3.2. Frontier Molecular Orbitals
Frontier molecular orbitals, namely, the highest occupied molecular orbital (HOMO) and the lowest unoccupied molecular orbital (LUMO). The energy levels and symmetry of these orbitals play a crucial role in the reaction process, such as the positions of electrophilic and nucleophilic reactions, cycloaddition reactions, electrocyclic reactions, and so on.
Figure 3 shows the HOMO and LUMO of these high-energy-density nitrogen-rich energy storage molecular systems. Orbital energy level diagrams depict red areas as the positive phase and green areas as the negative. For molecule A1, its HOMO is mainly contributed by the whole molecular skeleton, while its LUMO is contributed by the tetrazole ring, indicating that the electronic excitation of A1 molecule mainly occurs from the HOMO of the whole molecule to the LUMO of the tetrazole ring. The HOMO of the B series molecules is mainly contributed by the whole molecular skeleton, while their LUMO is mainly contributed by all remaining parts except for the -NH
2 substituent and its connected tetrazole ring (such as molecules B1, B3, and B4), indicating that electronic excitation of the B series molecules mainly occurs from the HOMO of the whole molecule to the LUMO of the non-NH
2 substituent and its connected tetrazole ring. For C series molecules, the HOMO of all these molecules is mainly contributed by the whole molecular skeleton, while their LUMO is mainly contributed by all remaining parts except for the -N
3 and -ONO
2 substituents and the tetrazole ring they are connected to (such as molecules C3, B4, and C5), indicating that electronic excitation of C-series molecules mainly occurs from the HOMO of the whole molecule to the LUMO of the tetrazole ring and the LUMO of the nitro substituent. For D series molecules, their HOMO is mainly contributed by the whole molecular skeleton, while their LUMO is mainly contributed by all remaining parts except for the -ONO
2 substituent and the tetrazole ring they are connected with. This indicates that the electronic excitation of D series molecules mainly occurs from the HOMO of the whole molecule to the LUMO of the tetrazole ring and the LUMO of the nitro substituent. All or most of the HOMO and LUMO of these molecules involve molecular skeletons, indicating that these molecular skeletons are influenced by electron transference between their HOMO and LUMO.
The chemical reactivity of these energy storage molecules can be quantitatively assessed using the HOMO-LUMO energy gap (Δ
E).
Figure 4 displays the corresponding HOMO, LUMO, and Δ
E values. Typically, a larger Δ
E correlates with greater molecular stability, as it impedes electron transitions between these orbitals. The LUMO energy level position affects the ability of the molecule to accept electrons (electrophilicity). The LUMO energy levels of the D series molecules in the figure are significantly lower than those of other series molecules, indicating that they have the strongest electron accepting ability (strong electrophilicity), which is closely related to the strong electron withdrawing groups (nitro, nitrate ester groups) present in their structure. The LUMO of the A series molecules has the highest energy level and the weakest electrophilicity. The HOMO energy level reflects the ability of a molecule to provide electrons (nucleophilicity). From the figure, it can be seen that the HOMO energy levels of the C series molecules are relatively higher, indicating that they are more prone to losing electrons (with strong reducibility), which is related to the strong electron donating groups present in their structure. The relatively low HOMO energy levels in the D series molecules indicate a weak ability to provide electrons. As shown in
Figure 4b, there are significant differences in Δ
E values between different series molecules. The A series molecules have the largest Δ
E values, indicating that their electronic excitation requires higher energy, the molecular ground state stability is the highest, and the chemical reaction activity is relatively lower. The B and C series molecules have a centered Δ
E values and moderate stability. The D series molecules have the smallest Δ
E values and are most prone to electronic transitions, indicating relatively poor ground state stability and the possible highest chemical reactivity. Overall, molecule A1 with amino substituents achieved good electronic balance, which endowed the molecule with high kinetic stability but low chemical reactivity. Molecules with coexisting push–pull electron effects in substituent combinations (such as the coexistence of amino and nitro groups) (B and C series) have relatively balanced chemical properties and certain reactivity. Molecules with strong electron withdrawing substituents (such as multiple nitro and nitrate ester groups) (D series) exhibit strong electrophilicity and are expected to have relatively poor stability and high sensitivity.
3.4. Energy Characteristics
Energetic properties, containing density (
ρ), heat of formation (Δ
fH298K(s)), detonation heat (
Q), detonation velocity (
D), detonation pressure (
P), and oxygen balance (
OB), represent key attributes of energetic molecular systems.
