AIM Study on the Reaction of CH2SH Radical with Fluorine Atom

采用MP2(Full)/6-311G(d,p)、QCISD(T)/6-311++G(2df,p)和B3LYP/6-311G(d,p)方法研究了CH2SH自由基与F原子的反应．F原子通过进攻自由基上的C原子或S原子形成三种不同的反应通道．计算结果表明F原子进攻自由基上的C原子生成CH2S和HF为主要的反应通道．对反应进程中若干关键点进行了电子密度拓扑分析,找到了该反应的结构过渡区(结构过渡态)和能量过渡态．计算结果表明,对于比较显著的吸热或放热反应,其结构过渡区范围很小,对于吸热或放热不太显著的反应,结构过渡区范围较大.     

钴络合物催化甲醇羰基化制甲酸甲酯反应的理论研究

本文运用密度泛函理论B3LYP方法,对C、O、H采用6-311+G(2d,p)基组,计算研究了钴络合物催化甲醇羰基化制甲酸甲酯反应的微观机理,优化了各反应物、中间体和过渡态的构型特征,用频率分析方法和内禀反应坐标方法对过渡态进行了验证,同时对各中间体进行电荷分析.对比了催化过程与非催化过程的能垒.结果表明,有催化剂参与后反应活化能明显降低.     

SiF_2自由基与异硫氰酸反应机理的理论研究北大核心CSCD

采用密度泛函理论B3LYP方法研究了SiF2自由基与异硫氰酸(HNCS)的反应机理,并在B3LYP/6-311++G**水平上对反应物、中间体、过渡态进行了全几何参数优化,通过频率分析和内禀反应坐标(IRC)确定中间体和过渡态的真实性.为了得到更精确的能量值,又用CCSD(T)/6-311++G**方法计算了在B3LYP/6-311++G**水平优化后的各个驻点的相对能量.根据统计热力学及用Winger校正的Eyring过渡态理论,利用自编程序,计算不同温度下低势垒反应的平衡常数和速率常数,并且通过电子密度拓扑分析讨论了化学反应过程中主要化学键的生成和断裂.计算结果表明,单重态的SiF2自由基与HNCS反应有6条可能的反应通道,其中反应通道SiF2+HNCS→IM1→TS1→IM2HSiF2NCS(P1)为主反应通道.     

Theoretical Study on Reaction Mechanism of Aluminum-Water System

在B3LYP/6-311+G(d,p)和QCISD(T)/6-311++G(d,p) 水平上,对气相中铝与水的反应进行了计算. 理论计算结果表明,铝水反应经过了三条可能的反应通道并且涉及了四个异构体、七个过渡态和两种产物. 其中两条反应通道所涉及的中间物和产物已被实验测得. 同时,在298 K和2000 K计算了铝水反应的焓变和吉布斯自由能,一些计算结果与以前的计算和实验结果吻合较好.     

CH2F自由基与HNCO反应机理的理论研究

采用密度泛函理论的B3LYP方法,在6-311 G(d,p)基组水平上研究了CH2F自由基与HNCO的微观反应机理,优化了反应过程中的反应物、中间体、过渡态和产物的几何构型,通过振动分析验证了所有可能的过渡态;并且还在QCISD(T)/6- 311 G**//B3LYP/6-311 G(d,p)机组水平上计算了相应单点能．找到了CH2F自由基与HNCO反应的7条可行的反应通道,对结果的分析表明,CH2F HNCO→TS8→IM5→TS9→IM4通道的控制步骤活化能最低,是该反应的主要通道．     

顺式羰基铑碘络合物催化甲醇制乙酸反应的动力学研究

本文运用密度泛函理论DFT-B3LYP方法,对铑、碘元素采用相对论校正赝势基组SDD,对C、O、H采用6-311+G(2d,p)基组,计算研究了顺式羰基铑碘络合物催化甲醇羰基化制乙酸反应的微观机理,优化了各反应物、中间体和过渡态的构型特征,用频率分析方法和内禀反应坐标方法对过渡态进行了验证,运用Kozuch撰写的能量跨度模型获得循环反应的动力学信息,确定了决定循环反应速率的决速过渡态和决速中间体,并利用转化频率评估了催化性能与温度的变化关系.     

