分子束外延生长的n型Al掺杂ZnS_(1-x)Te_x深中心研究

应用电容-电压、光致荧光和深能级瞬态谱技术研究了分子束外延生长的n型Al掺杂ZnS_(1-x)Te_x外延层深中心。Al掺杂ZnS_(0.977)Te_(0.023)的光致荧光强度明显低于不掺杂的ZnS_(0.977)Te_(0.023),这表明一部分Al原子形成非辐射深中心。Al掺杂ZnS_(1-x)Te_x(x=0,0.017,0.04和0.046)的深能级瞬态傅里叶谱表明，Al引进导带下的0.21和0.39eV电子陷阱，Te除了作为材料合金的成分和等电子中心外，还涉及到一个电子陷阱的形成，其相对导带的能级位置随Te组分增加而减小。实验结果还表明仅有少量掺杂的Al原子形成非辐射中心，这说明Al对于Te组分范围内(x≤0.046)的ZnS_(1-x)Te_x外延层的确是一种非常好的施主杂质。

优质应变Si_(1-x)Ge_x/Si超晶格的气源分子束处延

于2010-11-23批量导入

InxGa（1-x）As/GaAs应变单量子阱结构的静压光致发光研究

国家自然科学基金

The growth of ZnO on bcc-In2O3 buffer layers and the valence band offset determined by X-ray photoemission spectroscopy

This work was supported by the 863 High Technology R&D Program of China (Grant Nos. 2007AA03Z402 and 2007AA03Z451), the Special Funds for Major State Basic Research Project (973 program) of China (Grant No. 2006CB604907), and the National Science Foundation of China (Grant Nos. 60506002 and 60776015). The authors express their appreciation to Dr. Tieying Yang and Prof. Huanhua Wang (Beijing Synchrotron Radiation Facility, Institute of High Energy Physics, Chinese Academy of Sciences) for XRD measurements and helpful discussions.

维生素C二步发酵新组合菌G.529及其应用

本文筛选一株苏芸金杆菌与氧化葡萄糖酸杆菌组成的新组合菌G. B529，并对其生物学性质进行研究，结果表明：新组合菌的摇瓶发酵转化率较原菌系提高4.83个百分点，发酵速度快，且具有耐受高浓度（10%）山梨糖的特性。为使G. B529的潜能得到最大程度的发挥，对其影响因素进行研究。首先应用均匀设计方法确立了G. B529的发酵培养基优化配比，在所实验的范围内，发酵转化率与玉米浆浓度成正相关性，尿素浓度 1．45%佩W/V)时，转化率达最大。其次种液各参数对发酵影响实验确立了判断种子质量高低的方法。结果显示种液中的大菌OD值一1.6 X小菌OD值可以作为种液的质量指数。最后对种子质量的影响实验显示适当提高玉米浆、葡萄糖等成分的浓度与降低尿素的浓度及调高pH值均有利于种液质量的改善。同时低接种量、大通气量和选择种龄为14小时均有助于种液质量指数的提高。 新组合菌系在选定的条件下枷3罐中4批发酵显示出很强的发酵能力，平均醇酸转化率较对照提高8.16个百分点，周期缩短10.6小时。其在300M3罐中生产试用行，连续26批次的平均醇酸转化率达87.40%,较生产用菌提高3.32个百分点。平均周期也缩短1．3小时。

高电荷态离子Arq+与Nb作用产生的X射线谱

利用光谱技术在超导离子源SECRAL上研究了10~20keV·q的Arq+(q=16,17)离子入射在金属Nb表面产生的X射线谱.实验结果表明,高电荷态Ar16+离子在金属表面中性化过程中存在着多电子激发,Ar16+的K壳层电子被激发产生空穴,级联退激发射Ar的Kα特征X射线.Ar空心原子的K层发射X射线的强度随入射离子的动能减弱,靶原子Nb的L层发射X射线强度随入射离子动能的增加而增强.Ar17+单离子的Kα-X射线产额比Ar16+单离子的Kα-X射线产额大3个数量级.

高电荷态离子Ar~(q+)与Nb作用产生的X射线谱

利用光谱技术在超导离子源SECRAL上研究了10~20keV·q的Arq+(q=16,17)离子入射在金属Nb表面产生的X射线谱.实验结果表明,高电荷态Ar16+离子在金属表面中性化过程中存在着多电子激发,Ar16+的K壳层电子被激发产生空穴,级联退激发射Ar的Kα特征X射线.Ar空心原子的K层发射X射线的强度随入射离子的动能减弱,靶原子Nb的L层发射X射线强度随入射离子动能的增加而增强.Ar17+单离子的Kα-X射线产额比Ar16+单离子的Kα-X射线产额大3个数量级.

