计及级联内缺陷空间关联的团簇动力学模拟

团簇动力学（CD）是一种快速模拟材料辐照损伤长时间动力学演化方法.基于平均场速率理论的CD不考虑级联内的缺陷空间关联效应.而实体动力学蒙特卡罗（OKMC）模型虽然考虑空间关联效应,但受到时间尺度和辐照剂量的限制.将模拟粒子初级辐照级联缺陷分布的Monte Carlo模型（IM3D）与OKMC基于常数时间退火方法进行耦合,有效计及级联内的缺陷空间关联性,作为CD模型的有效辐照产生项,建立计及空间关联效应的团簇动力学模型（CD-SC）.结果表明：CD-SC模拟的辐照损伤结果与长时间OKMC结果吻合.有助于提高典型辐照条件下核材料长时间辐照损伤的多尺度模型的准确度和效率.     

Non-Adiabatic Effects of Superconductor Silane under High Pressure

We present the investigations of non-adiabatic effects by including vertex corrections in the standard Eliashberg theory and show that high phonon frequency is unfavorable to superconductivity in the regime of strong vertex correction. This means that it is hard to find high-transition-temperature superconductors in the compounds with light elements if the non-adiabatic effects are strong. The interplay interaction between non-adiabatic effect and Coulomb interaction makes the transition temperature of silane superconductor not so high as predicted by the standard Eliashberg theory.     

中性和带电小钨团簇的第一性原理研究

采用基于密度泛函理论的第一性原理方法,计算了中性和带电小钨团簇W_n（n＝3—6）的构型,得到了一些能量较低的结构,它们都有可能是团簇的基态.研究发现,这些团簇大多具有较低的自旋多重度：中性小钨团簇为自旋单态或三重态;带电小钨团簇为自旋双重态或四重态.当n>3时,小钨团簇具有三维立体结构.通过拟合光电子谱、计算垂直离化能并与实验值比较,进一步讨论了带负电小钨团簇的基态结构. 关键词： 小钨团簇 构型 密度泛函理论     

YBa_2Cu_3O_(7-δ)系高Tc超导体中的铜氧互作用

本文用子团模型模拟了在高Tc超导材料YB_2Cu_3O(7-δ)中铜氧原子(离子)间的相互作用,在局域密度近似下求解HFS方程的自给解的DV-X_α方法研究了一种可能的YBa_2Cu_3O_(7-δ)晶体结构模型基础上存在的各种不同的铜氧离子间的电子转移,键结合及费密面附近的态密度。     

中子预辐照损伤对钨中氢滞留行为影响机制的多尺度模拟

高温等离子体作用下的中子辐照损伤和氢氦滞留行为一直是聚变堆钨基材料面临的两个关键问题,尤其是预辐照损伤对氢氦滞留的协同作用。鉴于制约因素的复杂性和实验上的困难,相关基础问题的理论研究至关重要。我们基于发展的顺序多尺度模拟方法研究了多晶钨的中子预辐照损伤及其对低能（20 eV）氢注入下缺陷动力学演化和氢滞留分布的影响。通过定量对比有无中子预辐照的多晶钨中氢的滞留行为,我们发现中子预辐照损伤产生的稳定空位团簇作为新的氢捕获点,加剧了氢在近表面处的滞留和表面损伤,限制了其向深度的扩散,从而导致了低能氢滞留量的急剧增加。相关结果将直接为实际等离子体环境下聚变堆钨基材料的辐照损伤和氢氦效应提供理论指导与预测。     

Structural, electronic, and magnetic properties of CrN under high pressure

The structural,electronic and magnetic properties of CrN under high pressure are investigated by first-principles calculations.The antiferromagnetic orthorhombic structure is identified to be the preferred ground state structure.It possesses a bulk modulus of 252.8 GPa and the nonzero magnetic moment of 2.33 μ B per Cr ion,which agree well with the experimental results.CrN undergoes structural and magnetic transitions from an antiferromagnetic rocksalt structure to a non-magnetic Pnma phase at 132 GPa.Under compression,the magnetic moment of the Cr ion reduces rapidly near the equilibrium and phase transition point,and the distribution of the density of states is broadened,but the form of overlap between the orbitals of Cr d and N p remains unchanged.The broadening of the band induces spin flipping,which consequently results in the smaller magnetic moment of the Cr ion.     

Interaction of hydrogen molecules on Ni-doped single-walled carbon nanotube

Adsorption of hydrogen molecules on an Ni-doped (8,0) single-walled carbon nanotube (SWNT) is investigated by using first-principles density functional calculations. The result shows that a single Ni atom adsorbed on the bridge site of the tube could cannot dissociate the H₂, however it can chemisorb three H₂ at most, with the average binding energy per H₂ suitable for the hydrogen storage at the room temperature. More H₂ would physisorb around an Ni atom weakly. As for the SWNT with an Ni dimer adsorbed, we find that when the H₂ approaches the Ni--Ni bond, it dissociates without overcoming any barrier and makes bonds with Ni atom.     

Route to Stabilize Cubic Gauche Polynitrogen to Ambient Conditions via Surface Saturation by Hydrogen

Cubic gauche polynitrogen(cg-N) is an attractive high-energy density material. However, high-pressure synthesized cg-N will decompose at low pressure and cannot exist under ambient conditions. Here, the stabilities of cg-N surfaces with and without saturations at different pressures and temperatures are systematically investigated based on first-principles calculations and molecular dynamics simulations. Pristine surfaces at 0 GPa are very brittle and will decompose at 300 K, especially(110) sur...