Theoretical studies on the stability of phenylpentazole and its substituted derivatives of –OH, –OCH3, –OC2H5 and –N(CH3)2

Xueli Zhang, Junqing Yang, Ming Lu and Xuedong Gong*
School of Chemical Engineering, Nanjing University of Science and Technology, Nanjing 210094, China. E-mail: gongxd325@mail.njust.edu.cn

Received 18th September 2014 , Accepted 20th October 2014

First published on 21st October 2014


Abstract

Phenylpentazole (PhN5) and its derivatives with 1–3 electron donating substituents (–OH, –OCH3, –OC2H5 and –N(CH3)2) were studied using density functional theory. The pyrolysis mechanism and effects of substituents on stabilities were discussed. The activation energies (Eas, 362–402 kJ mol−1) for the cleavage of the C–N bonds linking the aryl and the pentazole are far larger than those (109–117 kJ mol−1) for the breaking of the N–N bonds in the pentazole ring. Decomposition of the pentazole ring should be the initial step of pyrolysis of arylpentazole and its derivatives. The pentazole ring in PhN5 is stabilized by substituents which increase the electron density and strengthen the delocalization of the N5 ring. The abilities of these substituents to improve Ea and to decrease the frontier orbital energy gap (Eg) have the same order: –N(CH3)2 > –OC2H5 > –OCH3 > –OH.


1. Introduction

Nitrogen-rich compounds, such as triazole, tetrazole and pentazole, are important azole-ring compounds. They are extensively found in purine, pyrimidine and natural products,1 and many synthetic drugs also contain these nitrogen-rich azole rings.2 In addition, azole compounds have high nitrogen contents, high heats of formation (HOFs), high solid-state densities3–8 and more environmentally benign decomposition products. Hence, they are widely used in medicinal chemistry and the military,2,9,10 and have been attracting significant interest in recent years.

Many triazole and tetrazole derivatives have been synthesized and studied.11–21 Great progresses have been made in developing compounds based on triazole or tetrazole. On the other hand, researches on pentazole, which has an all-nitrogen five-membered ring and possesses strong aromaticity and high HOF (107.5 kcal mol−1),22 have not yielded fruitful results. In 1903, Hantzsch et al. tried to prepare arylpentazole (PhN5, A) but they failed.23 Until 1956, PhN5 was synthesized at low temperature by Huisgen and Ugi.24 4-Hydroxyphenylpentazole (A11, Fig. 1) was synthesized through cycloaddition reaction in 2002 by Benin et al.25 Although this reaction is very fast, many by-products appear. 4-Dimethylaminophenylpentazole (A14) and anisylpentazole (A12) were produced in 2003 and 2008, respectively.26,27 In addition, Frison et al. proposed that syntheses of some mono- and di-oxidized pentazole derivatives seem to be realistic.28 Although some other pentazole derivatives have also been studied,29–33 the development of pentazole derivatives is much slower in comparison with that of triazole and tetrazole derivatives. This is mainly because the N5 ring easily decomposes.25–27 In recent years, several photochemistry experimental investigations reveal that the N5 rings of arylpentazole derivatives such as p-(dimethylamino)phenyl pentazole (DMAP) and p-oxidophenylpentazole easily decompose into N2 and the corresponding phenyl azides.34–36 Hence, the low stability of the N5 ring should be the crucial factor in preventing the development of the pentazole derivatives.


image file: c4ra10669e-f1.tif
Fig. 1 Structures of the title compounds.