NH3与MH(M=Li,Na)反应机理的密度泛函理论研究

采用密度泛函理论B3LYP方法研究了NH3与MH(M=Li,Na)的放氢反应机理,在6-311G(2d,2p)基组水平上对反应物、中间体、过渡态及产物进行了全几何参数优化,频率分析和内禀反应坐标(IRC)计算证实了中间体和过渡态的正确性和相互连接关系。计算结果表明,NH3与MH(M=Li,Na)的反应均为单通道的氢取代反应,反应生成LiNH2(NaNH2)与H2。     

NH_3与CaH_2反应机理的密度泛函理论研究

基于密度泛函理论(DFT)当中的B3LYP(杂化密度泛函)方法,于6-311G(d,p)基组水平上对NH_3与CaH_2的反应机理进行了计算分析,对反应过程中的反应物、中间体、过渡态及产物进行了全几何参数优化,得到其构型和基本参数.对得到的中间体和过渡态进行频率分析和内禀反应坐标(IRC)计算,以证实中间体和过渡态的正确性和相互连接关系.使用QCISD方法在6-311G(d,p)基组水平对各驻点的单点能进行计算,给出能量信息.计算结果表明:CaH_2与NH_3主要以摩尔比为1:2进行反应,分两步氢取代过程,生成产物Ca(NH2)2和2H2.反应所释放的H2中两个H原子分别来源于CaH_2和NH_3,反应的关键是脱氢,主要在于克服N—H键断裂所需能量.相比较而言从NH_3中脱氢比从—NH2中脱氢较易.     

异硫氰酸与CF2自由基反应机理的量子化学研究

采用密度泛函理论B3LYP方法研究了CF₂自由基与HNCS的反应机理,并在B3LYP/6-311++G**水平上对反应物、中间体、过渡态进行了全几何参数优化,通过频率分析和IRC确定中间体和过渡态的真实性.为了得到更精确的能量值,又用CCSD（T）/6-311++G**方法计算了在B3LYP/6-311++G**水平优化后的各个驻点的相对能量.根据统计热力学及用Winger校正的Eyring过渡态理论,利用自编程序,计算不同温度下低势垒反应的平衡常数和速率常数.计算结果表明,单重态的CF₂自由基与HNCS的反应有6条可能的反应通道,三重态的CF₂自由基与HNCS的反应有1条反应通道.其中单重态反应通道CF₂+HNCS→IM1→TS1→IM2 HCF₂NCS（P1）为主反应通道.     

氟代吡啶阳离子的理论研究

利用量子化学密度泛函理论B3LYP方法及 6 31G(d ,p)、6 311G(d ,p)、6 31+G(d ,p)和 6 311+G(d ,p)基组对五氟代吡啶、2 ,6 二氟代吡啶和 2 氟代吡啶分子的阳离子进行了计算研究 .B3LYP构型优化和频率分析计算结果表明这三种氟代吡啶阳离子的结构分别具有C2v、C2v和Cs 对称性 ,电子基态分别为2 A2 、2 A2 和2 A″ .对离子和分子的计算构型做了比较 .利用B3LYP方法和不同的基组对这三种阳离子及其分子进行了自然布居分析计算 .用B3LYP方法对这三种阳离子 (自由基 )中的超精细结构进行了计算 ,对五氟代吡啶、2 ,6 二氟代吡啶和2 氟代吡啶分子的垂直电离势和绝热电离势进行了计算 ,与实验值符合得很好     

SnO2/CeO2表面反应速率方程和分子反应几率

介绍了反应温变测试装置原理及其实验规律,利用粉末溅射平面薄膜型SnO2/CeO2酒敏传感器测试了反应温变;并用内插法给出了反应温变随酒气气体浓度变化的规律.对表面反应速率方程进行了推导,并对分子表面反应的几率进行了计算.给出了普遍的反应速率方程,它包括了两种常用的经验公式:双曲线型和幂函数型公式;同时得到了分子反应几率是小的概念,其值一般为10-3～10-5.     

氟原子与反式1,3-丁二烯分子反应动力学的理论研究

在CCSD(T)／6-311g(d,p)／B3LYP／6-311g(d,p)的基础上对F原子与反式的1,3-丁二烯的反应体系进行了理论研究．计算中发现,这个反应体系有两个形成中间复合物的通道．同时,理论计算结果表明,在交叉分子束的实验中探测到的H原子是通过这两个形成长寿命的中间复合物的通道产生的．而通过同一个复合物通道,生成C2H3 C2H3F的速率要比生成氢原子的低,在交叉分子束实验中要探测到C2H3 C2H3F通道也是很困难的．理论分析的结果还表明, HF也可能是反应中的一个产物,它主要是通过直接抽取反应产生的．     

Cross-section measurements for the reaction B(p, He)Be

Cross sections have been measured for the transitions to the ground state and first excited state of ⁸Be and to the two 2⁺ levels at 16.63 MeV and 16.93 MeV excitation in the reaction ¹⁰B(p, ³He) at E_p = 49.5 MeV. The angular distributions of the cross section were compared with DWBA predictions.     