~(129)Xe~(q+)入射金属表面激发的X射线谱

用高电荷态离子129Xeq+(q=25,26,27)轰击金属Au表面,产生Au原子的特征X射线谱.实验结果表明,足够高的电荷态低速离子激发靶表面原子,无需很强的束流强度(nA量级),便可有效地产生重原子的特征X谱线(Au,Mα),单离子X射线产额可达10-8量级,特征X射线的产额随入射离子的动能和势能(电荷态)的增加而增加.通过Au原子Mα的特征X射线谱,利用Heisenberg不确定关系对Au原子的第N能级寿命进行了估算.

高电荷态离子~(40)Ar~(q+)与Au表面作用产生的X射线谱

利用光谱技术研究了高电荷态离子40Arq+(q=16,17,18)离子入射金属Au表面产生的X射线谱.分析结果表明,Ar的Kα-X射线是离子在与固体表面相互作用过程中在固体表面之下形成的空心原子发射的.当电子组态为1s2的高电荷态Ar16+离子在金属表面中性化过程中,存在着多电子激发过程使Ar16+的K壳层电子激发产生空穴,进而级联退激发射Ar的Kα特征X射线.入射离子的Kα-X射线产额与其最初的电子组态有关,靶原子的X射线产额与入射离子的动能有关.

Measurement of the inelastic branch of the O-14(alpha, p)F-17 reaction: Implications for explosive burning in novae and x-ray bursters

A measurement of the inelastic component of the key astrophysical resonance in the 14O(α,p)17F reaction for burning and breakout from hot carbon-nitrogen-oxygen (CNO) cycles is reported. The inelastic component is found to be comparable to the ground-state branch and will enhance the 14O(α,p)17F reaction rate. The current results for the reaction rate confirm that the 14O(α,p)17F reaction is unlikely to contribute substantially to burning and breakout from the CNO cycles under novae conditions. The reaction can, however, contribute strongly to the breakout from the hot CNO cycles under the more extreme conditions found in x-ray bursters.

Kinetic energy and charge state effects in the X-ray emission of Mo surface induced by Xeq+ (q=25, 29) ions

L-shell X-ray spectra of Mo surface induced by Xe25+ and Xe29+ were measured. The X-ray intensity was obtained in the kinetic energy range of the incident ions from 350 to 600 keV. The relationship of X-ray intensity with kinetic energy of the projectile and its charge state were studied, and the simple explanation was given.

X-ray spectra induced by slow highly charged Arq+ ions in collision with Nb surface

The X-ray spectra of Nb surface induced by Arq+ (q = 16,17) ions with the energy range from 10 to 20 keV/q were studied by the optical spectrum technology. The experimental results indicate that the multi-electron excitation occurred as a highly charged Ar16+ ion was neutralized below the metal surface. The K shell electron of Ar16+ was excited and then de-excited cascadly to emit K X-ray. The intensity of the X-ray emitted from K shell of the hollow Ar atom decreased with the increase of projectile kinetic energy. The intensity of the X-ray emitted from L shell of the target atom Nb increased with the increase of projectile kinetic energy. The X-ray yield of Ar17+ is three magnitude orders larger than that of Ar16+.

X-ray spectra induced by Xe-129(q+) impacting the metal surface

Using the slow highly charged ions Xe-129(q+) (q = 25, 26, 27; initial kinetic T-0 <= 4.65 keV/a.u.) to impact Au surface, the Au atomic M alpha characteristic X-ray spectrum is induced. The result shows that as long as the charge state of projectile is high enough, the heavy atomic characteristic X-ray can be effectively excited even though the incident beam is very weak (nA magnitude), and the X-ray yield per ion is in the order of 10(-8) and increases with the kinetic energy and potential energy of projectile. By measuring the Au M alpha-X-ray spectra, Au atomic N-level lifetime is estimated at about 1.33x10(-18) s based on Heisenberg uncertainty relation.

X-ray spectra induced in highly charged Ar-40(q+) interacting with Au surface

By use of optical spectrum technology, the spectra of X-ray induced by highly charged Ar-40(q+) ions interacting with Au surface have been studied. The results show that the argon K alpha X-ray were emitted from the hollow atoms formed below the surface. There is a process of multi-electron exciting in neutralization of the Ar16+ ion, with electronic configuration 1s(2) in its ground state below the solid surface. The yield of the projectile K alpha X-ray is related to its initial electronic configuration, and the yield of the target X-ray is related to the projectile kinetic energy.