In addition, the central C–N bond connecting the aryl and the pentazole may break. This is supported by the experiments of Östmark et al.26 and Vij et al.37 which have detected N5 in gas phase from high-energy mass spectrometric degradation of arylpentazoles. So, which can take place more easily and is the initial step of pyrolysis of arylpentazoles, breaking of the central C–N bond or the N5 ring? Furthermore, we find that the synthesized PhN5 compounds are mainly the substituted derivatives with –OH, –OCH3 and –N(CH3)2, which seems to show that the electron donating groups may stabilize PhN5. If this is the case, why can they stabilize PhN5 and what's the difference in effects of different substituents? In view of the facts that the synthesized PhN5 derivatives are limited and have low stabilities, above questions can not be answered by experiment at present. Fortunately, with the rapid development of computer technology, structures and properties of nitrogen-rich compounds can be accurately predicted.27–29,38–47 In this paper, the stabilities and pyrolysis mechanisms of PhN5 and its derivatives were theoretically studied, and the effects of different substituents (–OH, –OCH3, –OC2H5 and –N(CH3)2) on the stability of PhN5 were investigated to answer the above questions. The structures of the title molecules are plotted in Fig. 1.

2. Computational details

Geometry optimizations of A and its derivatives were carried out using the restricted Kohn–Sham formalism at the RB3LYP/6-31G* and RM06-2X/6-311G** levels. The optimized structures were confirmed to be local minima without imaginary frequencies.

The relaxed potential energy surface scans along the stretching of the C–N bond and the N–N bonds were carried out at the RB3LYP/6-31G* level for searching transition states (TSs). Then, the structures of the discovered TSs were optimized at the RM06-2X/6-311G** level, which is reliable for computation of transition state.48–51 The optimized TSs were confirmed by only one imaginary frequency.

The optimized structures of A, its derivatives and TSs are shown in Fig. S1. After optimization, the pentazole and benzene rings in A and its derivatives are coplanar. The HN5 and benzyne (C6H4) and its derivatives (C6H3R) in the optimized structures of TS1 are coplanar, too. The N2, azide group and the benzene ring are not coplanar in the optimized conformations of TS2.

The methyl groups in A12, A16, and A22 are all coplanar with the benzene ring. One methyl group in A32 is coplanar with the benzene ring. All ethyl groups in A13, A17, A23, A26 and A36 are coplanar with the benzene ring. One of 2–3 ethyl groups in A33 and A35 is coplanar with the benzene ring. No ethyl group in A25 is coplanar with the benzene ring.

The OH group in all molecules is coplanar with the benzene ring. The N(CH3)2 groups in A14, A18 and A24 are essentially coplanar with the benzene ring, while in A26 and A36 are almost perpendicular to the benzene ring.

One and two hydrogen bonds are found in A25 and A36, respectively. The hydrogen bond energies are 13.6 kJ mol−1 for A25 and 41.0 kJ mol−1 for A36, respectively. There is no hydrogen bond in A31. The conformations of A25 and A36 with hydrogen bond paths are shown in Fig. S2.

Geometry optimizations of the radicals produced in breaking of the central C–N bond were carried out at the UM06-2X/6-311G** level. All geometry optimizations and relaxed potential energy surface scans were computed with the Gaussian program package.52

The bond dissociation energy (BDE), the energy difference between the parent molecule and the corresponding radical products in the unimolecular bond dissociation,53–56 was calculated using the following equation:

 
BDE = ER1˙ + ER2˙E (1)
where E represents the zero-point-corrected total energy of A and its derivatives obtained at the RM06-2X/6-311G** level, ER1˙ and ER2˙ stand for the zero-point-corrected total energies of two radicals obtained at the UM06-2X/6-311G** level. In this paper, only BDE for breaking of the central C–N bond was computed.

The activation energy (Ea) was obtained by eqn (2):

 
Ea = ETSER (2)
ETS and ER respectively represent the total energies of TS and reactant obtained at the RM06-2X/6-311G** level.

The density of electron at the bond critical point of the central C–N bond (ρBCP) was analyzed using the Multiwfn57 program. The wavefunction files (.wfn) obtained from the Gaussian package were used as inputs for Multiwfn to perform these quantum theory of atoms in molecules (QTAIM)58 analyses.