Figure 5a demonstrates how substituent type, quantity, and location substantially influence molecular density. Generally, density increases with substituent count. The benchmark molecule A1 has the lowest
ρ value of 1.75 g·cm
−3 due to its lack of any substituents. For B series energy storage molecules with one fixed -NH
2 substituent, the
ρ values of all molecules are no more than 1.90 g·cm
−3 and even those of four molecules B1, B3, B4, and B5 are no more than 1.80 g·cm
−3, which is owing to the presence of more -NH
2 and -N
3 in these molecules that contribute less to the
ρ of them. For C series power molecules with one fixed -N
3 substituent, the
ρ values of these molecules are significantly higher than those of the B series molecules, except for molecules C4 and C5, because these two molecules contain two -N
3 substituents that contribute less to the
ρ. For molecule C1 containing only one -N
3 and two -NO
2, molecule C2 containing only one -N
3 and two -ONO
2, and molecule C3 containing only one -N
3 and one -NO
2 and one -ONO
2, their density values are close to 1.90 g·cm
−3, which are 1.88 g·cm
−3, 1.88 g·cm
−3, and 1.89 g·cm
−3, respectively, which is more than that of 1,3,5-trinitro-1,3,5-triazacyclohexane (RDX) [
34], indicating that -NO
2 and -ONO
2 contribute more to the
ρ of energy storage molecules than that of -N
3. It can be clearly seen that the
ρ of D series molecules is higher than 1.90 g·cm
−3, with D1 being 1.92 g·cm
−3 and D2 being 1.93 g·cm
−3, which is more than that of 1,3,5,7-tetranitro-1,3,5,7-tetraazacyclooctane (HMX) [
34]. This is because the substituents of the D series molecules are all composed of -NO
2 or -ONO
2, which contribute significantly to the
ρ of energy storage molecules. Analysis of
ρ reveals the substituent impact sequence is -ONO
2 > -NO
2 > -N
3 > -NH
2. Specifically, incorporating -ONO
2 or -NO
2 groups effectively enhances
ρ values, whereas -N
3 and -NH
2 substitutions yield minimal density improvement. These findings provide critical guidance for designing high-energy-density compounds. Notably, molecules B2, B8, B9, C1, C2, C3, D1, and D2 surpass RDX in density, positioning them as promising candidates.
Figure 5b presents the Δ
fH298K(s) for these energy storage molecules. All molecules exhibit substantially higher values than HMX, even exceeding 2,4,6,8,10,12-hexanitro-2,4,6,8,10,12-hexaazaisowurtzitane (CL-20) [
34] despite substituent variations. This confirms their significant detonation capabilities. Additionally,
Q values were assessed and are displayed in
Figure 5c. It can be seen that except for molecules A1 and B3, all molecules have higher
Q values than HMX, and even higher
Q values than CL-20, with the highest
Q value of 1912 cal·g
−1 for molecule C2. The benchmark molecule A1 has the lowest
Q value of 1167 cal·g
−1 due to its lack of any power substituents, which is consistent with that of
ρ. For B series energy storage molecules with one fixed -NH
2 substituent, the
Q values of all molecules are no more than 1800 cal·g
−1, except for that of B2 and B9, with
Q values of more than 1800 cal·g
−1, owing to the presence of more -ONO
2 or -NO
2 in these two molecules, which contribute more to the
Q. For C series power molecules with one fixed -N
3 substituent, the
Q values of these molecules are significantly higher than those of the B series molecules, except for molecule C4, because molecule C4 contains two -N
3 substituents that contribute less to the
Q. For molecule C2, containing only one -N
3 and two -ONO
2, and molecule, C3 containing only one -N
3, one -NO
2, and one -ONO
2, their
Q values are around 1900 cal·g
−1, which are 1912 cal·g
−1 and 1897 cal·g
−1, respectively, which are far higher than that of CL-20, indicating that -NO
2 and -ONO
2 contribute more to the
Q of energy storage molecules than other substituents. It is obvious that molecule D1 has a relatively higher
Q value of 1846 cal·g
−1, while molecule D2 has a relatively lower
Q value of 1689 cal·g
−1, which is also higher than that of CL-20. Analysis of
Q reveals that the substituent efficacy order is -ONO
2 > -NO
2 > -N
3 > -NH
2, aligning with the trends of
ρ. Specifically, incorporating -ONO
2 or -NO
2 groups more effectively enhances
Q values than -N
3 or -NH
2 substitutions in these molecules. For example, the order of
Q values for molecules B3, B4, and B5 is B3 < B4 < B5, and that for molecules B1 and B3 is B1 > B3.
