kcal mol−1 for the ns(G)⋯σ*(Se–O) interactions in 1[thin space (1/6-em)](OO). The larger value for 1[thin space (1/6-em)](LO) relative to 1[thin space (1/6-em)](OO) implies the more effective interaction of the np(G)⋯σ*(Se–O) type in 1[thin space (1/6-em)](LO). The contribution of the 4c–4e interaction of the O–Se⋯Se–O type was not detected by the NBO analysis. Fig. 3 summarizes the interactions.


The np(G)⋯σ*(Se–O) interaction in 1 (LO) and the ns(G)⋯σ*(Se–O) interactions in 1 (OO) evaluated by the NBO method.
Fig. 3 The np(G)⋯σ*(Se–O) interaction in 1[thin space (1/6-em)](LO) and the ns(G)⋯σ*(Se–O) interactions in 1[thin space (1/6-em)](OO) evaluated by the NBO method.

The nature of the np(G)⋯σ*(Se–O) interaction in 1[thin space (1/6-em)](LO) and the ns(G)⋯σ*(Se–O) interactions in 1[thin space (1/6-em)](OO) are evaluated based on the AIM analysis, next.

AIM analysis of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO)

The AIM analysis are carried out on 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO). The 6-311+G(3df) basis sets are employed for Se and the 6-311+G(3d,2p) basis sets for C and H at the B3LYP level. Table 5 collects the AIM parameters of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) for the bond critical points (BCPs: rc) on the interaction lines between non-bonded Se atoms.

The low values of electron densities at BCPs (ρb(rc)) in 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) (0.016–0.020 eao−3) show that the interactions are ionic in nature. Laplacian values of ρb(rc) (Δρb(rc)) are both positive, whereas the total electron energy densities at BCPs (Hb(rc)) for 1[thin space (1/6-em)](LO) is negative but it is positive for 1[thin space (1/6-em)](OO). The results strongly suggest that the np(G)⋯σ*(Se–O) interaction in 1[thin space (1/6-em)](LO) is the CT interaction in nature similarly to the case of R2Se⋯Br2 (MC) but the ns(G)⋯σ*(Se–O) interactions in 1[thin space (1/6-em)](OO) seems weaker than such CT interactions.40

Fig. 4 shows the counter map of ρb(rc) in the SeSeC9 plane for 1[thin space (1/6-em)](LO), together with BCPs (ugraphic, filename = b809763a-u1.gif), ring critical points (ugraphic, filename = b809763a-u2.gif), bond paths and the interaction lines. BCP are detected on the Se⋯Se and O⋯2H interaction lines. The BCP on the Se⋯Se interaction line well visualize the np(Se)⋯σ*(Se–O) interaction in 1[thin space (1/6-em)](LO). While BCP is also detected on the O⋯2H interaction line, the interaction is very small. A similar counter map is also drawn for 1[thin space (1/6-em)](OO), which is shown in Fig. S2 of the ESI.


Contour map of ρb(rc) for 1 (LO) in the SeSeC9 plane, together with BCPs (), ring critical points () and bond paths. The contours [eao−3] are at 2l (l = ±8, ±7,…0) and 0.0047 (heavy line). Two Me groups are located upside and downside of the SeSeC9 plane. The C2, C3, C6 and C7 atoms with the C–H bonds deviate substantially from the plane.
Fig. 4 Contour map of ρb(rc) for 1[thin space (1/6-em)](LO) in the SeSeC9 plane, together with BCPs (ugraphic, filename = b809763a-u3.gif), ring critical points (ugraphic, filename = b809763a-u4.gif) and bond paths. The contours [eao−3] are at 2l (l = ±8, ±7,…0) and 0.0047 (heavy line). Two Me groups are located upside and downside of the SeSeC9 plane. The C2, C3, C6 and C7 atoms with the C–H bonds deviate substantially from the plane.

Conclusion

X-Ray crystallographic analysis of 8-methylselanyl-1-(methylseleninyl)naphthalene (1[thin space (1/6-em)](LO)) and 1,8-bis(methylseleninyl)naphthalene 1[thin space (1/6-em)](OO) revealed that the three Se⋯Se[double bond, length as m-dash]O atoms in 1[thin space (1/6-em)](LO) and the four O[double bond, length as m-dash]Se⋯Se[double bond, length as m-dash]O atoms in 1[thin space (1/6-em)](OO) align linearly. All Se–O bonds are placed in the naphthyl plane. The superior tendency for the Se–O bonds to stay on the naphthyl plane (O dependence) must be the driving force for the fine structures of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO). The noncovalent np(Se)⋯σ(Se–O) 3c–4e interactions (G dependence) operate effectively to stabilize the structure of 1[thin space (1/6-em)](LO). On the other hand, the driving force for the structure of 1[thin space (1/6-em)](OO) must mainly come from the O dependence for each Se–O bond in 1[thin space (1/6-em)](OO), since the G dependence cannot operate without np(Se).