3. Results and discussion

3.1 Stability of the central C–N bond

Density of electron at the bond critical point (ρBCP) is tightly related to the bond strength, the increase in ρBCP is usually consistent with the increment in the bond strength. ρBCP of the central C–N bond connecting the benzene and pentazole rings and the differences in ρBCPρBCPs) between derivatives and A are tabulated in Table 1. The positive ΔρBCPs of A11–A14 suggest that the para-substitution strengthens the C–N bond. While the negative ΔρBCPs of A12′–A14′ and A22–A24 reflect that the meta-substitution weakens the C–N bond. ΔρBCPs of A25–A26, A31–A32 and A35 are positive, which suggests that the effects on the C–N bond strengths caused by the para-substitution are stronger than by the meta-substitution.
Table 1 Predicted ρBCP and ΔρBCP of C–N bonda
    n = 1 n = 2 n = 3 n = 4 n = 5 n = 6
a ρBCP of A is 0.269916 a.u.
A1n ρBCP (a.u.) 0.270719 0.270477 0.270352 0.270585    
ΔρBCP (a.u.) 0.000803 0.000561 0.000436 0.000669    
A1n′ ρBCP (a.u.) 0.270285 0.269348 0.269190 0.267478    
ΔρBCP (a.u.) 0.000369 −0.000570 −0.000730 −0.002440    
A2n ρBCP (a.u.) 0.270546 0.269066 0.268735 0.265553 0.270899 0.270333
ΔρBCP (a.u.) 0.000630 −0.000850 −0.001180 −0.004360 0.000983 0.000417
A3n ρBCP (a.u.) 0.271165 0.270117 0.269728 0.269123 0.270474 0.269290
ΔρBCP (a.u.) 0.001249 0.000201 −0.000190 −0.000790 0.000558 −0.000630


Experimental researches show that N5 can be detected in gas phase from high-energy mass spectrometric degradation of arylpentazoles.26,37 This means that the C–N linkage connecting the aryl and pentazole breaks. Cleavages of the C–N bonds of A and its derivatives were simulated using a relaxed potential energy surface scan for studying the thermal and kinetic stabilities of this bond. The simulated energy variation with breaking of the C–N bond of A is shown in Fig. 2 (left). Since the energy variation curves of derivatives are similar, only that of A21 is presented in Fig. 2 (right).


image file: c4ra10669e-f2.tif
Fig. 2 Variation of energy with the length of C–N bond of A (left) and A21 (right).

The energy of A increases with the elongation of the C–N bond, and the slope of the curve decreases gradually. The energy will finally reach a constant and no TS exists in this decomposition process. The products are two radicals, i.e., pentazole radical (N5˙) and benzene radical (Ph˙) (cf. Fig. 3). The energy of A21 increases first and then decreases, finally reaches a constant. The maximum point indicates that a TS exists in this decomposition process due to the H transfer and structural rearrangement. In fact, we found that the C–N bond of A may also break via a TS to produce molecules, not radicals, and that of A21 may also break without through a TS to produce radicals rather than molecules. So there are two possible pyrolysis processes of the central C–N bond: (1) C–N bond breaks without a TS and finally produces two radicals. The energy (BDE) needed for this path is the energy difference between two radicals and parent molecule; (2) C–N bond breaks through a TS and produces two ground state molecules (HN5 and benzyne (C6H4) derivatives). The minimum energy required for this path is the activation energy (Ea,1), i.e., the energy difference between the total energies of TS and reactant. In order to figure out the more preferred breaking process of the C–N bond, two pyrolysis paths of all derivatives were studied. Taking A as example, these two paths are shown in Fig. 3. The calculated BDE and Ea,1 are listed in Table 2.


image file: c4ra10669e-f3.tif
Fig. 3 Two possible pyrolysis paths of the C–N bond of A.
Table 2 Predicted BDE and Ea,1 at the M06-2X/6-311G** levela
    n = 1 n = 2 n = 3 n = 4 n = 5 n = 6
a BDE and Ea,1 of A are 534.9 and 375.6 kJ mol−1, respectively.
A1n BDE (kJ mol−1) 540.4 541.2 541.9 548.2    
Ea,1 (kJ mol−1) 391.8 396.9 397.1 401.8    
A1n′ BDE (kJ mol−1) 534.0 535.6 536.1 539.5    
Ea,1 (kJ mol−1) 362.5 367.1 367.9 373.9    
A2n BDE (kJ mol−1) 533.7 536.5 537.3 543.9 538.1 535.8
Ea,1 (kJ mol−1) 371.8 373.7 374.8 382.2 367.2 367.4
A3n BDE (kJ mol−1) 537.6 536.6 540.8 544.9 538.2 537.7
Ea,1 (kJ mol−1) 371.2 369.6 374.2 382.4 355.8 370.7


