87 resultados para Al_2O_3


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Eu~(2+)4f~7组态内f→f跃迁发射有可能实现激光振荡,Eu~(2+)激活并可产生锐峰发射的若干晶体,储能高、阈值低,是有前景的短波可见固体激光材料的后备物。 Eu~(2+)实现f→f跃迁发射的条件是4f~65d吸收下限位于~6P_l能级之上。符合这一条件的基质化合物必须满足若干结晶学和光谱学条件。为此,许多作者从不同角度建立了相关的判

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Co-Mo 系催化剂由于其优越的耐硫性能和对水煤气变换反应的高活性,因此在制氢工业中日益得到重视。已知 Co-Mo-K/Al_2O_3催化剂是一种优良的水煤气变换催化剂,该催化剂在使用前须经硫化。实际上催化剂在反应时

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为了排除和减小电极与熔体接触面间的阻抗,电极与连接导线的电阻以及石英电导池腐蚀的影响,本文用交流四电极法测量了熔体Na_3Na_3AlF_6-Al_3O_3-RE_2O_3的电导率,其中RE指以Ce为主的混合稀土。 实验装置如图1所示,电极为φ0.8mm的Pt和Pt-Rh丝(其中二根Pt、二根Pt-Rh),中

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Micro-fracture toughness in one nanoceramic composite, Al_2O_3/SiC_{nano}, is measured by Nanoindentation tests. Microscopy is adopted to probe that all nanoindentations are local at Al_2O_3, matrix component of the current composite and measure length of radial micro-cracks at corriers of nanoindentation. The measured fracture toughness at the shallow indentation is higher than those at deeper ones. Relations between micro-toughness and peak loads as well as peak depths are discussed. And an analysis to the energy consumed during the indentation and fracture toughness explained that, the lower fracture toughness measured in the deeper impression probably resulted from its fracture modes yielded by higher load and larger depth.

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热浸镀铝钢材在铝铁界面处易产成FeAl冶金结合层。本文就FeAl层对铝镀层等离子体电解氧化(PEO)陶瓷层的表面形貌、截面组织、相结构和元素分布的影响进行了研究。结果表明:由于FeAl参与,PEO陶瓷层局部区域出现了50μm~80μm的贯穿性孔洞,在孔洞/FeAl界面处出现了许多微观裂纹。EDS结果显示孔洞周围的Fe、Na元素含量增高了近8倍。陶瓷层主要由γ-Al_2O_3、莫来石相、α-Al_2O_3和Fe_3O_4相组成。与FeAl层相比,PEO陶瓷层具有较高的硬度和塑性变形能力。

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采用纳米压入方法表征了热浸镀铝钢表面由Al_2O_3层、Al层和FeAl层组成的复合涂层的纳米硬度、弹性模量及断裂韧性等微观力学性能,采用扫描电镜(SEM)观察了纳米压痕形貌,并分析了孔洞对陶瓷层的纳米压入行为和压痕裂纹扩展的影响.结果表明:等离子体电解氧化(PEO)陶瓷层中包含许多微米和亚微米尺度的细小孔洞,陶瓷层弹性模量约为226.4 GPa,纳米硬度约为19.6 GPa.当纳米压入深度为250 nm时,所测得陶瓷层的力学参数分散性较大.与FeAl层比较,PEO陶瓷层具有较高的裂纹扩展阻力.FeAl层纳米压痕顶端产生了沿直线扩展的径向裂纹;而陶瓷层纳米压痕中除径向裂纹外出现了侧边裂纹.

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利用阳极化处理的铝板做激光能量计的探测元件是一条较好的途径。本文对CO_2激光辐照下铝板上的Al_2O_3膜的特性参数,取得了一些有益的结果。

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采用公共阳极法实现了Pyrex玻璃与铝多层晶片的静电键合,对玻璃/铝/玻璃阳极接合界面的组织结构及其连接机理和力学特征进行了重点研究。分别利用微拉伸测试设备和ANSYS软件分析了连接区的力学性能和残余应力分布特征。分析认为键合区由玻璃-过渡层-铝组成,过渡层为Al_2O_3-SiO_2复合氧化物。玻璃/铝界面的微观组织和元素分布均以铝为对称轴呈对称分布。在玻璃/铝/玻璃多层连接区,键合界面附近的残余应力和应变呈对称分布,多层结构的对称性有利于缓解接头应变和应力,表明应用公共阳极法可实现多层玻璃/铝/玻璃的良好键合。

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热浸镀铝钢经等离子体电解氧化(Plasma Electrolytic Oxidation,PEO)处理后,表面铝镀层转化为陶瓷层.实验对阳极电压变化、陶瓷层生长规律、涂层截面形貌和成分等进行了研究.结果表明:在PEO初期,热浸铝试件的阳极电压变化趋势与纯铝试件相同,在PEO后期电压有下降趋势.铝镀层消耗和陶瓷层厚度增长近似为线性变化.当铝镀层完全陶瓷化后,FeAl层参与PEO反应,但陶瓷层生长速率变慢,在界面处出现大量裂纹;陶瓷层主要成分为Al、Si、O元素,相结构主要为γ-Al_2O_3与莫来石相,在PEO后期出现α-Al_2O_3相.复合陶瓷层硬度呈区域性分布,陶瓷层最高硬度可达HV1800.

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采用等离子体电解氧化技术在铝硅合金表面制备了陶瓷层,电解液为磷酸盐系列。利用轮廓仪、SEM和XRD对陶瓷层的粗糙度、形貌和相组成进行了研究。结果表明,PEO处理过程可分为4个典型阶段。随处理时间延长,陶瓷层的厚度近似线性增长,表面缺陷增大增多,粗糙度显著增加,达到9.5μm。PEO处理初期只生成γ-Al_2O_3,一定时间后α-Al_2O_3出现,其相对含量逐渐增多.

