Are the Nitro- and Amino-substituted Piperidine High-energy-density Compounds?

Bu-Tong LI Lu-Lin LI Quan-Bao ZHOU

Citation:  Bu-Tong LI, Lu-Lin LI, Quan-Bao ZHOU. Are the Nitro- and Amino-substituted Piperidine High-energy-density Compounds?[J]. Chinese Journal of Structural Chemistry, 2020, 39(7): 1266-1270. doi: 10.14102/j.cnki.0254–5861.2011–2619 shu

Are the Nitro- and Amino-substituted Piperidine High-energy-density Compounds?

English

  • High-energy-density materials (HEDM) are applied extensively in industry and military, so the development of new high-energy-density materials is an important aspect in materials science[1-5]. In general, good high-energy-density materials have some special chemical and physical characters including good oxygen balance, good thermal stability, high-energy-density, and low sensitivity[6-8]. Nowadays, high-energy-density materials with low sensitivity to compact and friction are focus of research to scientists. However, high-energy-density is usually contradictory with low sensitivity and the balance between them is difficult to achieve.

    In 1888 and 1998, famous 1, 3, 5-triamino-2, 4, 6-trinitrobenzen (TATB) and 1, 1-diamino-2, 2-dinitroethylene (FOX-7) were synthesized[9, 10], respectively. Recently, the calculations about the aminonitrocyclopropanes have shown their heats of formation close to zero and the densities close to 2 g∙cm-3, which is regarded as a typical feature of the next-generation explosive[11]. The low heat of formation indicates good insensitivity, and the high density is usually accompanied with an excellent detonation characters. More instances can also be found elsewhere[12, 13]. Therefore, the planar structure is not always necessary and introducing both the amino and nitro groups into a molecule may be an effective way to achieve the balance between the detonation characters and the molecular sensitivity.

    Inspired by the former works, the piperidine was chosen as the parent body and nitro and amino groups were introduced into it to design new high-energy-density derivatives. The regulation between stabilities and sensitivities can be achieved through adjusting the positions of nitro groups and amino groups. Thermal stabilities and detonation characters are calculated systematically and our work will be helpful for further exploration of the title molecules.

    All of the optimizations are carried out at the B3PW91/6-311+G(d, p) level by using the G03 software package on a computer cluster[14]. Frequency analyses are performed at the same level, and the stationary points on the potential energy surface are confirmed. All optimized structures are listed in Fig. 1 and labeled as α, β1, β2, β3, γ, and δ.

    Figure 1

    Figure 1.  Optimized geometries of nitro- and amino-substituted piperidine molecules at the B3PW91/6–311+G(d, p) level

    The heats of formation are calculated based on the isodesmic reaction as follows[15]:

    $ \begin{array}{l} {{\rm{C}}_4}{{\rm{H}}_{10 - 2n}}{({\rm{N}}{{\rm{H}}_2})_n}{({\rm{N}}{{\rm{O}}_2})_n} + 2n{\rm{C}}{{\rm{H}}_4} \to {{\rm{C}}_4}{{\rm{H}}_{10}} + \\ n{\rm{C}}{{\rm{H}}_3}{\rm{N}}{{\rm{H}}_2} + n{\rm{C}}{{\rm{H}}_3}{\rm{N}}{{\rm{O}}_2}(n = 1 \sim 5) \end{array} $

    (1)

    The reaction enthalpy can be obtained from the following formula:

    $ {\Delta _r}{H_{{\text{298K}}}} = \sum {\Delta _f}{H_{{\text{298K}}}}(P) - \sum {\Delta _f}{H_{{\text{298K}}}}(R) $

    (2)

    in which ${\Delta _f}{H_{{\text{298K}}}}(R)$ and ${\Delta _f}{H_{{\text{298K}}}}(P)$ are the heats of formation of reagent and product, respectively. ΔH298 can be calculated with the following formula:

    $ {\Delta _r}{H_{{\text{298K}}}} = \Delta {E_0} + \Delta ZPE + \Delta {H_{\text{T}}} + \Delta nRT $

    (3)

    Since the heats of formation can be obtained from NIST WebBook for reference molecules, the heats of formation can be estimated for the title molecules.