For path 1, BDEs are all higher than 533 kJ mol−1. In view of these large values, pyrolysis through path 1 should be difficult. Compared with the corresponding BDEs, Ea,1s are lower by 144–172 kJ mol−1. Therefore, path 2 is easier to proceed than path 1, which means that breaking of the C–N bond is more likely to follow the path 2 rather than 1, with the products of HN5 and derivatives of C6H4. In addition, the acidity of HN5 was estimated to be stronger than that of HNO3.59 This explains why N5 appears in the gaseous state of PhN5.26,37

Ea,1s have the order of A11 < A12 < A13 < A14, A11′ < A12′ < A13′ < A14′, A21 < A22 < A23 < A24, and A32 < A31 < A33 < A34. Ea,1 of A32 is smaller than that of A31, which may be because the steric repulsion is stronger in the former than in the latter. Generally speaking, the C–N bonds of the molecules with –N(CH3)2 are most stable, and those of the molecules with –OCH3 and –OC2H5 have comparable stabilities. This conclusion is in accordance with the variation trends of BDEs.

Ea,1s of A11–A14 are larger than that of A, i.e., C–N bonds of A11–A14 are stronger than that of A, which is consistent with the fact that ρBCPs of A11–A14 are larger than that of A. Ea,1s of A11′–A14′ are smaller than that of A. These suggest that the para-substituents improve the thermal stability of the C–N bond, while the meta-substituents decrease the stability. Ea,1s of A31–A34 are close to the corresponding ones of A21–A24 while smaller than those of A11–A14, because steric repulsions are stronger in A21–A24 and A31–A34 than in A11–A14. The lower symmetries and stronger repulsion interactions of A25 and A26 result in the fact that Ea,1s of them are lower than that of A21–A24.

Ea,1 or the stability of the C–N bond, is affected by the different substituents and substitution positions which lead to different symmetries and steric repulsions. BDE and Ea,1 obtained at the B3LYP/6-31G* level (in Table S1) lead to similar conclusions.

3.2 Stability of the pentazole ring

According to experimental investigations,25–27,34–36,60 A and its derivatives easily decompose into N2 and azido compounds. This suggests that breaking of the N–N bonds of the N5 ring may take place. Hence, a relaxed potential energy surface scan along stretching of two N–N bonds (labelled as SC1 and SC2) was carried out to simulate the decomposition of the pentazole ring. The simulated energy surface of A24 is plotted in Fig. 4. After geometry optimizations of possible TS structures, one TS was found and shown in Fig. 4, too.
image file: c4ra10669e-f4.tif
Fig. 4 Potential energy surface with breaking of N–N bonds of A24.

Fig. 5 shows the TSs and products of decompositions of the N5 ring of A and A11. For other molecules, the processes are similar. In the pyrolysis processes, TSs appear when SC1 and SC2 elongate respectively to about 1.70 and 1.75 Å, N2 and azido benzene derivatives finally emerge as products. Conversion of the reactant into TS is the key step in decomposition of the N5 ring, the activation energy (Ea,2) of this step is listed in Table 3.