QC calculations clarify the factors that protect from racemization of selenoxides. The energies of 8-G-1-[MeSe(OH)2]C10H6 from (8-G-1-[MeSe(O)]C10H6 + H2O) are shown to be in an order of G = H (14.4 kJ mol−1) < F (17.6) < Cl (21.8) ≈ Br (21.5) < trans-SeMe (24.4) < cis-SeMe (31.5). The activation energies for the racemization should increase in this order, since 8-G-1-[MeSe(OH)2]C10H6 must be the key intermediates. The activation energy of 1 (LO: G = MeSe) is evaluated to be larger than that of 5 (L: G = H) and 8 (L: G = Br) by 10 and 3 kJ mol−1, respectively. The results will help to design the optically stable selenoxides. The NBO and AIM analyses support the discussion and visualize the interactions.

Investigations on the chiral 3a[thin space (1/6-em)](LO), prepared in the oxidation of 3a[thin space (1/6-em)](LL) with chiral reagents, are in progress. Details will be reported elsewhere.

Experimental

General considerations

Manipulations were performed under an argon atmosphere with standard vacuum-line techniques. Glassware was dried at 130 °C overnight. Solvents and reagents were purified by standard procedures if necessary. Melting points were determined on a Yanaco MP-S3 melting point apparatus and uncorrected. NMR spectra were recorded at room temperature on a JEOL AL-300 spectrometer (1H, 300 MHz; 13C, 75 MHz) and on a JEOL Lambda-400 spectrometer (1H, 400 MHz; 77Se, 76 MHz). The 1H, 13C and 77Se NMR spectra were recorded in CDCl3. Chemical shifts are given in ppm relative to Me4Si for the 1H and 13C NMR spectra and relative to reference compound MeSeMe for the 77Se NMR spectra. Column chromatography was performed by using silica gel (Fujishilysia PSQ-100B) and basic alumina (E. Merck) and analytical thin layer chromatography was performed on precoated silica gel plates (60F-254) with the systems (v/v) indicated.

