射频反应性溅射沉积的Cd2SnO4薄膜物理性质与缺陷特性研究

在Ar+O₂混合气氛中射频反应性溅射Cd-Sn合金靶制备了透明导电Cd₂SnO₄(简称CTO)薄膜。用X射线衍射测量了CTO膜的结构。实验结果表明,这种薄膜的电学和光学性质依赖于混合气体中的氧浓度、衬底温度以及沉积后的热处理。获得的CTO膜最低电阻率为1.74×10^-6Ω·cm,可见光光谱区最高透射率为95％。对于氧浓度为6％、衬底温度为400℃时沉积的CTO膜,经热处理后,其光隙能由热处理前的2.37eV增大为2.6 关键词：     

合成温度和N2/O2流量比对碳纤维衬底上生长的SnO2纳米线形貌及场发射性能影响

采用化学气相沉积法系统研究了合成温度和N₂/O₂流量对生长在碳纤维衬底上的SnO₂纳米线形貌及场发射性能的影响规律. 利用扫描电镜(SEM)、透射电镜(TEM), X射线衍射(XRD)及能谱仪(EDS)对产物细致表征, 结果表明, SnO₂纳米线长径比随反应温度的升高而增大; 随N₂/O₂流量比值的增大先增大后变小, 场发射测试表明, 合成温度780 ℃, N₂/O₂流量比为300 : 3 时SnO₂纳米线阵列具有最佳的场发射性能, 开启电场为1.03 V/μm, 场强增加到1.68 V/μm时, 发射电流密度达0.66 mA/cm², 亮度约2300 cd/m².     

大气等离子体中氮氧化物粒子行为的数值模拟

利用一个空间零维大气等离子体模型对其中的氮氧化物在不同电离度情况下的变化规律进行了数值模拟,得到了放电后不同初始电子密度下的氮氧化物(包括NO,NO⁺,NO₂,NO₂⁺,N₂O,N₂O⁺,NO₃和N₂O₅)及影响其产消的主要反应物N和O₃的密度随时间的演化规律.结果表明,电子初始密度n_e0=10⁹ cm^-3时,NO和NO₂的去除率较高,氮氧化物总密度较小,最适合消除氮氧化物污染.同时,还对N和O₃随电离度变化的行为进行了分析. 关键词： 大气等离子体 氮氧化物 电离度 数值模拟     

前驱体和退火温度对Nd2O3薄膜组分影响的定量研究

采用Nd(thd)₃和O₃作为反应前驱体, 利用先进的原子层淀积方法在P型硅(100)衬底上制备了超薄Nd₂O₃介质膜, 并在N₂气氛下进行了退火处理. 采用X射线光电子能谱仪对薄膜样品组分进行分析. 研究结果表明, 淀积过程中将前驱体温度从175 ℃提高到185 ℃后, 薄膜的质量得到提高, O/Nd 原子比达到1.82, 更接近理想的化学计量比, 介电常数也从6.85升高到10.32.     

采用详细化学反应机理研究煤富氧燃烧NO_x生成机制

本文采用详细化学反应机理,建立氧煤燃烧气固反应模型,分析煤在富氧燃烧条件下NO_x生成机制,研究不同O₂浓度和分级燃烧对NO_x排放的影响。富氧燃烧时,NO_x生成主要路径为:HCN→CN→NCO→NO和HCN→CN→NCO→HNCO→HN₂→NH→HNO→NO。初始O₂增大,挥发分和HCN析出时间提前,高的O₂初始浓度对燃料N转化率有促进作用;煤富氧分级燃烧时,主燃区还原气氛有利于NO还原为N₂,其主要还原路径如下:NO+CO→N+CO₂、NO+H→N+OH和NO+N→N₂+O,当主燃区过量空气系数SR₁从1.15减小到0.6,N最终转化率（t=1000 ms）只是从0.379减小到0.339,相对于未分级燃烧时变化了10.55%,与煤空气分级燃烧相比,煤富氧分级燃烧对N转化率影响较小。     

碰撞诱导离解(CID)(Ⅱ)——I2(B3∏o+u)在高振动态(v′=62)的碰撞猝灭机理实验研究

本文研究了B³∏_o+u激发态I₂分子在高振动态v′=62时的碰撞猝灭过程。实验中得到了该能级I₂分子和其自身以及与其他气体分子(He,Ar,Kr,H₂,CO,N₂,O₂,CH₄,NH₃,C₂H₆,CCl₄)的碰撞猝灭速率常数,并且发现,在I关键词：     