    The detonation velocities and detonation pressures are calculated by using the Kamlet-Jacobs equation as follows[16]:

    $ D = (1.011 + 1.312\rho ){(N{\overline M ^{{1 \mathord{\left/ {\vphantom {1 2}} \right. } 2}}}{Q^{{1 \mathord{\left/ {\vphantom {1 2}} \right. } 2}}})^{{1 \mathord{\left/ {\vphantom {1 2}} \right. } 2}}} $

    (4)

    $ P = 1.558{\rho ^2}N{\overline M ^{{1 \mathord{\left/ {\vphantom {1 2}} \right. } 2}}}{Q^{{1 \mathord{\left/ {\vphantom {1 2}} \right. } 2}}} $

    (5)

    The bond dissociation energies are estimated through homolytic reactions:

    $ A - B \to A \bullet + B \bullet $

    (6)

    $ BD{E_{{\text{(A - B)}}}} = \left[ {{E_{\text{A}}} + {E_{\text{B}}}} \right] - {E_{{\text{(A - B)}}}} $

    (7)

    The zero point energy corrections are also considered as below:

    $ BD{E_{({\rm{A}}-{\rm{B}})}}_{{\rm{ZPE}}} = {\rm{ }}[{E_{{\rm{A}} \bullet }} + {E_{{\rm{B}} \bullet }}]-{E_{\left( {{\rm{A}} - {\rm{B}}} \right)}} + \Delta ZPE$

    (8)

    The characteristic heights are calculated from the equation[17]:

    $ {H_{50}} = 0.1926 + 98.64Q_{_{NO2}}^2 - 0.03405O{B_{100}} $

    (9)

    in which QNO2 is the net charge on nitro group and $ O{B_{100}} $ is the oxygen balance value. QNO2 in equation 9 can be deduced by equation 10 as follows:

    $ {Q_{{\text{NO2}}}} = {Q_{\text{N}}} + {Q_{{\text{O1}}}} + {Q_{{\text{O2}}}} $

    (10)

    QN, QO1, and QO2 are the net charges on N, O1 and O2 atoms, respectively. OB100 can be calculated by using Eq. (11):

    $ O{B_{100}} = 100(2{N_{\rm{O}}}{\rm{ - }}{N_{\rm{H}}}{\rm{ - }}2{N_{\rm{C}}}{\rm{ - }}2{N_{{\rm{COO}}}})/M $

    (11)

    NO, NH, NC, and NCOO represent the number of -O, -H, -C, and -COO, respectively. M is a molecular weight.

    Heat of formation is an important index of thermal chemistry for high-energy-density molecule. It is related to the detonation characters and can be used to predict the energy-content for target molecule. So the heats of formation of the title molecules are calculated and listed in Table 1 accompanied with the reference data.

    Table 1

    Table 1.  Total Energies (E0, a.u.), Zero Point Energies (ZPE, a.u.), Thermal Correction Energies (HT, a.u.) and Heats of Formation (HOF, kJ/mol) Calculated at the B3PW91/6-311+G(d, p) Level
    DownLoad: CSV
    Compound ZPE E H HT HOF
    α 0.16726 −527.58733 −527.57720 0.17738 −9.60
    β1 0.18609 −787.41406 −787.39980 0.20035 −50.41
    β2 0.18610 −787.41221 −787.39798 0.20033 −45.63
    β3 0.18655 −787.39957 −787.38586 0.20026 −13.80
    γ 0.20495 −1047.2224 −1047.2045 0.22282 −44.31
    δ 0.22469 −1307.0294 −1307.0083 0.24575 −35.83

    From Table 1, it is found that all molecules have negative heats of formation, but the values are close to zero. Although positive heats of formation have been found for many high energy density compounds, it must be mentioned that the negative heats of formation are not contradictory to the high energy density. For example, famous insensitive explosive 3-nitro-l, 2, 4-triazol-5-one (NTO) and 2, 2-dinitro-ethene-1, 1-diamine (DADE) have the heats of formation of −33.4[18], −30.9[10] and −32.0 kJ/mol[19], respectively. Therefore, our results are reasonable and the outstanding stability is evaluated for the title molecules.

