HPO_2异构体结构和相对稳定性

在MP2/6-311++G（d,p）和QCISD（t）/6-311++G（3df,2p）（单点）水平下计算得到了包括8个异构体和12个过渡态的HPO2体系势能面.在势能面上,异构体cis-HOPO（EI）的能量是最低的,其次是trans-HOPO（E2）和HPO（O）（C2v,E3）,能量分别比cis-HOPO高10.99和48.36 kJ/mol.根据体系的势能面,只有异构体E1和E3具有较高的动力学稳定性,在实验中应该可以观测到.PH和O2直接反应生成的cis-HPOO（E5）和trans-HPOO（E6）经过几步势垒较低的异构化过程就可以异构化为具有较高动力学稳定性的产物E1;而OH和PO反应可直接生成E1.计算结果较好地解释了相关实验.     

HAsS2异构体结构与稳定性

在MP2/6-311++G(d,p)和QCISD(t)/6-311++G(3df,2p)(单点)水平下计算得到9个异构体和10个过渡态的HAsS₂体系势能面.异构体cis-HSAsS(E1)的能量最低,其次是trans-HSAsS(E2)、具有AsSS三元环的立体HAs(S)S(C_{s,E3)和HAs(S)S(C2v,E4)结构的异构体,能量分别比cis-HSAsS高1.46,60.78和93.63kJ/mol.根据体系的势能面,异构体E1,E2,E3和E4具有一定的动力学稳定性.AsH和S2第一步反应产物将会异构化为具有较高动力学稳定性的异构体E3,而SH和AsS第一步反应产物将会异构化为E1.计算结果与HNO2,HNS2,HPO2,HPS2和HAsO2等价电子相同的分子的势能面进行了比较.}     

HPOS体系异构体结构与稳定性

在MP2／6－311＋＋G(d,p)和QCISD（T）／6－311＋＋G（3df,2p)（单点）水 平下计算得到了HPOS体系势能面上18个异构体和25个过渡态及解离碎片等驻点，并 分析了这些异构体的结构及异构化过程，讨论了可能的解离方式。在得到的异构体 中，有8个异构体是动力学较稳定的，它们是dis-HOPS,trans-HOPS,trans-HSPO, cis-HSPO,HP(O)S(Cs),trans-HPSO,cis-HPSO和HP（O）S（C1）。这些异构体在实 验中应该可以观测到。理论研究表明，P与S原子较强的超价能力在降低异构体能量 ，提高异构体动力学稳定性方面起到了关键的作用。得到的计算结果与HPO2， HPS2，HNOS等价电子相同的体系进行了比较。     

HPS2异构体结构与相对稳定性

在MP2/6-311++G(d,p)和QCISD(t)/6-311++G(3df,2p)(单点)水平下计算得到了包括9个异构体和15个过渡态的HPS2势能面.其中,异构体trans-HSPS(E1)的能量最低, 其次是cis-HSPS(E2)和HPS(S)(C2_V,E3),能量分别比trans-HSPS(E1)高3.43和14.17 kJ/mol.计算结果表明,异构体E1,E2,E3和立体的三元环结构的异构体HP(S)S(C_S,E4), 及与E4共存的trans-HPSS(E5)和cis-HPSS(E6)具有一定的稳定性.在QCISD(t)/6-311++G(3df,2p)//MP2/6-311++G(d,p)并包含零点能水平下,PH和S₂反应生成的E6和E5分别越过65.75和71.73 kJ/mol的势垒就可以异构化为具有较高动力学稳定性的产物E4, 计算结果对实验认定的产物是cis-HPSS(E6)的结论进行了修正.     