Syntheses

Bis(methylselanyl 1,8-bis(methylselanyl)naphthalene (1[thin space (1/6-em)](LL)). To a solution of the dianion of naphtho[1,8-c,d]-1,2-diselenole, which was prepared by reduction of the diselenole 923 (1.03 g, 3.64 mmol) with NaBH4 in an aqueous THF solution, was added methyl iodide (1.29 g, 9.06 mmol) at room temperature. After a usual workup, the crude was purified by column chromatography (flash column, SiO2, hexane). Recrystallization of the chromatographed product from hexane gave 1[thin space (1/6-em)](LL) as colorless prisms in 98% yield, mp 85.0–85.5 °C, 1H NMR (300 MHz, CDCl3, δ, ppm, TMS): 2.33 (s, 6H), 7.32 (t, 2H, J = 7.7 Hz), 7.70 (dd, 2H, J = 1.2 and 8.2 Hz), 7.73 (dd, 2H, J = 1.2 and 7.5 Hz); 13C NMR (75 MHz, CDCl3, δ, ppm, TMS): 13.3, 125.7, 128.3, 131.9, 132.3, 135.3, 135.6; 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 231.4. Anal. Calc. for 1[thin space (1/6-em)](LL) (C12H12Se2): C, 45.88; H, 3.85%. Found: C, 45.73; H, 3.77%.
8-Methylselanyl-1-(methylseleninyl)naphthalene (1[thin space (1/6-em)](LO)). 1[thin space (1/6-em)](LL) (0.98 mg, 3.12 mmol) was dissolved in 20 mL of CH2Cl2 and the solution was bubbling with the ozone for 5 min. TLC was checked for the completion of the reaction (rf = 0.07 (chloroform)). Then the solution was evaporated and dried in vacuo. The crude product was purified by column chromatography (flash column, Al2O3, CH2Cl2). 1[thin space (1/6-em)](LO) gave 85% yield as colorless powder, mp 129.8–130.1 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 2.29 (s, 3H), 2.78 (s, 3H), 7.48 (t, J 7.6 Hz, 2H), 7.76 (t, J 7.7 Hz, 2H), 7.98–8.05 (m, 2H), 8.10 (dd, J 1.1 and 7.2 Hz, 1H), 8.88 (dd, J 1.2 and 7.4 Hz, 1H); 13C NMR (75 MHz, CDCl3, δ, ppm, TMS): 13.87, 41.12, 125.73, 126.28, 126.35, 126.57, 131.01, 132.44, 133.06, 136.13, 138.93, 141.34; 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 210.8, 833.0. Anal. Calc. for 1[thin space (1/6-em)](LO) (C12H12OSe2): C, 43.66; H, 3.66%. Found: C, 43.61; H, 3.60%.
1,8-Bis(methylseleninyl)naphthalene (1[thin space (1/6-em)](OO)). 1[thin space (1/6-em)](LL) (0.58 g, 0.30 mmol) was dissolved in 20 mL of CH2Cl2 and the solution was bubbling with the ozone for 15 min. TLC was checked for the completion of the reaction (rf = 0.00 (chloroform)). Then the solution was evaporated and dried in vacuo. The crude product was purified by column chromatography (flash column, Al2O3, CH2Cl2). 1[thin space (1/6-em)](OO) gave 59% yield as colorless powder, mp 154.8–155.2 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 2.71 (s, 6H), 7.84 (t, J 7.7 Hz, 2H), 8.18 (dd, J 1.2 and 6.9 Hz, 2H), 8.71 (dd, J 1.4 and 6.9 Hz, 2H); 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 821.3. Anal. Calc. for 1[thin space (1/6-em)](OO) (C12H12O2Se2): C, 41.64; H, 3.49%. Found: C, 41.55; H, 3.45%. Anal. Calc. for 1[thin space (1/6-em)](OO)·2.5H2O (C24H24O4Se4·5H2O): C, 36.84; H, 4.38%. Found: C, 36.87; H, 4.41%.
1,8-Bis(ethylselanyl)naphthalene (2[thin space (1/6-em)](LL)). Following the similar method to that used for 1[thin space (1/6-em)](LL), 2[thin space (1/6-em)](LL) gave 80% yield as colorless powder, mp 52.3–52.8 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 1.35 (t, J 7.4 Hz, 6H), 2.89 (q, J 7.5 Hz, 4H), 7.32 (t, J 7.6 Hz, 2H), 7.70 (dd, J 1.2 and 8.1 Hz, 2H), 7.76 (dd, J 1.1 and 7.2 Hz, 2H); 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 341.7. Anal. Calc. for 2[thin space (1/6-em)](LL) (C14H16Se2): C, 49.14; H, 4.71%. Found: C, 49.23; H, 4.72%.
