两个基于[Fe(bpca)(CN)3]-的一维3d-4f异金属配合物的合成和晶体结构

以[(bpca)Fe(CN)3]-(bpca=二(2-吡啶羰基)酰胺阴离子)为构筑基元,设计合成了2个新颖的3d-4f异金属配合物,{[(bpca)Fe(CN)3Pr(H2O)5]Cl2}n(1)和{[(bpca)2Fe2(CN)6Pr(H2O)6]Cl·4H2O}n(2),并测定了它们的晶体结构.化合物1的晶体属正交晶系,Pnma空间群;而化合物2属三斜晶系,P1空间群.在这2个化合物中,[(bpca)Fe(CN)3]-和[Pr(H2O)x]3 (1,x=5;2,x=6)交替排列形成一维链状结构,并通过π-π堆积作用、氢键作用及分子间短距离相互作用形成三维网络结构.     

MOCVD水平式反应器中热泳力对沉积过程中反应前体浓度分布的影响分析及数值模拟

在MOCVD反应器中,针对GaN生长中的TMGa分子,推导出热泳力、热泳速度以及扩散速度的计算公式.在低温区,热泳速度大于扩散速度;在高温区则相反.影响热泳力的主要因素为温度梯度和分子直径.水平式反应器内,粒子同时受到热泳速度和扩散速度的影响.在只考虑组分输运以及包括化学反应等两种情况下,通过改变反应器上壁面温度,模拟得到水平式反应器中热泳力对沉积速率以及反应物粒子浓度分布的影响.并与文献中的实验数据对比,验证了模拟结果的正确性.结果显示,由于热泳力的影响,在相同操作条件下高温区H2等小直径粒子的质量分数增大、TMGa和NH3等大分子粒子的质量分数减小.从提高生长速率的角度,需减小上下壁面温度梯度;从沉积均匀性的角度,应使到达下游的反应粒子数增多,故需增大上下壁面温度梯度.     

硅晶体生长固液界面形貌研究

结合杰克逊界面理论、分子动力学模拟(MD)和密度泛函理论(DFT),对硅晶体(100)和(111)面生长过程中固液界面形貌进行研究,包括界面自由能变化、结构变化和生长位置吸附能等.通过杰克逊界面理论计算,发现(100)界面晶相原子和流体相原子在表面各占约50;时吉布斯自由能达到极小值,而(111)界面在表面占比约0;或100;时达到极小值,说明当热力学平衡时,(100)面趋向于粗糙面,(111)面趋向于光滑面;分子动力学模拟显示,随着生长的进行,初始光滑的固液界面在(100)面上会逐渐转变为粗糙界面,而(111)面则始终保持光滑界面生长;且在生长过程中,(100)面的生长速率明显高于(111)面,因为(100)面始终为粗糙面生长;DFT计算发现,(100)面上的所有生长位置吸附能接近,可以实现连续生长,(111)面吸附能则存在明显的差值,生长原子需要吸附在台阶处才能进行层状生长.     

立方相KNbO3晶体本征空位点缺陷的电子结构研究

利用第一性原理从头计算方法对立方相KNbO3晶体的肖特基缺陷的稳定性、能带结构、电子态密度和磁性性质进行了研究.发现含本征点缺陷的KNbO3体系结构稳定;K,Nb空位诱导KNbO3缺陷晶体产生铁磁性;O空位则无此性质.K空位诱导KNbO3缺陷晶体磁性源于O原子2p轨道退简并;Nb空位诱导KNbO3缺陷晶体磁性源于O-2p电子极化.     

代数κ-拟-A类算子的Weyl定理

若T或T~*是无穷维可分的Hilbert空间H上的代数κ-拟-A类算子,则Weyl定理对任意的f∈H(σ(T))成立,其中H(σ(T))为σ(T)的开邻域上解析函数的全体.若T~*是代数κ-拟-A类算子,则a-Weyl定理对f(T)成立。还证明了若T或T~*是代数κ-拟-A类算子,则Weyl谱与本质近似点谱的谱映射定理对f(T)成立.     

一类混合单调算子的不动点定理

运用锥理论与迭代方法,讨论了在较弱条件下一类混合单调算子的不动点的存在唯一性,所得结果是某些已有结果的本质改进和推广.     

Theoretical Study on Properties of New Isotope 265Bh

The properties of nuclei belonging to the newly observed α-decay chain starting from 265Bh have been studied. The axially deformed relativistic mean-field calculation with the force NL-Z2 has been performed in the blockedBCS approximation. Some ground state properties such as binding energies, deformations, spins, and parities, as well as Q-values of the α-decay for this decay chain have been calculated and compared with known experimental data. Good agreement is found. The single-particle spectrum of the nucleus 265 Bh is studied and some new magic numbers are found,while the magnitudes of the shell gaps in superheavy nuclei are much smaller than those of nuclei before the actinium region, and the Fermi surfaces are close to the continuum. Thus the superheavy nuclei are usually not stable. The The methods which give good agreement with the data are selected.     

Correlations of Active Galactic Nuclei with Microquasars

Correlations of active galactic nuclei (AGNs) with microquasars are discussed based on the coexistence of the Blandford-Znajek (BZ) and magnetic coupling (MC) processes (CEBZMC) in black hole (BH) accretion disk.The proportions of several quantities of BH systems for both AGNs and microquasars are derived by combining the observational data with CEBZMC. It is shown that the square of the magnetic field at the BH horizon is inversely proportional to the BH mass, while the accretion rate of the disk is proportional to the BH mass. In addition, the very steep emissivity indexes from the recent XMM-Newton observations of the nearby bright Seyfert 1 galaxy MCG-6-30-15 and the microquasars XTE J1650-500 are well fitted by considering the MC effects on the disk radiation. These results suggest strongly the correlations of A GNs with microquasars.     

壳模型对143Pm核跃迁几率的计算

原子核跃迁几率理论计算和实验对比是分析描述原子核内部结构的主要手段之一。目前采用重离子核反应观测到^143Pm核（Z=61，N=82）高自旋能级结构:激发态最大能级达x=8397．6keV，对应自旋J=47／2（h=1）。利用核壳模型在计算^143Pm核能级结构及对应的自旋宇称基础上，系统地对其γ级联跃迁链以及纯E2跃迁进行了计算，并与实验数据进行对比。采用OXBASH程序的单粒子跃迁公式计算了^143Pm的跃迁几率。At present, the high spin state of ^143 Pm（Z = 61, N = 82） have been investigated. The level scheme of ^143Pm has been extended up to an excitation energy Ex = 8 397.6 keV and spin J =47/2（ h = 1 ）. Based on the nuclear shell model （NSM）, we have calculated the sequences of γ-ray transition rates and the pure E2 reduced transition probabilities of ^143Pm, and compared with experimental data. The formula of single-particle transition probability in the OXBASH code was applied in this paper.