BH+2与C2H2反应势能面的量子化学研究

用B3LYP/6-311G(d,p) 密度泛函方法和高级电子相关的CCSD(T)/6-311G(2df,p)偶合簇法研究BH+2与C2H2反应势能面. 结果表明 该势能面上存在(a) H2B+*C2H2, (b) HBCHCH2+, (c) H2BCCH+2和(d) H2*BHCCH+四种异构体, 其中(b)能量最低且在动力学上最稳定, (a), (c)和(d)在动力学上均不稳定; BH+2通过对C2H2的分步亲电加成以及随后的氢迁移和H2消除等反应形成离解产物HBCCH++H2, 该反应不需要活化能且大量放热. 计算结果有助于深入了解BH+2等缺电子硼氢正离子的反应行为.     

范德华复合物Kr-C2H2的势能面和振转光谱的理论研究

采用[CCSD（T）]-F12方法和aug-cc-pVTZ基组,同时引入中心键函数（3s3p2d1f1g）构建了Kr-C₂H₂体系的高精度四维势能面.在构建势能面时考虑了分子间的振动方式及C₂H₂单体内的ν₁对称伸缩和ν₃反对称伸缩振动.将计算得到的四维势能面在Q₁方向和Q₃方向分别做积分得到C₂H₂单体分别处于振动基态和（ν₁,ν₃）=（1,1）激发态的平均势能面.计算结果表明,这2个平均势能面均存在2个等价的T型全局极小值和2个等价线性极小值.全局极小值的几何构型位于R=0.41 nm,θ=65.6°/114.4°,势阱深度为151.88 cm^-1.对径向部分采用离散变量表象法（DVR）,角度部分采用有限基组表象法（FBR）,并结合Lanczos循环算法计算了Kr-C₂H₂的振转能级和束缚态.计算结果表明,复合物在（ν₁,ν₃）=（1,1）区域的带心位移为-1.48 cm^-1,表现为红移,与实验值-1.38 cm^-1很接近;计算得到的红外跃迁频率也与实验值相吻合,说明得到的从头算势能面具有高精度.     

乙炔基自由基(C2H·)与二氧化氮(NO2)气体反应势能面的理论研究

在 CCSD(T)/6-311G(d,p)//B3LYP/6-311G(d,p)+ZPE 水平上对反应C2H+NO2 进行了计算, 建立了反应势能面并得到了3种产物. 利用RRKM理论估算了反应的总速率和分支比. 总速率为1.427×10-12×T0.556×exp(190.547/T) cm3*molecule-1*s-1, 其中主要产物P1(HCCO+NO)比例大于96%, 次要产物P2(HCNO+CO)和P3(HCN+CO2)小于4%.     

H+HCNO反应势能面的理论研究

在CCSD(T)/6-311G(d,p)//B3LYP/6-311G(d,p)+ZPVE水平下, 对反应H＋HCNO进行了研究. 建立了反应势能面, 揭示了该反应的反应机理, 通过H迁移、N—O键或C—N键断裂等多步反应, 得到4种产物, 其中最主要产物为P1(HCN+OH).     

CO2势能面和振动激发态的理论研究

采用振动自洽场-组态相互作用(SCF-CI)方法通过实验振动光谱优化了CO₂分子的势能函数,由该势能函数计算得到的纯振动光谱数据与实验值相比,所有能级的误差均在4cm^-1以内,均方根偏差为1.50cm^-1,所预测的Π态振转光谱也与实验值很接近.     

SO2基态势能面和振转能级的理论研究

在键长-键角坐标下,精确求解SO₂的核振动方程,并通过与实验数据比较来优化势能参数,由所得势能面计算得到38个振动能级,与实验值相比,均方根误差为0.93cm^-1.计算了³⁴SO₂的部分振动能级以及³²SO₂的J=6以下的部分振动能级,所得结果均与实验值较为吻合     

Topological complexity of potential surfaces and application to C2H2 molecule

Summary In this work, we search for the simplest complete surfaces of systems with three and four atoms, i.e. the minimal sets of critical points with their index, which are topologically consistent in the whole configuration space. Then we show the smallest change in the A₂B₂ system by requiring at least one stable acetylene configuration and one stable vinylidene configuration, like on the C₂H₂ surface. Finally, we give complete sets of minima, saddle points and maxima obtained for C₂H₂ with analytical potentials proposed in the literature and with a semi-empirical method at the CAS-CI level.     