To further assess the detonation characteristics,
D and
p values were computed and presented in
Figure 5d,e. These results demonstrate that substituent type, quantity, and location significantly influence their detonation parameters. Clearly, increased energetic substituent count enhances molecular detonation properties. This aligns with trends showing that D series molecules exceed C series in
D and
p values, which surpass B series molecules. Overall, these molecules demonstrate strong detonation performances (
D > 8.5 km·s
−1,
P > 30 GPa), except for the benchmark molecule A1, owing to absent energetic substituents. Specifically, for B series energy storage molecules with one fixed -NH
2 substituent, the
D and
p values of these nine molecules are more than 8.5 km·s
−1 and 30 GPa, respectively; the
D values of four molecules B2, B7, B8, and B9 are more than 9.0 km·s
−1; and the
p values of two molecules B2 and B9 are more than 40 GPa, owing to the presence of more -ONO
2 or -NO
2 in these molecules, which contribute more to the
D and
P. For the C series power molecules with one fixed -N
3 substituent, the
D and
p values of all these molecules are significantly higher than those of the B series molecules, except for molecules C4 and C5; this is due to their substituents containing relatively less -NO
2 or -ONO
2—i.e., more -N
3. For example, molecule C1 has one -N
3 and two -NO
2, C3 has one -N
3, one -NO
2, and one -ONO
2, and C4 has one -NO
2 and two -N
3; their
D and
p values follow the order of C4 < C1 < C3, indicating that the contribution order to the
D and
P of the energy storage molecules is -ONO
2 > -NO
2 > -N
3. For molecule C2, containing only one -N
3 and two -ONO
2, and molecule C3, containing only one -N
3, one -NO
2, and one -ONO
2, their
D and
p values are both over 9.6 km·s
−1 and 42 GPa, which are far higher than that of HMX and equivalent to that of CL-20, indicating that -NO
2 and -ONO
2 contribute more to the
Q of energy storage molecules than other substituents. Moreover, molecule B1 has one -NH
2 and two -N
3, and B3 has one -N
3 and two -NH
2; their
D and
p values follow the order of B1 > B3, suggesting that the contribution order to the
D and
P of the energy storage molecules is -N
3 > -NH
2. It is obvious that molecule D1 has the highest
D and
p values (9.71 km·s
−1 and 42.09 GPa), and molecule D2 also has relatively higher
D and
p values (9.54 km·s
−1 and 43.49 GPa), which are equivalent to that of CL-20. Analysis establishes the substituent contribution order to
D and
P as -ONO
2 > -NO
2 > -N
3 > -NH
2, which agree well with that of
ρ and
Q. This correlation arises because
D and
P derive from
ρ and
Q. Specifically, -NO
2 or -ONO
2 incorporation yields greater
D and
P enhancement in these molecules than the -N
3 or -NH
2 groups.
Oxygen balance (
OB) further serves as a key indicator of oxygen sufficiency during explosive decomposition to form carbon and hydrogen oxides. Typically, positive OB values correlate with enhanced energy properties. It can be seen in
Figure 5g that all these molecules show negative
OB values except for molecules D1 (4.3%) and D2 (8.24%). It is notable that molecule C2 exhibits the standard zero oxygen balance. On the whole, the
OB values of all these energy storage molecules obey the order of D series > C series > B series > A series, suggesting that the order of contribution to
OB values is -ONO
2 > -NO
2 > -N
3 > -NH
2, which is consistent with that of
ρ,
Q,
D, and
P. Namely, introducing -ONO
2 and -NO
2 is more beneficial for increasing the
OB values of these molecules than other substituents, such as -N
3 and -NH
2. For example, molecule B5, containing one -ONO
2 and two -NH
2, has the highest
OB value (−25.63%); molecule B4, containing one -NO
2 and two -NH
2, has the second highest
OB value (−32.41%); molecule B1, containing one -NH
2 and two -N
3, has the third highest
OB value (−35.2%); and molecule B3, containing one -N
3 and two -NH
2, has lowest
OB value (−43.81%).
In summary, molecules B2, B8, B9, C1, C2, C3, D1, and D2 exceed HMX in D and P, positioning them as promising candidates of high-energy-density molecules.
3.5. Safety Evaluation
The molecular surface electrostatic potential (ESP) is of great significance in predicting the reactivity of molecules [
35,
36,
37].
Figure 6 shows the ESP of these energy storage molecular systems.