8-Phenylselanyl-1-(methylseleninyl)naphthalene (3a[thin space (1/6-em)](LO)). Following the similar method to that used for 1[thin space (1/6-em)](LO), 3a[thin space (1/6-em)](LO) gave 80% yield as colorless needles, mp 129.8–130.2 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 2.72 (s, 3H), 6.98–7.02 (m, 2H), 7.11–7.16 (m, 3H), 7.56 (t, J 7.6 Hz, 1H), 7.76 (t, J 7.7 Hz, 1H), 8.05 (dd, J 1.2 and 8.0 Hz, 1H), 8.10 (dd, J 1.3 and 8.1 Hz, 1H), 8.15 (dd, J 1.3 and 7.2 Hz, 1H), 8.82 (dd, J 1.3 and 7.3 Hz, 1H); 13C NMR (75 MHz, CDCl3, δ, ppm, TMS) 40.56, 123.19, 126.51, 126.57, 126.75, 126.88, 128.42 (2J(Se,C) 5.9 Hz), 129.63, 131.95, 132.42, 133.03, 133.50, 136.29, 140.89, 141.37; 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 398.2, 831.4. Anal. Calc. for 3a[thin space (1/6-em)](LO) (C17H14OSe2): C, 52.06; H, 3.60%. Found: C, 52.11; H, 3.66%.
8-Phenylseleninyl-1-(methylseleninyl)naphthalene (3a[thin space (1/6-em)](OO)). Following the similar method to that used for 1[thin space (1/6-em)](OO), 3a[thin space (1/6-em)](OO) gave 63% yield as colorless needles, mp 148.0–148.8 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 2.74 (s, 3H), 7.33–7.50 (m, 3H), 7.51–7.58 (m, 2H), 7.78 (t, J 7.7 Hz, 1H), 7.81 (t, J 7.7 Hz, 1H), 8.13 (dd, J 1.1 and 8.1 Hz, 1H), 8.14 (dd, J 1.1 and 8.1 Hz, 1H), 8.63 (dd, J 1.4 and 7.4 Hz, 1H), 8.72 (dd, J 1.3 and 7.3 Hz, 1H); 13C NMR (75 MHz, CDCl3, δ, ppm, TMS): 38.25, 126.72, 126.80, 126.85, 127.01, 127.64, 127.92, 130.02, 131.70, 133.33, 133.71, 135.55, 138.88, 139.22, 141.66; 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 820.0, 832.5. Anal. Calc. for 3a[thin space (1/6-em)](OO) (C17H14O2Se2): C, 50.02; H, 3.46%. Found: C, 50.07; H, 3.57%.
8-p-Anisylselanyl-1-(methylseleninyl)naphthalene (3b[thin space (1/6-em)](LO)). Following the similar method to that used for 1[thin space (1/6-em)](LO), 3b[thin space (1/6-em)](LO) gave 88% yield as colorless needles, mp 129.6–130.4 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 2.70 (s, 3H), 3.82 (s, 3H), 6.70 (d, J 8.8 Hz, 2H), 7.01 (d, J 8.8 Hz, 2H), 7.51 (t, J 7.2 Hz, 1H), 7.74 (t, J 7.2 Hz, 1H), 7.88 (dd, J 1.1 and 6.8 Hz, 1H), 8.01 (dd, J 1.1 and 6.8 Hz, 1H), 8.03 (dd, J 1.1 and 6.8 Hz, 1H), 8.10 (dd, J 1.1 and 6.8 Hz, 1H); 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 385.9, 833.9. Anal. Calc. for 3b[thin space (1/6-em)](LO) (C18H16O2Se2): C, 51.20; H, 3.82%. Found: C, 50.98; H, 3.83%.
8-p-Anisylseleninyl-1-(methylseleninyl)naphthalene (3b[thin space (1/6-em)](OO)). Following the similar method to that used for 1[thin space (1/6-em)](OO), 3b[thin space (1/6-em)](OO) gave 43% yield as colorless powder, mp 144.5–145.0 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 2.75 (s, 3H), 3.76 (s, 3H), 6.87 (d, J 8.9 Hz, 2H), 7.45 (d, J 8.9 Hz, 2H), 7.83 (t, J 7.7 Hz, 2H), 8.15 (dd, J 1.0, 8.2 Hz, 1H), 8.17 (dd, J 1.0, 8.2 Hz, 1H), 8.69 (dd, J 1.3, 9.1 Hz, 1H), 8.71 (dd, J 1.2, 9.1 Hz, 1H); 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 821.6, 846.4. Anal. Calc. for 3b[thin space (1/6-em)](OO) (C18H16O3Se2): C, 49.33; H, 3.68%. Found: C, 49.30; H, 3.73%.
8-p-Nitrophenylselanyl-1-(methylseleninyl)naphthalene (3d[thin space (1/6-em)](LO)). Following the similar method to that used for 1[thin space (1/6-em)](LO), 3d[thin space (1/6-em)](LO) gave 61% yield as colorless powder, mp 141.5–142.0 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 2.67 (s, 3H), 7.07 (dt, J 2.1 and 9.0 Hz, 2H), 7.64 (t, J 7.5 Hz, 1H), 7.83 (t, J 7.5 Hz, 1H), 7.99 (dt, J 2.4 and 9.0 Hz, 2H), 8.11 (dd, J 1.2 and 6.9 Hz, 2H), 8.18 (dd, J 1.2 and 4.2 Hz, 1H), 8.21 (dd, J 1.5 and 4.8 Hz, 1H), 8.84 (dd, J 1.2 and 6.0 Hz, 1H); 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 426.4, 835.6. Anal. Calc. for 3d[thin space (1/6-em)](LO) (C17H13NO3Se2): C, 46.70; H, 3.00; N, 3.20%. Found: C, 46.75; H, 3.03; N, 3.22%.