HAsO~2异构体结构、相对稳定性与体系势能面

在MP2/6-311++G(d,p)和QCISD(T)/6-311++G(3df,2p)(单点)水平下计算得到了包括9个异构体和10个过滤态的HAsO~2体系势能面。在势能面上，异构体cis-HOAsO(E1)的能量是最低的，其次是trans-HOAsO(E2)和HAsO(O)(C~2~V,E3)，能量分别比cis-HOAsO高13.15和192.74kJ/mol。根据体系的势能面，异构体E1，E3及cis-HOOAs(E6),trans-HOOAs(E5)具有一定的动力学稳定性，在实验中应该可以观测到。AsH和O~2反应的第一步产物将会异构化为具有较高动力学稳定性的异构体E3；而OH和AsO反应可直接生成E1。计算结果与HPO~2,HPS~2,HNO~2,HNS~2等价电子相同的分子的势能面进行了比较。     

HBO2异构体的结构和相对稳定性

用ab initio方法在MP2/6 311＋＋G(d,p)水平下优化得到了HBO2体系的若干异构体和过渡态，并在QCISD(t)/6 311＋＋G(3df,2p)//MP2/6 311＋＋G(d,p)水平下进行了单点能量校正.对计算结果的分析表明，无论是在热力学还是在动力学上，具有链状结构的HOBO异构体(E1)是势能面上最稳定的结构，并对E1的电子结构进行了分析；另一具有C2v对称性的HBO(O)结构的异构体(E2)的能量比E1高381.72 kJ•mol－1，由于E2处于一个较深的势垒中，因此是比较稳定的，可以推断，在适合的实验中应该可以观察到异构体E2.     

[C, N, N, P]体系异构体结构与稳定性

在B3LYP/6-311G(d)和QCISD(t)/6-311+G(2df)水平下计算得到了[C, N, N, P]体系的9个异构体、20个过渡态及一些相关的解离碎片, 并研究了异构体之间的异构化过程, 讨论了该体系异构体的结构与稳定性. 结果表明在得到的9个异构体中, 具有2A′电子态的、非线型链状NCNP, NCPN, CNPN和CNNP 4个异构体是较稳定的. 其余异构体由于易于重排或是解离, 稳定性较低. 研究同时给出了这4个异构体的振动频率、转动常数、偶极矩、第一绝热电离能和绝热电子亲合能等相关数据, 为可能的实验和星际光谱观测提供相关的理论数据. 得到的计算结果与等价电子体系SiNNP进行了比较.     

[Si,N,N,P]体系异构体结构与稳定性

在B3LYP/6-311G(d)和QCISD(t)/6-311+G(2df)(单点)水平下计算得到了[Si,N,N,P]体系势能面上的一些驻点, 研究了异构体之间的异构化过程, 并讨论了该体系异构体的结构与稳定性. 结果表明在[Si,N,N,P]体系中的11个异构体中只有含有Si-P交叉成键的类蝶型四元环异构体SiNPN(E1, ²A″)是稳定的, 其他异构体由于易于重排或是解离, 稳定性较低. 研究同时给出了E1的电子与几何结构、振动频率及指认、偶极矩和转动常数等相关数据. 分析结果表明通过中间体E3(SiNPN)的反应SiN(²Π) + PN(¹Σ)→E1是由SiN(²Π)和PN(¹Σ)碎片产生E1的最有利途径, 因此E1可成为星际观测的目标. G2级别下此反应的反应焓变为215.25 kJ/mol (298.15 K), 而异构体E1在298.15 K下的标准生成焓为457.99 kJ/mol.     

C70S可能异构体的结构与稳定性的理论研究

分别用半经验的AMl，PM3及MNDO方法研究了富勒烯衍生物C70S的12种可能异构体的结构和稳定性．计算结果表明：S原子加成在4种6-6键上的稳定构型中，非赤道带6-6键加成的三个异构体为闭环结构，赤道带6-6键加成的一个异构体为开环结构；S原子加成在4种6-5键上均可产生开环和闭环两种稳定构型．加成在6-5双键的异构体其闭环构型更稳定，加成在6-5单键的异构体其开环构型更稳定．闭环异构体中S原子加成在碳球极处6-6键上的构型1，2最稳定，开环异构体中S原子加成在赤道带6-6键上的构型8最稳定．     