image file: c4ra10669e-f5.tif
Fig. 5 Decompositions of the N5 ring of A and A11.
Table 3 Predicted Ea,2s and Qts of all derivatives at the M06-2X/6-311G** levela
    n = 1 n = 2 n = 3 n = 4 n = 5 n = 6
a Ea,2 and Qt of A is 112.6 kJ mol−1 and −0.471e, respectively.
A1n Ea,2 (kJ mol−1) 114.5 114.9 114.9 116.7    
Qt (e) −0.486 −0.487 −0.489 −0.506    
A1n′ Ea,2 (kJ mol−1) 111.6 113.9 114.0 115.2    
Qt (e) −0.471 −0.475 −0.476 −0.479    
A2n Ea,2 (kJ mol−1) 111.6 114.2 114.4 116.8 113.7 109.2
Qt (e) −0.475 −0.479 −0.482 −0.484 −0.486 −0.484
A3n Ea,2 (kJ mol−1) 114.2 114.0 113.4 117.4 114.9 113.4
Qt (e) −0.484 −0.484 −0.488 −0.493 −0.493 −0.483


Ea,2s required for breaking the N5 rings of A and its derivatives are 109–118 kJ mol−1, which are far smaller than Ea,1s for breaking the C–N bonds through path 2 (>355 kJ mol−1). Obviously, decomposition of the N5 ring is much easier than breaking of the C–N bond, so decomposition of the N5 ring may be the initial step of pyrolysis of these molecules. This conclusion is consistent with the experimental results.25,27,34–36

Ea,2s of derivatives are generally larger than that of A. Although the increases in Ea,2 caused by introduction of electron donating groups are not significant, these groups generally do improve the stability of the pentazole. The total charges (Qts) of five N atoms in the N5 ring were calculated and are listed in Table 3, too. Qts of all molecules but A11′ are more negative than that of A, that is, these substituents increase the electron density of N5 in A which may strengthen the delocalization of the N5 ring and stabilize this ring. Inspections of Ea,2s and Qts of A11–A14, A11′–A14′ and A21–A24 reveal that the increments in stability and electron density of the N5 ring caused by these substituents generally have the order of –N(CH3)2 > –OC2H5 > –OCH3 > –OH. This reveals that the abilities of these functional groups to improve the stability of A have the order of –N(CH3)2 > –OC2H5 > –OCH3 > –OH. Qts of A31 and A32 are the same, Ea,2 of the former is larger than that of the latter, which is benefit from the weaker steric repulsion of the former in comparison with the latter. Ea,2s and the absolute values of Qts of A11′–A14′ are smaller than the corresponding ones of A11–A14, so the pentazoles of the para-substituted molecules are more stable than those of the meta-substituted molecules. Ea,2s and Qts calculated at the B3LYP/6-31G* level (Table S2) lead to similar conclusions.

3.3 Chemical stability

Table 4 summarizes the highest occupied molecular orbital energy (EHOMO), the lowest unoccupied molecular orbital energy (ELUMO) and the energy gap (Eg) between the frontier orbitals. Variation trends of them are plotted in Fig. 6. This figure shows that the variation trends of EHOMO and ELUMO are the same, which are completely contrary to that of Eg. EHOMOs and ELUMOs of all derivatives are higher than that of A, while increases in ELUMOs are smaller than that in EHOMOs. Therefore, Egs of derivatives are smaller than that of A, i.e., these electron donating substituents lower the chemical stability of PhN5.
Table 4 Predicted EHOMO, ELUMO and Eg at the M06-2X/6-311G** levela
    n = 1 n = 2 n = 3 n = 4 n = 5 n = 6
a EHOMO, ELUMO and Eg of A are −8.91, −1.11 and 7.80 eV, respectively.
A1n EHOMO (eV) −8.24 −8.10 −8.07 −7.09    
ELUMO (eV) −0.89 −0.84 −0.82 −0.55    
Eg (eV) 7.35 7.26 7.25 6.54    
A1n′ EHOMO (eV) −8.42 −8.24 −8.20 −7.20    
ELUMO (eV) −1.09 −1.08 −1.06 −0.83    
Eg (eV) 7.33 7.16 7.15 6.37    
A2n EHOMO (eV) −8.28 −8.19 −8.13 −6.79 −7.98 −7.86
ELUMO (eV) −1.10 −1.05 −1.00 −0.58 −0.97 −0.99
Eg (eV) 7.17 7.13 7.12 6.21 7.01 6.87
A3n EHOMO (eV) −7.92 −8.09 −7.91 −6.78 −7.21 −8.03
ELUMO (eV) −0.92 −0.99 −0.84 −0.69 −0.83 −0.94
Eg (eV) 7.00 7.10 7.07 6.09 6.38 7.09



image file: c4ra10669e-f6.tif
Fig. 6 Variations of EHOMOs, ELUMOs and Egs of title compounds.