8-p-Nitrophenylseleninyl-1-(methylseleninyl)naphthalene (3d[thin space (1/6-em)](OO)). Following the similar method to that used for 1[thin space (1/6-em)](OO), 3d[thin space (1/6-em)](OO) gave 82% yield as colorless powder, mp 151.2–152.0 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 2.83 (s, 3H), 7.72–7.92 (m, 4H), 8.12–8.27 (m, 4H), 8.57 (dd, J 1.1 and 6.2 Hz, 1H), 8.74 (dd, J 1.3 and 6.1 Hz, 1H); 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 821.4, 849.0. Anal. Calc. for 3d[thin space (1/6-em)](OO) (C17H13NO4Se2): C, 45.05; H, 2.89; N, 3.09%. Found: C, 45.12; H, 2.83; N, 3.12%.
1,8-Bis(phenylselanyl)naphthalene (4a[thin space (1/6-em)](LL)). Under an argon atmosphere, 1,8-diiodonaphthalene (4.33 g, 11.40 mmol) was dissolved in 100 mL of dry THF and the solution was added to nBuLi (15.0 mL, 23.94 mmol, 1.6 N) at −78 °C. After 20 min, a THF solution of phenylselenobromide (22.80 mmol) was added to the above solution at −78 °C. Then the reaction mixture was stirring for 2 h and warmed up room temperature. Then, 20 mL of 5% acetone hydrochloric acid and 100 mL of benzene were added. The organic layer was separated, washed with brine, 10% aqueous solution of sodium hydroxide, saturated aqueous solution of sodium bicarbonate and brine. Then the solution was dried over sodium sulfate, evaporated and dried in vacuo. The crude product was purified by column chromatography (flash column, SiO2, hexane). 4a[thin space (1/6-em)](LL) gave 89% yield as yellow prisms, mp 64.0–64.8 °C; 1H NMR (300 MHz, CDCl3, δ, ppm, TMS): 7.22–7.28 (m, 8H), 7.39–7.45 (m, 4H), 7.64 (dd, J 1.1 and 7.3 Hz, 2H), 7.74 (dd, J 1.1 and 8.3 Hz, 2H); 13C NMR (75 MHz, CDCl3, δ, ppm, TMS): 126.0, 127.4, 129.2, 129.4, 131.4, 133.4, 135.18, 135.19, 135.5, 135.9; 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 435.4. Anal. Calc. for 4a[thin space (1/6-em)](LL) (C22H16Se2): C, 60.29; H, 3.68%. Found: C, 60.21; H, 3.75%.
8-Phenylselanyl-1-(phenylseleninyl)naphthalene (4a[thin space (1/6-em)](LO)). Following the similar method to that used for 1[thin space (1/6-em)](LO), 4a[thin space (1/6-em)](LO) gave 65% yield as colorless prisms, mp 155.5–156.3 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 6.90–6.95 (m, 4H), 7.10–7.13 (m, 6H), 7.22–7.26 (m, 6H), 7.48–7.53 (m, 4H), 7.52 (t, J 8.2 Hz, 1H), 7.83 (d, J 7.7 Hz, 1H), 8.07 (dd, J 1.3 and 7.2 Hz, 1H), 8.08 (dd, J 1.3 and 8.2 Hz, 1H), 9.02 (dd, J 1.3 and 7.3 Hz, 1H); 13C NMR (75 MHz, CDCl3, δ, ppm, TMS): 123.90, 126.45, 126.51, 126.79, 127.86, 127.91, 128.70, 129.17, 129.49, 130.11, 131.73, 132.76, 133.27, 133.78, 136.31, 140.17, 140.71, 146.21; 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 400.1, 863.7. Anal. Calc. for 4a[thin space (1/6-em)](LO) (C22H16OSe2): C, 58.17; H, 3.55%. Found: C, 58.11; H, 3.65%.
1,8-Bis(phenylseleninyl)naphthalene (4a[thin space (1/6-em)](OO)). Following the similar method to that used for 1[thin space (1/6-em)](OO), 4a[thin space (1/6-em)](OO) gave 78% yield as colorless prisms, mp. 187.5–188.3 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 7.21–7.30 (m, 8H), 7.37 (tt, J 1.5 and 6.8 Hz, 2H), 7.76 (t, J 7.7 Hz, 2H), 8.15 (dd, J 0.9 and 7.5 Hz, 2H), 8.47 (dd, J 1.1 and 6.2 Hz, 2H); 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 877.1. Anal. Calc. for 4a[thin space (1/6-em)](OO) (C22H16O2Se2): C, 56.19; H, 3.43%. Found: C, 56.22; H, 3.53%.
1,8-Bis[(p-tert-butylphenyl)selanyl]naphthalene (4c[thin space (1/6-em)](LL)). Following the similar method to that used for 4a[thin space (1/6-em)](LL), 4c[thin space (1/6-em)](LL) gave 87% yield as yellow prisms, mp 97.8–98.3 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 1.30 (s 18H), 7.24 (t, J 7.7 Hz, 2H), 7.27 (d, J 8.6 Hz, 4H), 7.38 (d, J 8.6 Hz, 4H), 7.65 (dd, J 1.3 and 6.1 Hz, 2H), 7.73 (dd, J 1.3 and 7.0 Hz, 2H); 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 424.6. Anal. Calc. for 4c[thin space (1/6-em)](LL) (C30H32Se2): C, 65.45; H, 5.86%. Found: C, 65.41; H, 5.88%.