磷炔R-C≡P(R=-BH2,-CH3,-NH2,-OH)及其异构体的稳定性

采用 B3LYP和 CCSD(T)方法对 R-C≡ P(R=-BH2, -CH3,-NH2, -OH)体系进行了理论研究 .结果表明,含 C≡ P三键的异构体 BH2-C≡ P和 CH3-C≡ P在各自的体系中分别是热力学最稳定的结构 .而在 HO-C≡ P和 NH2-C≡ P体系中,热力学最稳定的结构却是 H-P=C=O和含 C≡ N三键的 N≡ C-PH2.动力学理论研究表明,没有相关实验研究的 R-C≡ P(R=-BH2,NH2)体系中共有 5种异构体是动力学稳定的 .在 HO-C≡ P体系的 2种动力学稳定的异构体中, H-P=C=O连接方式的异构体已被实验所证实,而另外一种 HO-C≡ P连接方式的异构体的动力学稳定性较高,实验中可以观察到 .对于 CH3C≡ P体系,研究所预示的 2种动力学稳定的异构体中 CH3-C≡ P已被实验证实,从理论上推测另一种动力学稳定性较高的异构体 HC≡ C-PH2在实验中也可以检测到.     

Two Novel Isomers of HPS3 System

Two new isomers of HPS3 system, FIP(S)S2 and HSSPS, are predicted by means of B3LYP method with 6-311 G(3df,3pd) basis set. The two isomers can isomerize into thermodynamically the most stable species HSPS2, which have been experimentally identified,with relatively higher reaction barriers. In view of their higher thermodynamical and kinetic stability and the experimental observation for I-IP(O)O2 and HOOPO in previous study, we can reasonably believe that the two species can be spectrosymmetrically characterized in future experiments.     

Structures and stabilities of HPO_2 isomers

The potential energy surface of HPO2 system including eight isomers and twelve transition states is predicated at MP2/6-311++G(d, p) and QCISD(t)/6-311++G(3df,2p)(single-point) levels of theory. On the potential energy surface, cis-HOPO(E1) is found to be thermodynamically and kinetically most stable isomer followed by trans-HOPO(E2) and HPO(O)(C2v, E3) at 10.99 and 48.36 kJ/mol higher, respectively. Based on the potential energy surface, only E1 and E3 are thermodynamically stable isomers, and should be experimentally observable. The products cis-HPOO(E5) and frans-HPOO(E6) in the first-step reaction of HP with O2 can isomerize into isomer E1 that has higher stability. The reaction of OH with PO will directly lead to the formation of isomer E1. The computed results are well consistent with the previous experimental studies.     

The Structures and Stability of HNOS Isomers

Potential energy surface of HNOS system is investigated by means of MP2 method with 6-311 G(d,p) basis set.The energy for each minimum and saddle point on the potential energy surface is corrected at the QCISD(T)/6-311 G(3df,2p) level of theory with zero-point vibrational energy included.As a result ,eighteen isomers are theoretically predicted and cis-HNSO is found to be global minimum on the potential energy surface,Wherein,fourteen isomers are considered as kinetically stable species,and should be experimentally observed.Comparisons are made for HNOS system with its analogues,HNO2 and NHS2.The nature of bonding and isomers‘ stability of HNOS system are similar to HNS2.The obvious similarities and discrepancies among HNOS,HNO2 and HNS2 are attributed to the hypervalent capacity of sulfur,oxygen and nitrogen atoms.     