Egs of A11–A14 are larger than the corresponding ones of A11′–A14′, i.e., the para-substituted molecule is more stable than the meta-substituted molecule in chemical process with electron transfer. Inspections of the variations of Egs of A11–A14, A11′–A14′ and A21–A24 show that Egs of derivatives with different substituents have the order of –OH > –OCH3 > –OC2H5 > –N(CH3)2. Effects on the chemical stability caused by these substituents are completely contrary to that on the thermal stability, i.e., the substituent that leads to the greater increment in thermal stability causes the larger decrease in the chemical stability. The Egs of the derivatives with –OCH3 and –OC2H5 are very close, which is similar to their comparable thermal stabilities. Comparisons of Egs of A11–A14, A21–A24 and A31–A34 reveal that the chemical stability decreases with the increasing number of substituents. Egs in Table S3 obtained at the B3LYP/6-31G* level have the same variation trends to those obtained at the M06-2X/6-311G** level.

4. Conclusion

Decomposition of the N5 ring (Ea,2 = 109–117 kJ mol−1) is much easier than breaking of the central C–N bond (Ea,1 = 362–402 kJ mol−1), and should be the initial step of pyrolysis of PhN5 and its derivatives with the products of N2 and azido benzene derivatives. Substituents somewhat improve the thermal stability of the N5 ring by increasing the electron density of the N5 ring with the order of –N(CH3)2 > –OC2H5 > –OCH3 > –OH. The para-substitution is more helpful for improving the thermal stability than the meta-substitution. Higher symmetry and weaker steric interactions are also helpful for improving thermal stability. Substituents lower the chemical stability of PhN5 with the order of –OH > –OCH3 > –OC2H5 > –N(CH3)2.

Acknowledgements

Thanks to the 086 Project for supporting this research.