8-[(p-tert-Butylphenyl)selanyl]-1-[(p-tert-butylphenyl)seleninyl]naphthalene (4c[thin space (1/6-em)](LO)). Following the similar method to that used for 1[thin space (1/6-em)](LO), 4c[thin space (1/6-em)](LO) gave 86% yield as colorless powder, mp 179.5–180.2 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 1.22 (s, 9H), 1.27 (s 9H), 6.91 (d, J 8.3 Hz, 2H), 7.15 (d, J 8.1 Hz, 2H), 7.28 (d, J 8.8 Hz, 2H), 7.43 (d, J 8.6 Hz, 2H), 7.51 (t, J 7.9 Hz, 1H), 7.82 (t, J 7.7 Hz, 1H), 8.07 (d, J 8.3 Hz, 3H), 9.01 (dd, J 1.3 and 7.5 Hz, 1H); 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 393.2, 861.2. Anal. Calc. for 4c[thin space (1/6-em)](LO) (C30H32OSe2): C, 63.61; H, 5.69%. Found: C, 63.55; H, 5.58%.
1,8-Bis[(p-tert-butylphenyl)seleninyl]naphthalene (4c[thin space (1/6-em)](OO)). Following the similar method to that used for 1[thin space (1/6-em)](OO), 4c[thin space (1/6-em)](OO) gave 87% yield as colorless powder, mp 172.5–173.2 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 1.63 (s, 18H), 7.39 (d, J 8.6 Hz, 4H), 7.47 (d, J 8.3 Hz, 4H), 7.83 (d, J 7.6 Hz, 2H), 8.16 (dd, J 0.8 and 7.3 Hz, 2H), 8.73 (dd, J 1.0 and 6.2 Hz, 2H); 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 843.7. Anal. Calc. for 4c[thin space (1/6-em)](OO) (C30H32O2Se2): C, 61.86; H, 5.54%. Found: C, 61.93; H, 5.58%.
1-(Methylselanyl)naphthalene (5 (L)). Following the similar method to that used for 1[thin space (1/6-em)](LL), 5 (L) gave 99% yield as pale yellow oil; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 2.37 (s, 2JSe,H 11.7 Hz, 3H), 7.35 (dd, J 7.3 and 8.1 Hz, 1H), 7.47 (ddd, J 1.6, 6.9 and 8.2 Hz, 1H), 7.53 (ddd, J 1.6, 6.9 and 8.3 Hz, 1H), 7.66 (dd, J 1.1 and 7.3 Hz, 1H), 7.71 (d, J 8.2 Hz, 1H), 7.80 (dd, J 1.7 and 7.9 Hz, 1H), 8.24 (ddd, J 0.7, 1.6 and 8.1 Hz, 1H); 13C NMR (75 MHz, CDCl3, δ, ppm, TMS): 36.54, 122.08 (J 14.9 Hz), 124.03 (J 6.2 Hz), 126.11, 126.79, 127.56, 129.35, 130.27, 131.40, 133.88, 138.68; 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 158.6. Anal. Calc. for 5 (L) (C11H10Se): C, 59.74; H, 4.56%. Found: C, 59.90; H, 4.49%.
1-(Methylseleninyl)naphthalene (5[thin space (1/6-em)](O)). Following the similar method to that used for 1[thin space (1/6-em)](LO), 5[thin space (1/6-em)](O) gave 67% yield as colorless needles, mp 97.2–97.8 °C; 1H NMR (400 MHz, CDCl3, δ, ppm, TMS): 2.71 (s, 2JSe,H 12.3 Hz, 3H), 7.56–7.65 (m, 2H), 7.70 (dd, J 7.4 and 8.2 Hz, 1H), 7.81–7.87 (m, 1H), 7.95–8.02 (m, 2H), 8.29 (dd, J 1.1 and 7.3 Hz, 1H); 13C NMR (75 MHz, CDCl3, δ, ppm, TMS): 7.52, 125.83, 126.14, 126.39, 126.63, 127.16, 128.58, 128.67, 131.10, 133.29, 133.77; 77Se NMR (76 MHz, CDCl3, δ, ppm, Me2Se): 809.3. Anal. Calc. for 5[thin space (1/6-em)](O) (C11H10OSe): C, 55.71; H, 4.25%. Found: C, 55.88; H, 4.18%.
X-Ray crystal structure determination. The colorless crystals of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) were grown by slow evaporation of methylene dichloride-hexane solutions at room temperature. A crystal of 1[thin space (1/6-em)](LO) was measured on a Rigaku AFC5R diffractometer with graphite monochromated Mo-Kα radiation source (λ = 0.71069 Å) and a rotating anode generator at 298(2) K. That of 1[thin space (1/6-em)](OO) was measured on a Rigaku/MSC Mercury CCD diffractometer equipped with a graphite-monochromated Mo-Kα radiation source (λ = 0.71070 Å) at 103(2) K. The structures of 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) were solved by direct method (SHELXS-97)41 and refined by full-matrix least-square method on F2 for all reflections (SHELXL-97).42 All the non-hydrogen atoms were refined anisotropically.