基态H2O+的全域多体势能面

基态H₂O⁺分子离子是重要的星际反应中间体.用MRCISD/cc-pVTZ先计算H₂O⁺势能面,然后拟合成多体势能函数.全域势能面能很好地描述基态H₂O⁺的行为.与两条反应通道的实验能变和其构型翻转反应能垒比较,表明计算结果与实验值相符.对计算点完成了力场的多项式拟合,对其振动模式进行了分析     

乙烯基自由基(C2H·3)与羟基自由基(OH·)反应势能面的理论研究

在QCISD（T）/6-311G（2df,p)//B3LYP/6-311G（d,p)水平上对自由基反应C2H3^. OH^.进行了计算，结果表明，经过缔合、多步H转移、CH3转移和离解等复杂过程，最终要得到8种产物（P1-P8），茯中产物P2（H2CCO H2）和P6（CH3CO^. H^.）是主要产物。本文得到的CH2CHOH（1或1‘），CH3CHO（2）和CH3COH（3）之间的过渡态TS1/2，TS1‘/3和TS2/3的能量顺序与Wesdemiotis等的实验推测相反，而与Smith等的计算结果一致。     

Theoretical Study on Dissociation Potential Energy Surface of Peroxynitric Acid

The lowest energy structures of peroxynitric acid have been studied with B3LYP/6-311+ G(2d,2p) method. The potential energy surfaces (PES) along the O-N and O-Obonds have been scanned at CCSD(T)/aug-cc-pVDZ level, respectively. The calculated results show that on the O-N PES, the O3-N4 bond length of the loose transition state is 2.82 ? and the corresponding energy barrier is 25.6 kcal/mol, while on the O-O PES, the loose transition state with of O2-O3 bond length of 2.35 ? has the energy barrier of 37.4 kcal/mol. Thus the primary reaction path for peroxynitric acid is the dissociation into HO₂ and NO₂.     

O+HCNO反应势能面的理论研究

采用CCSD(T)/6-311G(d,p)//B3LYP/6-311G(d,p)+ZPVE方法对反应O＋HCNO进行了研究. 通过反应势能面揭示了该反应的机理, 通过H或O迁移等多步反应路径得到3种产物, 其中, P1(HCO+NO)为主要产物, P2(HNO+CO)和P3(NCO+OH)为次要产物. 为进一步实验研究提供了参考.     

Ne-HCl势能面和振转光谱的理论研究

利用量子化学计算方法CCSD(T)和大基组aug-cc-pVTZ加键函数3_s3_p2_d对Ne-HCl体系的分子间势能面进行了理论研究.结果表明,势能面上有两个势阱,分别对应于线性Ne-ClH和Ne-HCl构型.通过精确求解核运动方程发现,该从头算势能面分别支持5个(对Ne-HCl)和7个(Ne-DCl)振动束缚态.计算得到的振转跃迁频率与实值值吻合.     

Three-dimensional Potential Energy Surface and Bound States of the Ar2-Ne Complex

The first three-dimensional interaction potential energy surface (PES) of the Ar₂-Ne complex is developed using the single and double excitation coupled cluster theory with noniterative treatment of triple excitations CCSD(T). The aug-cc-pVQZ basis sets are employed for all atoms, including an additional (3s3p2d2f1g) set of midpoint bond functions. The calculated single point energies are fitted to an analytic two-dimensional potential model at each of seven fixed r_Ar2 values. The seven model potentials are then used to construct the three-dimensional PES by interpolating along (r—r_e) using a sixth-order polynomial. The PES is used in the following rovibrational energy levels calculations. The comparisons of theoretical transition frequencies and spectroscopic constants with the experimental results are given.     

乙硼烷离子和自由基异构体重排与体系势能面的能量子化学计算研究

在B3LYP/6-311G(d,p)和QCISD(T)/6-311++G(3df,2p)(单点)水平下, 对B2H+5阳离子和B2H*5自由基全优化得到9个几何异构体: B2H+5单态体系(D3h, C1), B2H+5三重态(Cs, Cs, C1), B2H*5自由基(C2v, Cs, Cs, Cs). 得到势能面上与体系异构化过程相联系的5种过渡态.     

O3势能面和振动激发态的理论研究

由于O3在大气化学中的重要作用，近年来针对它的实验和理论研究皆较活跃．尽管对O3的高振动激发态已进行过广泛的研究［“］，得到过多种由实验光谱定出的势能面［‘，’］或由从头算得到的势能函数【‘］，但由于近年来又增加了一些新的高精度的振转光谱实验数据k，’」，而以     