References

  1. C. W. Tornøe, C. Christensen and M. Meldal, J. Org. Chem., 2002, 67, 3057–3064 CrossRef.
  2. V. K. Aggarwal, J. de Vicente and R. V. Bonnert, J. Org. Chem., 2003, 68, 5381–5383 CrossRef CAS PubMed.
  3. V. Thottempudi and J. M. Shreeve, J. Am. Chem. Soc., 2011, 133, 19982–19992 CrossRef CAS PubMed.
  4. V. Thottempudi, H. Gao and J. M. Shreeve, J. Am. Chem. Soc., 2011, 133, 6464–6471 CrossRef CAS PubMed.
  5. Y. Guo, G. H. Tao, Z. Zeng, H. Gao, D. A. Parrish and J. M. Shreeve, Chem.–Eur. J., 2010, 16, 3753–3762 CrossRef CAS PubMed.
  6. H. Gao and J. M. Shreeve, Chem. Rev., 2011, 111, 7377–7436 CrossRef CAS PubMed.
  7. V. D. Ghule, R. Sarangapani, P. M. Jadhav and S. P. Tewari, J. Mol. Model., 2011, 17, 1507–1515 CrossRef CAS PubMed.
  8. T. M. Klapötke and C. M. Sabaté, Chem. Mater., 2008, 20, 3629–3637 CrossRef.
  9. J. Zhang, S. Pang, Y. Li, Y. Yu and H. Zhang, Energ. Mater., 2006, 14, 355–357 CAS.
  10. M. T. Nguyen, Coord. Chem. Rev., 2003, 244, 93–113 CrossRef CAS.
  11. R. Huisgen, Angew. Chem., Int. Ed. Engl., 1963, 2, 565–598 CrossRef.
  12. Y. Wu, J. Deng, Y. Li and Q. Chen, Synthesis, 2005, 1314–1318 CrossRef CAS.
  13. F. Fazio, M. C. Bryan, O. Blixt, J. C. Paulson and C. H. Wong, J. Am. Chem. Soc., 2002, 124, 14397–14402 CrossRef CAS PubMed.
  14. T. L. Mindt and R. Schibli, J. Org. Chem., 2007, 72, 10247–10250 CrossRef CAS PubMed.
  15. S. J. Wittenberger, Org. Prep. Proced. Int., 1994, 26, 499–531 CrossRef CAS.
  16. S. J. Wittenberger and B. G. Donner, J. Org. Chem., 1993, 58, 4139–4141 CrossRef CAS.
  17. D. P. Curran, S. Hadida and S. Y. Kim, Tetrahedron, 1999, 55, 8997–9006 CrossRef CAS.
  18. Z. P. Demko and K. B. Sharpless, J. Org. Chem., 2001, 66, 7945–7950 CrossRef CAS PubMed.
  19. C. M. Athanassopoulos, T. Garnelis, D. Vahliotis and D. Papaioannou, Org. Lett., 2005, 7, 561–564 CrossRef CAS PubMed.
  20. Z. P. Demko and K. B. Sharpless, Angew. Chem., Int. Ed., 2002, 41, 2110–2113 CrossRef CAS.
  21. S. Hajra, D. Sinha and M. Bhowmick, J. Org. Chem., 2007, 72, 1852–1855 CrossRef CAS PubMed.
  22. P. A. Denis, Theor. Chem. Acc., 2011, 129, 219–227 CrossRef CAS.
  23. A. Hantzsch, Ber. Dtsch. Chem. Ges., 1903, 36, 2056–2058 CrossRef CAS.
  24. I. Ugi, R. Huisgen, K. Clusius and M. Vecchi, Angew. Chem., 1956, 68, 753–754 CrossRef CAS.
  25. V. Benin, P. Kaszynski and G. Radziszewski, J. Org. Chem., 2002, 67, 1354–1358 CrossRef CAS PubMed.
  26. H. Östmark, S. Wallin, T. Brinck, P. Carlqvist, R. Claridge, E. Hedlund and L. Yudina, Chem. Phys. Lett., 2003, 379, 539–546 CrossRef.
  27. R. N. Butler, J. M. Hanniffy, J. C. Stephens and L. A. Burke, J. Org. Chem., 2008, 73, 1354–1364 CrossRef CAS PubMed.
  28. G. Frison, G. Jacob and G. Ohanessian, New J. Chem., 2013, 37, 611–618 RSC.
  29. P. K. Swain, J. Mol. Liq., 2010, 157, 1–5 CrossRef CAS.
  30. X. F. Chen, J. H. Bu, T. Yu, W. P. Lai and Z. X. Ge, Communications in Computational Chemistry, 2013, 1, 118–123 Search PubMed.
  31. M. Xu, Q. Pan, Z. Q. Chen, G. Zhang, Y. L. Ning, M. C. Wang, M. Wang and F. Q. Bi, Chin. J. Explos. Propellants, 2013, 1, 005 Search PubMed.
  32. M. Xu, F. Q. Bi, G. Zhang, M. C. Wang, Z. X. Ge, Z. Q. Chen and C. Xu, Chin. J. Energ. Mater., 2012, 5, 031 Search PubMed.