    The linear regression is performed between the heats of formation and the substituent number. However, no evident linear equation was confirmed for the low R2 value and the groups additivity rule is confirmed not responsible for the title molecules. In general, the heats of formation rise with the introduction of nitro groups, but the situation is different here. In order to find out the reason, the molecular structures were checked carefully. It is found that more hydrogen bonds are formed when more nitro groups are introduced because of the twisted structure, which causes the instability from the introduction of nitro groups to be counteracted.

    In summary, the derivatives designed by us showed unusual stability for their negative heats of formation, especially as high energy density compounds. This also suggests the excellent insensitivity can be expected for title molecules.

    The kinetic stability is important to estimate the potential application as high-energy-density material and the bond dissociation energies have been proved to be good parameter for this purpose[20]. Therefore, the dissociation energies of the title molecules were calculated and listed in Table 2.

    Table 2

    Table 2.  Bond Dissociation Energy (BDE, kJ/mol), Zero Point Energy (ZPE, a.u.), Electronic Energy (E, a.u.) and the Bond Orders Calculated at the B3PW91/6–311+G(d, p) Level
    DownLoad: CSV
    Compound ZPE E BDE Bond order
    α 0.16725 −527.587 230.29 0.7143
    β1 0.18609 −787.414 234.80 0.6531
    β2 0.18609 −787.412 231.10 0.6763
    β3 0.18655 −787.4 207.01 0.7288
    γ 0.20495 −1047.22 227.99 0.6749
    δ 0.22468 −1307.03 197.22 0.7274
    RDX 145.62
    HMX 160.41

    In Table 2, all of the bond dissociation energies are quite large, even the least bond dissociation energy (197.22 kJ/mol) of δ is larger than 145.62 kJ/mol of RDX and 160.41 kJ/mol of HMX. This indicates excellent kinetic stability of the title molecules. All of the trigger bonds are C−N, which is consistent with the fact that C−N is the weakest bond compared to others. All of the bond orders are close to 1.0, and the single bond nature of C−N is confirmed. Furthermore, the correlation between the bond order and bond dissociation energy is performed, but no relationship is confirmed. For example, the bond dissociation energy (231.10 kJ/mol) of β2 is less than that (234.80 kJ/mol) of β1, but the bond order (0.6763) of β2 is greater than that (0.6531) of β1. In consideration of the undetectability of bond order in experiment, the bond dissociation energy is a more reliable parameter to predict the kinetic stability.

    In addition, the largest bond association energy is 230.29 kJ/mol of α, as well as the least is 197.22 kJ/mol of δ. The deviation is about 30 kJ/mol, which shows the bond dissociation energy is not affected by the introduction of nitro groups. The situation is different for the title molecules compared to other available data for which more energetic molecules have less stability.

    Detonation velocity and detonation pressure are two important parameters for high-energy-density molecules. Kamlet-Jacobs equation has been proved reliable to predict these two parameters so they were calculated in this paper by using the Kamlet-Jacobs equation and the final data are listed in Table 2. For comparison purpose, the corresponding data of RDX and HMX are also shown.

    From Table 2, the molecular densities are located from 1.8092 g/cm3 of δ to 1.3983 g/cm3 of α, and all density values of the derivatives are improved markedly compared to the parent molecule. It is also concluded that the detonation pressure and detonation velocity increased with the introduction of nitro groups. The linear regression was performed and the correlation equation is y = 1.1824x − 6.397 with the R² value of 0.9607 for the detonation velocity and y = 0.1589x − 1.3237 with the R² to be 0.988 for the detonation pressure. Obviously, the groups additivity rule is compatible for the detonation parameters of the title molecules. On considering the low heats of formation, the detonation characters are affected chiefly by the elemental composition rather than the heats of formation. Compared to HMX and RDX, δ shows better detonation velocity and detonation pressure. However, the explosive heat of δ is about 300 kJ/mol less than that of RDX, which indicates better insensitivity of δ than that of RDX, so the H50 values are calculated further.