Co1-xNixSb3-ySey热电输运中晶界和点缺陷的耦合散射效应

结合机械合金化与放电等离子烧结工艺制备了Ni和Se共掺的细晶方钴矿化合物Co_1-xNi_xSb_3-ySe_y,研究了晶界和点缺陷的耦合散射效应对CoSb₃热电输运特性的影响.通过Ni掺杂优化载流子浓度提高功率因子.在x=0.1时,功率因子达到最大值1750μWm^-1K^-2(450℃),是没有掺Ni试样的两倍.晶界和点缺陷的耦合散射机理使晶格热导率急剧下降,其中Co_0.9Ni_0.1Sb_2.85Se_0.15的室温晶格热导率降低至1.67Wm^-1K^-1,接近目前单填充效应所能达到的最低值1.6Wm^-1K^-1,其热电优值ZT在450℃时达到最大值0.53.将Callaway-Von Baeyer点缺陷散射模型嵌入到Nan-Birringer有效介质理论模型,对晶界散射和点缺陷散射的耦合效应对热导率的影响进行了定量分析,模型计算与实验结果符合.理论模型计算表明,当晶粒尺寸下降到50nm同时掺杂引入点缺陷散射后,Co_0.9Ni_0.1Sb_2.85Se_0.15的晶格热导率下降到0.8Wm^-1K^-1. 关键词： 3')" href="#">CoSb₃ Ni和Se掺杂 热电性能 耦合散射效应     

Ni/Au与N掺杂p型ZnO的欧姆接触

研究了Au,In,Ni/Au三种不同金属膜与N掺杂p型ZnO的接触特性,发现Ni/Au双层膜更适合作为其欧姆电极材料,并比较了不同气氛和不同温度退火对Ni/Au电极的影响.发现在O₂中退火电极性能发生蜕变,而在N₂中退火性能得到改善.指出即使在N₂中退火,退火温度的选择也是至关重要的,本实验在400℃,氮气气氛下退火150s,得到了较好的欧姆接触特性.     

Ca$lt;sub$gt;2$lt;/sub$gt;Si（O$lt;sub$gt;4-$lt;i$gt;x$lt;/i$gt;$lt;/sub$gt;N$lt;sub$gt;$lt;i$gt;x$lt;/i$gt;$lt;/sub$gt;）：Eu$lt;sup$gt;2+$lt;/sup$gt;绿色荧光粉的制备及其发光性能

利用在Ca-Si-O干凝胶前驱体中添加Si₃N₄的方法于非还原气氛下合成了含N固溶体Ca₂Si（O_4-xN_x）：Eu²⁺绿色荧光粉. 通过X射线衍射仪、扫描电子显微镜以及荧光分光光度计分别分析了产物的物相结构、颗粒形貌和发光性能. 结果显示,Si₃N₄与前驱体的混合物在非还原气氛（纯氮气）下于1100℃焙烧后获得含N固溶体Ca₂Si（O_4-xN_x）：Eu²⁺荧光粉,特别是其中Eu³⁺被还原为Eu²⁺,产物的晶体结构与βup -Ca₂SiO₄相一致. Ca₂Si（O_4-xN_x）：Eu²⁺能够被270–400 nm 范围内的紫外线有效激发,其发射光谱呈宽带发射. 随着N含量的增加,发射峰出现一定程度红移（501–504 nm）,而且发光强度显著提高. 当Eu²⁺浓度为0.25 mol%时发光强度达最大值,浓度超过0.25 mol%时,发光强度显著降低,出现浓度猝灭 效应. 关键词： 白光LED 荧光粉 溶胶凝胶法 3N₄')" href="#">Si₃N₄     

Zr4+掺杂对Er3+/Yb3+共掺NaYF4微晶晶相和发光性能的影响

采用油酸辅助的水热法制备了Er³⁺/Yb³⁺共掺NaYF₄微晶,通过在反应体系中引入Zr⁴⁺离子,实现了NaYF₄微晶的晶相控制和上转换发光增强。X-射线衍射和扫描电镜结果表明：Zr⁴⁺离子的引入能够明显加快立方相α-NaYF₄向六方相β-NaYF₄的相转变过程。当Zr⁴⁺离子的引入摩尔分数为5%时,获得了纯的六方相β-NaYF₄微晶。Er³⁺/Yb³⁺共掺NaYF₄微晶在980 nm激光泵浦下,观察到强的上转换绿光和红光发射,且上转换发光强度随着Zr⁴⁺离子添加量的增加逐渐增大。     

Search for narrow p¯p resonances in the reaction p¯p → p¯pπ+π−.