[GeCN2]分子异构化势能面的理论研究

在CCSD(T)/6-311＋G(2df)//B3LYP/6-311＋G(d)水平下, 研究了四原子分子 [GeCN2]的各个异构体的几何结构、红外振动光谱、相对能量及异构化和解离稳定性, 构建了[GeCN2]势能面. 我们得到了7个[GeCN2]异构体, 包括5个直线型结构GeNCN (1), GeNNC (2), NGeCN (3), NGeNC (4), GeCNN (5)和2个环形结构Ge-cCNN (6)和Ge-cNCN (7). 其中异构体5, 6, 7是我们新找到的构型, 而且GeCNN (5)是整个势能面上稳定性仅次于GeNCN (1)的异构体. 几何和电子结构分析表明, GeCNN (5)具有共轭三键结构: Ge≡C—N≡N:. 由于具有良好的热力学和动力学稳定性, 异构体GeCNN (5)有望在实验中观测到. 我们建议利用过渡金属羰基化合物的络合作用可以进一步稳定GeCNN (5). 本研究为寻找新型含高周期元素的多重键化合物提供了理论线索.     

He-N2O的从头算势能面及振转能级

采用超分子MP4方法和较大的基组计算得到了He-N₂O体系的分子间势能面,发现该势能面有3个极小值点,分别对应T形构型及两个线性He-ONN和He-NNO构型.同时采用离散变量表象方法预测了体系的振转能级,计算结果表明,MP4势能面支持5个振动束缚态.     

HCO+NO2反应势能面的理论研究

在B3LYP/6-311G(d,p)和CCSD(T)/6-311G(d,p)水平上给出了HCO+NO₂反应详细的势能面信息.计算结果表明,该反应采用两种无垒进攻方式,分别得到两种加合物H(O)CNO₂和H(O)CONO.找到7种能量低于反应物且合理的产物及相应的反应路径.通过对热力学和动力学的分析,产物HONO+CO(P2,P3),HNO+CO₂(P1)和H+CO₂+NO(P6)的形成更为有利.计算结果同实验相符,且有助于深入了解HCO自由基的化学行为.     

A Theoretical Study on the Potential Energy Surface of the C3 + NO Reaction

The reaction of linear form carbon cluster C₃ molecules in their ¹Σ ground state with NO (X²Π) radicals is explored theoretically to investigate the formation of hitherto undetected NCCCO molecules in the interstellar medium via a neutral-neutral reaction. The doublet potential energy surface is worked out by the ab initio MO calculations at the CCSD(T)/cc-pVTZ//B3LYP/6-311G(d,p)+ZPE level of theory. It is shown that the main pathway of the C₃(¹Σ)+NO(X²Π) reaction involves the N-atom of NO attacking the side C-atom of the ¹C₃ molecule first to form the adduct CCCNO, followed by the N-shift to give I6 CCNCO, and then to the main products P₁ (CCN+CO). Alternatively, I6 can be converted via the N-shift again to I9 (CN)CCO, and then it leads to the minor products P₂ (CNC+CO) and P₃ NCCCO. Since the three pathways have zero threshold energy and proceed via strongly bound energized complexes, they should possess the character of negative temperature dependence, and might be quite rapid even at very low temperature. The reaction represents facile neutral-neutral pathways to produce hitherto undetected CCN, CNC and NCCCO molecules in interstellar environments.     

Customizing Pore System in a Microporous Metal–Organic Framework for Efficient C2H2 Separation from CO2 and C2H4

Selective-adsorption separation is an energy-efficient technology for the capture of acetylene (C₂H₂) from carbon dioxide (CO₂) and ethylene (C₂H₄). However, it remains a critical challenge to effectively recognize C₂H₂ among CO₂ and C₂H₄, owing to their analogous molecule sizes and physical properties. Herein, we report a new microporous metal–organic framework (NUM-14) possessing a carefully tailored pore system containing moderate pore size and nitro-functionalized channel surface for efficient separation of C₂H₂ from CO₂ and C₂H₄. The activated NUM-14 (namely NUM-14a) exhibits sufficient pore space to acquire excellent C₂H₂ loading capacity (4.44 mmol g⁻¹) under ambient conditions. In addition, it possesses dense nitro groups, acting as hydrogen bond acceptors, to selectively identify C₂H₂ molecules rather than CO₂ and C₂H₄. The breakthrough experiments demonstrate the good actual separation ability of NUM-14a for C₂H₂/CO₂ and C₂H₂/C₂H₄ mixtures. Furthermore, Grand Canonical Monte Carlo simulations indicate that the pore surface of the NUM-14a has a stronger affinity to preferentially bind C₂H₂ over CO₂ and C₂H₄ via stronger C-H···O hydrogen bond interactions. This article provides some insights into customizing pore systems with desirable pore sizes and modifying groups in terms of MOF materials toward the capture of C₂H₂ from CO₂ and C₂H₄ to promote the development of more MOF materials with excellent properties for gas adsorption and separation.