Multiple coulomb excitation of 167Er

The ground-state rotational band in ¹⁶⁷Er has been investigated through multiple Coulomb excitation with a 160 MeV ³⁵Cl beam. Excited states up to $\text{25}\text{2}{}^{\mathrm{+}}$ were established by measuring γγ coincidences and γ-ray angular distributions. Gamma-gamma angular correlations were also measured. Nuclear lifetimes of levels up to spin $\text{23}\text{2}$ have been determined from Doppler-broadened γ-ray lineshapes, and B(M1) and B(E2) values of intra-band transitions deduced. Considerable signature dependence was observed for level energies and M1 transition probabilities. A Coriolis band-mixing calculation was carried our for comparison with the experimental results. The measured M1 transition probabilities are compared to calculations based on a particle-rotor model, a cranking model, and a microscopic model with quantum-number projection.     

On the possibility of detecting superheavy quasimolecules

The formation of superheavy electronic quasimolecules leads to measurable deviations from the Rutherford cross section in heavy ion collisions. For the system ²³⁸₉₂U-²³⁵₉₂U with E_c.m. = 800 MeV we find an average correction of 1.5% for the scattering cross section in forward directions. Additional background contributions like electronic shielding of the nucleus, vacuum polarization, nuclear Coulomb excitation and static deformations of the nuclei are taken into account.     

Problems of angular momentum projection in nuclear physics

In nuclear models approximate wave functions are often used which do no have sharp angular momentum as required of the exact wave functions. It seem obvious that model wave functions of this type should be improved by projection onto states of good angular momentum. It is not the purpose of this paper to discuss the technical difficulties of projection (which can be formidable for many particle systems), but rather to present in an elementary way certain fundamental ambiguities in the use of projection. An application to high spin states near the yrast line is suggested.     

The interaction of 538 MeV 56Fe with 238U

Binary coincident fragments from the ⁵⁶Fe+²³⁸U reaction at 538 MeV have been studied. Fragment energies were measured and fragment masses determined by a kinematic method. Three types of event are defined by suitable adjacent limits in the mass versus energy event space. The angular distributions of cross section, energy and mass have determined for each event region and particular attention paid to that part containing possible fissions following complete fusion. The total reaction cross section consists of about 50 % of binary fragmentation channels. The remaining channels correspond to a ternary process of heavy recoil fission.     

Polarization of preequilibrium proton emission in the 93Nb + 14N reaction

Spin polarization of protons emitted at 20° and 40° in the ⁹³Nb + ¹⁴N reaction at 95 MeV has been measured by the double scattering method using a polarimeter particularly designed for protons having a continuous energy distribution.The result shows that the polarization is small for low-energy protons, but increases smoothly with the increase of proton energy, reaching around + 20 % at about 20 MeV in the center-of-mass system. Energy and angular distributions of protons measured in the same reaction indicate coexistence of equilibrium and preequilibrium components in the proton emission of interest, the fraction of the preequilibrium component increasing with the increasing proton energy. If we assume that protons emitted in equilibrium are completely unpolarized, and that the value of polarization (P) for the preequilibrium component is independent of proton energy, the present result is consistent with $\text{P ? + 22 \%}$ for the emission at 20° and $\text{P ? + 38 \%}$ for the emission at 40°.The result is discussed in terms of the hot-spot model for precompound decay.     

Study of 94Mo through the (n,n′γ) reaction

The ⁹⁴Mo(n, n′γ) reaction has been studied in the neutron energy range 1.5–4.0 MeV. Neutron inelastic scattering cross sections for levels up to an excitation energy of 2.6 MeV have been measured from 1.5 to 3.0 MeV. The results have been analyzed with the optical-statistical and coupled-channels theories. The 1.74 MeV level has been observed and has been assigned to be 0⁺. The branching ratios for the γ-rays deexciting the levels below the 3.5 MeV excitation have also been obtained.