  33. F. Q. Bi, C. Xu, X. Z. Fan, Z. X. Ge, B. Z. Wang, M. C. Wang, Q. Liu and M. Xu, Chin. J. Explos. Propellants, 2012, 2, 002 Search PubMed.
  34. U. Geiger, A. Elyashiv, R. Fraenkel, S. Zilberg and Y. Haas, Chem. Phys. Lett., 2013, 556, 127–131 CrossRef CAS.
  35. P. Portius, M. Davis, R. Campbell, F. Hartl, Q. Zeng, A. J. Meijer and M. Towrie, J. Phys. Chem. A, 2013, 117, 12759–12769 CrossRef CAS PubMed.
  36. U. Geiger, Y. Haas and D. Grinstein, J. Photochem. Photobiol., A, 2014, 277, 53–61 CrossRef CAS.
  37. A. Vij, J. G. Pavlovich, W. W. Wilson, V. Vij and K. O. Christe, Angew. Chem., 2002, 114, 3177–3180 CrossRef.
  38. L. Y. Bruney, T. M. Bledson and D. L. Strout, Inorg. Chem., 2003, 42, 8117–8120 CrossRef CAS PubMed.
  39. L. Cheng, Q. Li, W. Xu and S. Zhang, J. Mol. Model., 2003, 9, 99–107 CrossRef CAS PubMed.
  40. T. K. Ha, O. Suleimenov and M. T. Nguyen, Chem. Phys. Lett., 1999, 315, 327–334 CrossRef CAS.
  41. H. Wu, X. Xu and H. Jiao, Chem. Phys. Lett., 2005, 412, 299–302 CrossRef CAS.
  42. M. Lein, J. Frunzke, A. Timoshkin and G. Frenking, Chem.–Eur. J., 2001, 7, 4155–4163 CrossRef CAS.
  43. D. L. Strout, J. Phys. Chem. A, 2005, 109, 1478–1480 CrossRef CAS PubMed.
  44. M. Rahm and T. Brinck, Chem.–Eur. J., 2010, 16, 6590–6600 CrossRef CAS PubMed.
  45. I. Alkorta, F. Blanco and J. Elguero, J. Phys. Chem. A, 2008, 112, 1817–1822 CrossRef CAS PubMed.
  46. P. G. Seybold and W. Kreye, Int. J. Quantum Chem., 2012, 112, 3769–3776 CrossRef CAS.
  47. Y. C. Li and S. P. Pang, Chin. J. Explos. Propellants, 2012, 35, 1–8 Search PubMed.
  48. L. Simón and J. M. Goodman, Org. Biomol. Chem., 2011, 9, 689–700 Search PubMed.
  49. Q. Wu, W. Zhu and H. Xiao, J. Mater. Chem. A, 2014, 2, 13006–13015 CAS.
  50. T. Yu, J. Zheng and D. G. Truhlar, Chem. Sci., 2011, 2, 2199–2213 RSC.
  51. S. Franzen, B. Skalski, L. Bartolotti and B. Delley, Phys. Chem. Chem. Phys., 2014, 16, 20164–20174 RSC.
  52. Gaussian 03, Revision C.02, ed. M. J. Frisch, G. W. Trucks, H. B. Schlegel, G. E. Scuseria, M. A. Robb, J. R. Cheeseman, J. A. Montgomery, 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, Inc., Wallingford CT, 2004 Search PubMed.
  53. S. W. Benson, Thermochemical kinetics: methods for the estimation of thermochemical data and rate parameters, Wiley, New York, 1976 Search PubMed.
  54. X. Q. Yao, X. J. Hou, G. S. Wu, Y. Y. Xu, H. W. Xiang, H. Jiao and Y. W. Li, J. Phys. Chem. A, 2002, 106, 7184–7189 CrossRef CAS.
  55. J. Shao, X. Cheng and X. Yang, J. Mol. Struct.: THEOCHEM, 2005, 755, 127–130 CrossRef CAS.
  56. X. W. Fan, X. H. Ju, Q. Y. Xia and H. M. Xiao, J. Hazard. Mater., 2008, 151, 255–260 CrossRef CAS PubMed.
  57. T. Lu and F. Chen, J. Comput. Chem., 2012, 33, 580–592 CrossRef CAS PubMed.
  58. R. F. Bader, Chem. Rev., 1991, 91, 893–928 CrossRef CAS.
  59. C. Chen, Int. J. Quantum Chem., 2000, 80, 27–37 CrossRef CAS.
  60. S. Kamijo, T. Jin, Z. Huo, Y. S. Gyoung, J. G. Shim and Y. Yamamoto, Mol. Diversity, 2003, 6, 181–192 CrossRef CAS PubMed.

Footnote

Electronic supplementary information (ESI) available. See DOI: 10.1039/c4ra10669e

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