QC calculations

QC calculations are performed on 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO), as the models of n[thin space (1/6-em)](LO) and n[thin space (1/6-em)](OO) (n = 1, 3 and 4), respectively, employing the 6-311+G(d) basis sets of the Gaussian 98 program.27 Calculations are performed at the density functional theory (DFT) level of the Becke three parameter hybrid functionals combined with the Lee-Yang-Parr correlation functional (B3LYP).28,29 QC calculations are also performed on 8-G-1-[MeSe(X)]C10H6 [G = MeSe (1), H (5), F (6), Cl (7) and Br (8) with X = lone pair (L), O (O), OH+ (OH+) and O2H2 (OH·OH)], employing the B3LYP/6-311+G(d) method. The NBO19,20 analysis were performed with the B3LYP/6-311+G(d) method. The AIM21,22 analysis are performed on 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) with the Gaussian 03 program employing the 6-311+G(3df) basis sets for Se with the 6-311+G(3d,2p) basis sets for C and H at the B3LYP level. They are analyzed employing the AIM 2000 program.21,22 NBO analysis are also performed on 1[thin space (1/6-em)](LO) and 1[thin space (1/6-em)](OO) with the same method for the AIM analysis. Optimized structures and the molecular orbitals are drawn using MolStudio R3.2 (Rev 1.0).43

Acknowledgements

This work was partially supported by a Grant-in-Aid for Scientific Research (Nos. 16550038, 19550041 and 20550042) from the Ministry of Education, Culture, Sports, Science and Technology, Japan.

