银团簇电磁性质的研究
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摘要
团簇研究的最重要意义在于各种特殊性质的应用,银团簇在各个领域中都具有重要的应用价值。本文首先采用密度泛函理论,应用计算程序VASP优化了Agn(n=2-19)团簇的基态结构,并给出了能隙、结合能和对称性等结构参数。在此基础上,本文又进行了两部分计算。
     第一部分,采用FEFF8程序对Agn(n=2-19) X射线近边吸收谱进行了计算。通过比较发现,K、L1、L2、L3边吸收谱有所不同,反映允许的跃迁不同,与电偶极跃迁规则一致。另外,通过比较Ag13的X射线吸收谱发现,处于同一结构不同位置的原子的吸收谱也不一样,谱线波动比较大的对应团簇中心的原子,波动较小的谱线对应团簇外层的原子。
     第二部分,对Agn团簇的磁矩进行了计算。计算结果显示当n<13时,n为偶数Agn没有磁矩,n为奇数Agn有磁矩。n=13时,Agn的磁矩最大,因为Ag13结构高度对称,电子转移较多;n>13时,n为偶数时Agn也有磁矩,这与团簇的结构有关。
As a transition metal clusters, Ag clusters have some unexpected properties. These properties have been widely used in physics, chemistry, materials and other fields. The structure of the clusters greatly affects their properties, but the present experimental conditions were not able to determine the micro-cluster structures, now the information of clusters’structure can only be derived from theoretical calculations. To solve these problem, the VASP procedures were used to calculate their structure by us. First of all,we calculate the structure, energy gap and the vertical ionization energy of Agn (n=2-6) through VASP procedures, compared with the theoretical calculation results and experimental data in published literature. We found the calculation results in this article are in good agreement with the literature, which verify the correctness of calculations.
     Then this article optimized Agn(n = 2-19) clusters structure with VASP in the relativistic core potential approximation ,using density functional theory methods. We calculate energy, energy gap of Agn (n = 2-19) clusters on those ground state structure. By comparison, we found that there was no peak before white line, which is due to K edge is corresponding to the electrons transition from 1 s to 2 s. According to transition selection rule, only P-state can transition to the S state. But the lowest empty state in transition-metal is d state. So transition is not allowed before the white line. However, the L2 and L3 are respectively corresponding to 2P1/2, 2P3/2 transition. In addition to S-state, there is D-state transition, it is allowed transition before the adsorption edge peak, so there is adsorption peak.
     Furthermore, this article also compares three atoms’XANES in the structure of Ag13, the adsorption spectra of atomic is different. The vibration intensity in XANES of the center atom has relatively large vibration intensity. But vibration intensity of the edge atom is light. Using this method, we can determine the surrounding information of the absorption atom in the clusters.
     Finally, magnetic moment of Ag clusters is also calculated in this article. According to results, Agn (n =2-12): when n is even, the average atom magnetic moment is 0; when n is odd, the average atom magnetic moment is gradually reduced. Because of fact that there is a s electron in Ag atom, when n is an even number there are even s electrons, spin angle momentum coupling is 0, there is no magnetic moment of clusters. When n is odd, there are odd s electrons, spin angle momentum coupling is not 0, clusters have magnetic moment. But when n =13, the average magnetic moment is the largest. Because the structure is icosahedral, which is high degree of symmetry. When n is between 13 and 19 except 18, the even clusters have magnetic moment. This structure has a central atom, which has the higher coordination number. The orbital overlap between the 4d orbit of the central atom and the outer 4d orbit increase. Therefore, the 4d low-energy electron transfer from the outer layer of atoms to the center. Then uncouple electrons of the outer layer atoms are increased, so magnetic moment increases . But when n> 13, the even-numbered clusters also have magnetic moment. Because we add an atom on the previous structure to get the structures of Agn(n = 13-17). So the even clusters also have magnetic moment. But there is a central atom, or two at this time, and the structure of clusters is not very symmetrical so the magnetic moment of clusters decreases.
引文
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