    Table 3

    Table 3.  Molecular Density (ρ, g/cm3), Detonation Heats (Q, kJ/g), Detonation Velocity (D, km/s), Detonation Pressure (P, GPa) and Character Height (H50, cm) Calculated at the B3PW91/6-311+G(d, p) Level
    DownLoad: CSV
    Compound Q ρ D P H50
    α 996.45 1.3983 6.05 13.80 52
    β1 1115.28 1.5687 7.17 20.96 50
    β2 1120.81 1.5704 7.19 21.06 46
    β3 1157.71 1.5937 7.32 22.05 56
    γ 1222.64 1.7035 7.99 27.39 42
    δ 1292.24 1.8092 8.58 32.79 34
    RDX 1591.03 1.78(1.82) 8.87(8.75) 34.67(34.00) 26
    HMX 1633.90 1.88(1.91) 9.28(9.10) 39.19(39.00) 29

    Usually, drop hammer experiments were used to test impact sensitivities. In theory, equation 9 can be used for calculation. Based on our calculations, all derivatives of piperidine have H50 values from 34 cm of δ to 56 cm of β3. These values are all larger than 26 cm of RDX and 29 cm of HMX, and excellent insensitivity characters are indicated for the title molecules. On the consideration of both compact sensitivity and detonation characters, δ has better characters than RDX and can be regarded as the potential high energy density compounds.

    Based on our calculations, the negative heats of formation are obtained for the derivatives of piperidine, and the introduction of nitro- and amino-groups reduced molecular heats of formation accompanied with the molecular density increased. Among six designed molecules, δ has the largest detonation velocity and detonation pressure with the largest molecular density. In addition, large dissociation energies are confirmed, indicating the excellent thermal stability for all derivatives. Furthermore, all derivatives designed have better H50 values with RDX and HMX, which indicated their lower compact sensitivity. Overall consideration about the thermal stability and the detonation characters shows the molecule δ is screened out as a high-energy-density molecule for its better insensitivity and comparable detonation characters to RDX and HMX.


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  • Figure 1  Optimized geometries of nitro- and amino-substituted piperidine molecules at the B3PW91/6–311+G(d, p) level

    Table 1.  Total Energies (E0, a.u.), Zero Point Energies (ZPE, a.u.), Thermal Correction Energies (HT, a.u.) and Heats of Formation (HOF, kJ/mol) Calculated at the B3PW91/6-311+G(d, p) Level

    Compound ZPE E H HT HOF
    α 0.16726 −527.58733 −527.57720 0.17738 −9.60
    β1 0.18609 −787.41406 −787.39980 0.20035 −50.41
    β2 0.18610 −787.41221 −787.39798 0.20033 −45.63
    β3 0.18655 −787.39957 −787.38586 0.20026 −13.80
    γ 0.20495 −1047.2224 −1047.2045 0.22282 −44.31
    δ 0.22469 −1307.0294 −1307.0083 0.24575 −35.83
    下载: 导出CSV

    Table 2.  Bond Dissociation Energy (BDE, kJ/mol), Zero Point Energy (ZPE, a.u.), Electronic Energy (E, a.u.) and the Bond Orders Calculated at the B3PW91/6–311+G(d, p) Level

    Compound ZPE E BDE Bond order
    α 0.16725 −527.587 230.29 0.7143
    β1 0.18609 −787.414 234.80 0.6531
    β2 0.18609 −787.412 231.10 0.6763
    β3 0.18655 −787.4 207.01 0.7288
    γ 0.20495 −1047.22 227.99 0.6749
    δ 0.22468 −1307.03 197.22 0.7274
    RDX 145.62
    HMX 160.41
    下载: 导出CSV

    Table 3.  Molecular Density (ρ, g/cm3), Detonation Heats (Q, kJ/g), Detonation Velocity (D, km/s), Detonation Pressure (P, GPa) and Character Height (H50, cm) Calculated at the B3PW91/6-311+G(d, p) Level

    Compound Q ρ D P H50
    α 996.45 1.3983 6.05 13.80 52
    β1 1115.28 1.5687 7.17 20.96 50
    β2 1120.81 1.5704 7.19 21.06 46
    β3 1157.71 1.5937 7.32 22.05 56
    γ 1222.64 1.7035 7.99 27.39 42
    δ 1292.24 1.8092 8.58 32.79 34
    RDX 1591.03 1.78(1.82) 8.87(8.75) 34.67(34.00) 26
    HMX 1633.90 1.88(1.91) 9.28(9.10) 39.19(39.00) 29
    下载: 导出CSV
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  • 发布日期:  2020-07-01
  • 收稿日期:  2019-09-25
  • 接受日期:  2019-12-13
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