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  32. M. J. Frisch, G. W. Trucks, H. B. Schlegel, G. E. Scuseria, M. A. Robb, J. R. Cheeseman, J. A. Montgomery, Jr, T. Vreven, K. N. Kudin, J. C. Burant, J. M. Millam, S. S. Iyengar, J. Tomasi, V. Barone, B. Mennucci, M. Cossi, G. Scalmani, N. Rega, G. A. Petersson, H. Nakatsuji, M. Hada, M. Ehara, K. Toyota, R. Fukuda, J. Hasegawa, M. Ishida, T. Nakajima, Y. Honda, O. Kitao, H. Nakai, M. Klene, X. Li, J. E. Knox, H. P. Hratchian, J. B. Cross, V. Bakken, C. Adamo, J. Jaramillo, R. Gomperts, R. E. Stratmann, O. Yazyev, A. J. Austin, R. Cammi, C. Pomelli, J. W. Ochterski, P. Y. Ayala, K. Morokuma, G. A. Voth, P. Salvador, J. J. Dannenberg, V. G. Zakrzewski, S. Dapprich, A. D. Daniels, M. C. Strain, O. Farkas, D. K. Malick, A. D. Rabuck, K. Raghavachari, J. B. Foresman, J. V. Ortiz, Q. Cui, A. G. Baboul, S. Clifford, J. Cioslowski, B. B. Stefanov, G. Liu, A. Liashenko, P. Piskorz, I. Komaromi, R. L. Martin, D. J. Fox, T. Keith, M. A. Al-Laham, C. Y. Peng, A. Nanayakkara, M. Challacombe, P. M. W. Gill, B. Johnson, W. Chen, M. W. Wong, C. Gonzalez and J. A. Pople, GAUSSIAN 03 (Revision B.05), Gaussian, Inc., Pittsburgh, PA, 2003 Search PubMed.
  33. The AIM2000 program (Version 2.0) is employed to analyze and visualize atoms in molecules: F. J. Biegler-König, Comput. Chem., 2000, 21, 1040–1048 Search PubMed ; see also ref. 22g.
  34. Data for A and B, together with LL, are given in the ESI.
  35. The type C of 1[thin space (1/6-em)](OH·OH) is discussed which is predicted to be most stable among the three44.
  36. Eqn (R1) shows the energies of n[thin space (1/6-em)](L) + H2O2 (E(n[thin space (1/6-em)](L) + H2O2)) relative to E(n[thin space (1/6-em)](O) + H2O) [ΔE(n[thin space (1/6-em)](LO)) = E(n[thin space (1/6-em)](L) + H2O2) −E(n[thin space (1/6-em)](O) + H2O)], although E(n[thin space (1/6-em)](L)) are not given in Table 3.45
     
    ΔE(n[thin space (1/6-em)](LO)) = E(n[thin space (1/6-em)](L) + H2O2) −E(n[thin space (1/6-em)](O) + H2O) 

    G = H (121.8 kJ mol−1) < F (131.3) < cis-MeSe (133.9) < Cl (136.8) ≤ Br (137.6) < trans-MeSe (141.0)

    (R1)
    .
  37. NOB analysis were also performed on the AC conformer of 8-G-1-[MeSe(O2H2)]C10H6. However, the corresponding CT interactions were not detected.
  38. The nonbonded Se⋯Se distance in 1[thin space (1/6-em)](LO) is predicted to be shorter than that of 1[thin space (1/6-em)](OO) by ca. 0.03 Å, while the observed values are almost equal (see Table 5). The crystal packing effect might contribute to the results.
  39. The value is very close to that evaluated with the B3LYP/6-311+G(d) method.
  40. W. Nakanishi, S. Hayashi and K. Narahara, unpublished results.
  41. G. M. Sheldrick, SHELXS-97, Program for Crystal Structure Solution, Universität Göttingen, Germany, 1997.
  42. G. M. Sheldrick, SHELXL-97, Program for Crystal Structure Refinement, University of Göttingen, Germany, 1997.
  43. MolStudio R3.2 (Rev 1.0), NEC Corporation, 1997–2003.
  44. Three structures (type A, type B and type C) were optimized for each of n[thin space (1/6-em)](OH·OH). The type C is the global minimum, which is slightly stable than type B and much stable than type A, although the steric repulsion between OH and G seems largest.
  45. Eqn (R1)36 shows that selenoxides are stabilized in this order through the non-bonded n(G)⋯σ*(Se–O) 3c–4e interactions, together with the O dependence.16 While G = trans-MeSe is demonstrated to be most effective to stabilize in the selenoxide relative to the corresponding bis-selenide, the effect of G = cis-MeSe places between F and Cl, where the CC form is postulated for the bis-selenide.

Footnote

Electronic supplementary information (ESI) available: Energies and relative energies for 8-G-1-[MeSe(X)]C10H6 [G = MeSe (1), H (5), F (6), Cl (7) and Br (8) with X = lone pair (L), O[thin space (1/6-em)](O), OH+ (OH+) and O2H2[thin space (1/6-em)](OH·OH)], the packing structures of 1[thin space (1/6-em)](OO), counter map for 1[thin space (1/6-em)](OO), Cartesian coordinates for optimized structures of 1 and 5–8 with X = lone pair (L), O[thin space (1/6-em)](O), OH+ (OH+) and O2H2[thin space (1/6-em)](OH·OH)]. CCDC reference numbers 688690 (1[thin space (1/6-em)](LO)) and 688691 (1[thin space (1/6-em)](OO)). For ESI and crystallographic data in CIF or other electronic format see DOI: 10.1039/b809763a

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