It can be seen that the ESP values of these molecules span up to 37.65 kcal·mol−1, indicating severe charge separation within the molecules. This is mainly due to the strong interaction between the inherent electron-rich property of the tetrazole ring and the extreme and opposite electronic effects of the four substituents. Specifically, -NO2 and -ONO2, as strong electron withdrawing groups, exhibit extremely negative ESP values in the rings they are connected to and their surrounding atoms, making them the strongest electron acceptor regions. As a strong electron donating group, -NH2 exhibits a significant increase in electron density in the connected rings and adjacent regions, resulting in strong negative ESP values. However, the H atom on its N-H bond will exhibit significant positive ESP values due to the electron being pulled towards N atom, becoming a strong electrophilic point. Molecules containing -N3 substituents with a moderate electron withdrawing induction effect exhibit moderate negative ESP values at the terminal N atom, while those in the vicinity of the N atom connected to the tetrazole ring are slightly positive, and the overall ESP performance is between -NH2 and -NO2, but with more electron withdrawing. In summary, these energy storage molecules exhibit highly non-uniform and polarized electrostatic potential distributions driven by the extreme electronic effects of the substituents. Amino groups provide strong electron donating and hydrogen bond donor sites, nitro and nitrate ester groups create strong electron withdrawing centers and super strong hydrogen bond acceptors and energy sources, and azide groups contribute reactivity and moderate polarity. This unique ESP distribution indicates their excellent multiple hydrogen bonding ability, abundant reaction sites, and enormous potential as high-energy-density compounds.
In addition, the surface area distributions within the different electrostatic potential ranges of these high-energy-density nitrogen-rich energy storage molecular systems were calculated. As a benchmark molecule, the surface area of the A1 molecule in different electrostatic potential ranges gradually decreases with the increase in electrostatic potential and is lower than that of any other substituted molecule in this electrostatic potential range, which is attributed to the intrinsic weak electron-rich property of its tetrazole ring. By comparing the surface area distribution of different molecules in different electrostatic potential ranges, it can be inferred that the contribution order of different substituents to negative ESP is -NH2 > -N3> -ONO2 > -NO2. This is because the nitrogen atom in -NH2 exhibits sp3 hybridization, with a lone pair of electrons perpendicular to the molecular plane and completely exposed to the surface, enhancing the electron density of the connected tetrazole ring through electron pushing. The terminal N− (sp hybridization) in -N3 provides localized lone pair electrons, partially offsetting the contribution of lone pair electrons (still showing net negativity). The resonant structure of -ONO2 causes oxygen lone pair electrons to delocalize, resulting in low surface exposure and weakening the electron density of connected atoms. The lone pair of -NO2 electrons are completely delocalized to the N=O bond, with no effective negative charge region on the surface and almost no negative ESP contribution. Overall, the surface area distributions of all these molecules in different electrostatic potential ranges are relatively uniform.
Safety properties constitute critical considerations for energy storage molecular systems. Impact sensitivity (
h50, cm) quantifies these molecules’ safety behavior. Higher
h50 values indicate lower molecular sensitivity. Comparative
h50 data for these molecules and common energetic benchmarks appear in
Figure 5f. It is found that substituent type, quantity, and location substantially influence
h50 values. Increased energetic group count typically reduces safety performance. Nevertheless, almost all molecules demonstrate sufficient
h50 values, validating our effective energy storage molecular design strategy. Specifically, the benchmark molecule A1 has a relatively higher
h50 value (30.35 cm) due to its lack of any power substituents. For the B series energy storage molecules with one fixed -NH
2 substituent, the
h50 values of all molecules are more than 26 cm, with even molecules B3 and B7 being over 40 cm, except for molecules B8 and B9, owing to their increase -NO
2 or -ONO
2, which contribute more to their
D and
P. Obviously, it can be seen that the
h50 values of the C series power molecules are slightly lower than those of the B series molecules, and those of the D series power molecules are slightly lower than those of the C series molecules. Specifically, the B series molecules exhibit
h50 values between 17.93 and 41.12 cm, while those of the C series molecules range from 15.22 to 37.43 cm, and the D series molecules range from 17.76 to 31.47 cm. This is due to the order of contribution to the molecules’ energetic performances (
D,
P) being -ONO
2 > -NO
2 > -N
3 > -NH
2, which is consistent with the inherent contradiction between the energy and sensitivity of energy storage molecules. That is, introducing substituents with a relatively lower energy contribution, such as -NH
2, is beneficial for increasing the
h50 value and enhancing the safety performance.
Collectively, molecules B2, C2, and D2 demonstrate superior energy metrics and enhanced safety profiles compared to HMX, establishing them as promising high-energy-density and low-sensitivity candidates.