Structures and Stability of HNS_2 Isomers

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Structures and Stability of NHS2 Isomers

Potential energy surface of HNS2 is investigated by means of second-order Moller-Plesset Perturbation theory(MP2) and QCISD(T) (single-point)methods,At final QCISD (T)/6-311 G(3df,2p)//MP2/6-311 G(d,p),level with zero-point vibrational energies included,cis-NHSS is found to be global minimum on the potential energy sufrace,followed by low-lying trans-HNSS ,HN(S)S(C2v).cis-HSNS,cis-NSSN,trans-HSNS,trans-NSSN,and HN(S)S(Cs) by 13.46,66.92,78.25,80.38,81.22,81.38 and 86.40 kJ/mol,respectively.A new high-lying HS(N)S isomer with Cs symmetry is located on the potential energy surface ,The kinetic stabilities of all isomers are predicted.Comprisons are made for HNS2 with its analogues,NHO2,HPS2 and HPO2,The causes that lead to the differences between HNS2 and its analogues are hypervalent capacity of phosphorus and distinct electronegativities of hydrogen,nitrogen and phosphorus.     

Structures,Vibrational Spectra,and Relative Energetics of CH3COIO3 Isomers

The structures, vibrational spectra, relative energetics, and enthalpies of formation of CH₃COIO₃ isomers have been investigated with B3LYP, B3P86 and B3PW91 methods in conjugation with the 6‐31+G(d), 6‐311+G(d,p) and 6‐311++G(3df,3pd) basis sets. The CH₃COOIO₂ structure was found to be the most stable form among the isomers with an estimated enthalpy of formation of ?314.6 kJ·mol^?1. The enthalpies of formation for CH₃COOOOI, CH₃COOOIO and CH₃COIO₃ are ?180.7, ?184.9 and ?50.6 kJ·mol^?1, respectively. The implication of the formation of CH₃COIO₃ isomers from the atmospheric cross‐reactions of the acetylperoxy (CH₃COO₂) and iodine monoxide (IO) radicals was examined and the possible dissociation products of the most likely CH₃COIO₃ isomers were determined.     

Theoretical Study on the Structures and Stability of Isomers and Complex of[Si,C,O,O] Sytem

A detailed singlet potential energy surface(PES) of [Si,C,O,O] system including a van der Waals (vdW) comples SiO……CO2,eight isomers,and twelve transiton states is investigated by MP2 and QCISD(T) (single-point)methods.At the final QCISD(T)/6-311 G(2df)//MP2/6-311G(d) level with zero-point energy included,the complex SiO……CO is found to be thermodynamically and kinetically the most stable species.Although eight ismoers are located as local energy minima,they are rather unstable toward isomerization to the dissociation fragments or comples.For the reaction of silocon atoms with carbon dioxide,two competitive reaction channels are found,and the primary pathway,which leads to the products of SiO and CO fragments,is the direct oxygen-abstraction process from carbon dioxide by silicon atom with a41.16 kJ/mol reaction barrier height.Our predications are in good agreement with previous experimental and theoretical studies.     

Singlet H-cCNC-C：A Potential Interstellar Molecule

A new planar isomer of HNC3 system,H-cCNC-C,is theoretically predicted by means of B3LYP and CCSD(T) methods.The suggested species can isomerize into other five kinetically more stable isomers,which have been experimentally identified,with relatively higher reaction barriers.In view of its higher kinetic stability,we can reasonably believe that the obtained species H-cCNC-C can be experimentally observed in future studies.     

Theoretical Study on the Structures and Stability of Isomers and Complex of [Si, C, O, O] System

Introduction[Si,C ,O ,O]systemhasattractedmuchattentioninthefieldsofchemistryandmaterials1 3becauseofthefollow ingseveralcauses .First,theinterestisthepotentialimpor tanceininterstellarspace .Heretofore ,SiC ,SiOandCOhavebeendetectedwithintheinterstellarmediumformanyyears,butno [Si,C ,O ,O]isomerswereobservedinthenebulae .FormanySi containingsystemshavebeenstudiedexperimentallyandtheoretically ,4 8andinviewofthepossibleexistenceofthe [Si,C ,O ,O]radicalininterstellarspace ,weselectthe…