The reaction p¯p → p¯pπ⁺π^?. has been studied with high statistics at CERN-LEAR with incident p¯ momenta from 1.65 to 2.0 GeV/c by the JETSET (PS202) experiment. The aim of this paper is to search for narrow resonances decaying to p¯p. No evidence for such structures is found. In particular, an upper limit for the production of a 2.02 GeV state with a width of Γ = 20 MeV, having been seen in other hadroproduction experiments, is established. Our results restrict the cross section for such a peak to be below 200 nb at the 95% confidence level.     

A study of the reactions γp→ωp and γp→ωp and γp→ωΔ+

The differential and total corss sections and the decay density matrix elements have been measured for the reactions, γp→ωp and γp→ωΔ⁺ (1232) in the photon energy range 2.8 to 4.8 GeV. The total cross sections for ωΔ⁺ (1232) photo-production are found to be slightly larger than those for elastic ω photo-production in this energy range. The data are compared to the predictions of a theoretical model and the contributing exchange mechanics are discussed.     

Multiplicity distributions in the reaction p+p→p+ anything

It is shown that, for fixed mass of the system X, the charged particle multiplicity distribution in the reaction p+p→p+X is remarkably similar to the shape of the multiplicity distribution for the reaction p+p→ anything observed at an equivalent fixed center of mass energy.     

A study of the reaction p + p → p + p + X at ISR energies

We have performed an experiment to investigate the reaction p + p → p₁ + p₂ + X at the CERN Intersecting Storage Rings (ISR). The dependence of the cross-section on the mass and rapidity of the system X, and on the momentum transfer squared t₁, t₂ to the outgoing protons is studied. We observe signals for the production of ?, ω, f, and A₂ mesons in the missing-mass spectra, and conclusions are made about the contribution of double-Pomeron exchange.     

Neutral kaon production in p+p and p+Nb collisions

The kaon nucleus (KN) interaction in dense nuclear matter is predicted to be repulsive and increasing with density. However, determined values for this potential are not yet consistent with each other (Benabderrahmane et al., Phys Rev Lett 102:182501, 2009; Agakishiev et?al., Phys Rev C 82:044907, 2010; Büscher et?al., Eur Phys J A 22:301–317, 2004). We analyze $K^0_S$ mesons identified with the HADES detector in p+p and p+?⁹³Nb reactions at 3.5?GeV kinetic beam energy. To determine the KN potential at normal nuclear density we propose to compare the $K^0_S$ differential distributions in p+?⁹³Nb and p+p collisions. High statistics of low p _t -kaons (p _t ?<?100?MeV/c) ensure the sensitivity of our measurements to the nuclear matter effects. We present the data analysis method and first results.     

Studies in\bar p p annihilation

Evidence is presented that \(\bar p\) p annihilation proceeds via the formation of two jets, with average transverse momentum of the order of the nucleon mass. The implications of this behaviour is linked to the measured cross sections and multiplicities, and explanations for it have been sought in the underlying gluon and quark constituents of the \(\bar p\) p system. The confrontation of the suggested constituent mechanisms and experimental data lead to the concept that charm meson production may play a significant role in the \(\bar p\) p experiments at the highest available energies.     

Suppression of the Coulomb interaction in the off-energy-shell p - p scattering from the p + d --> p + p + n reaction

Off-energy-shell effects in p - p scattering have been investigated at p - p relative energies from 600 down to 80 keV applying the Trojan horse method (THM) to the p + d --> p + p + n reaction at 5 MeV. In contrast with the on-energy-shell case, no Coulomb-nuclear interference minimum has been found in the extracted THM p - p cross section, due to the suppression of the Coulomb amplitude as predicted by the half-off-energy shell calculations. This hypothesis is strengthened by the agreement between THM p - p data and calculated on-energy-shell n + n, n + p and nuclear p + p cross sections.     

Comparing the p̅p → K − K + and p̅p → π−π+ reactions

A partial wave amplitude analysis of LEAR data on differential cross sections and analyzing powers of p?p → K ^? K ⁺ has been performed in the range p _lab = 360 ? 1000 MeV/c, and compared to the results from the same observables for p?p → π^?π⁺. Contrary to other analyses we see no compelling evidence of resonance behavior in our amplitudes. However, as we discuss, the resulting amplitudes are not unique since a third observable remains to be measured for both reactions. Another remarkable result is that for p?p → K ^? K ⁺ all our solutions in the momentum interval below 900 MeV/c, only partial wave amplitudes including J _max = 2 are necessary. This upper limit on the angular momentum is smaller than J _max = 3 which is required for the data of the reaction p?p → π^?π⁺ in the same momentum interval. This finding is consistent with a model analysis for data above 1 GeV/c. Annihilation models with short range baryon exchange give too small J ≥ 2 amplitudes and final state ππ and K?K interactions are presumably very important.