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本文针对发展新一代步兵战车复合材料履带板所面临的关键问题,结合其实际受载特点,设计制备了冲击疲劳实验加载装置,并着重从实验设计及机理分析上进行细致深入的探索,揭示了Al_2O_3/LC_4复合材料冲击疲劳破坏的微观过程和机理。首先分别对SiC_P/LC_4、Al_2O_(3P)/LC_4 及基体 LC_4 进行了显微组织的观察与定量分析,并对其拉伸、三点弯曲破坏过程进行了在位观察,结合其断裂形貌的观察与分析,揭示出颗粒增强铝基复合材料断裂破坏的根本原因是颗粒的聚集及脆性相在晶界的严重偏聚。针对这一结论,给材料制备单位提出工艺改进意见。对工艺改进后制备的复合材料进行常规力学性能的测试,结果表明,其拉伸性能明显优于改进前制备的相应材料。为了进行冲击疲劳的实验研究,在分析步兵战车履带板实际受载特点的基础上,自行设计制备了冲击疲劳实验的加载装置。主要包括主体框架和测量系统,前者与小型振动系统配合使用可以实现冲击能量为 0.3J、冲击频率为 1Hz、冲击速度为 0.6m/s 的多次冲击实验;后者可以准确记录下任意时刻的冲击载荷波形及冲击疲劳载荷的循环数。为了考察颗粒与加载速率对复合材料疲劳机理的影响,实验研究了 Al_2O_3/LC_4 复合材料和 LC_4 纯基体材料在冲击疲劳和常规疲劳过程中裂纹的扩展过程及扩展速率。综合结果发现:与LC_4纯基体材料相比,Al_2O_3/LC_4复合材料疲劳裂纹扩展得更为迅速。复合材料中,由于颗粒的加入,两种疲劳方式下袭纹都发生严重偏转;裂纹经过颗粒时,多数是绕过,少数是切过颗粒;冲击疲劳裂纹扩展速率明显高于常规疲劳裂纹扩展速率。纯基体材料中,两种加载方式下,裂纹基本都以穿晶的方式扩展,裂纹常常表现为小锯齿状;冲击疲劳裂纹尖端的塑性变形程度比常规疲劳更大;冲击疲劳裂纹比常规疲劳裂纹更曲折,表现出多尺度的锯齿状(Zig-Zag)特征;冲击疲劳裂纹扩展速率高于常规疲劳的裂纹扩展速率。在基本实验的基础上,进一步对断口及裂纹扩展途径进行了微观观察和定量分析,最后综合全文的实验和统计结果,讨论了颗粒增强铝基复合材料的冲击疲劳机理。复合材料疲劳裂纹扩展速率的提高主要与裂纹的偏转有关,裂纹更倾向于沿着颗粒与基体的界面扩展;两种材料的疲劳裂纹扩展速率均随加载速率的增加而增加,呈现加载速率的反作用。加载方式的改变,一方面,由于冲击情况下载荷持续时间降低,使裂纹扩展速率降低;另一方面,加载速率的提高使得断裂韧性值降低,材料变脆,裂纹扩展速率升高。这两个方面相互影响,相互竞争,决定实际的裂纹扩展速率。两种材料中,不同加载速率下的疲劳裂纹扩展的微观机制基本一致,没有明显的本质区别。

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To explain the ^(26)Mg isotopic anomaly seen in meteorites (^(26)Al daughter) as well as the observation of 1809-keV γ rays in the interstellar medium (live decay of 26Al) one must know, among other things, the destruction rate of ^(26)Al. Properties of states in ^(27)Si just above the ^(26)Al + p mass were investigated to determine the destruction rate of ^(26)Al via the ^(26)Al(p,γ)^(27)Si reaction at astrophysical temperatures.

Twenty micrograms of ^(26)Al were used to produce two types of Al_2O_3 targets by evaporation of the oxide. One was onto a thick platinum backing suitable for (p,γ) work, and the other onto a thin carbon foil for the (^3He,d) reaction.

The ^(26)Al(p,γ)^(27)Si excitation function, obtained using a germanium detector and voltage-ramped target, confirmed known resonances and revealed new ones at 770, 847, 876, 917, and 928 keV. Possible resonances below the lowest observed one at E_p = 286 keV were investigated using the ^(26)Al(^3He,d)^(27)Si proton-transfer reaction. States in 27Si corresponding to 196- and 286-keV proton resonances were observed. A possible resonance at 130 keV (postulated in prior work) was shown to have a strength of wγ less than 0.02 µeV.

By arranging four large Nal detector as a 47π calorimeter, the 196-keV proton resonance, and one at 247 keV, were observed directly, having wγ = 55± 9 and 10 ± 5 µeV, respectively.

Large uncertainties in the reaction rate have been reduced. At novae temperatures, the rate is about 100 times faster than that used in recent model calculations, casting some doubt on novae production of galactic ^(26)Al.

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Secondary-ion mass spectrometry (SIMS), electron probe analysis (EPMA), analytical scanning electron microscopy (SEM) and infrared (IR) spectroscopy were used to determine the chemical composition and the mineralogy of sub-micrometer inclusions in cubic diamonds and in overgrowths (coats) on octahedral diamonds from Zaire, Botswana, and some unknown localities.

The inclusions are sub-micrometer in size. The typical diameter encountered during transmission electron microscope (TEM) examination was 0.1-0.5 µm. The micro-inclusions are sub-rounded and their shape is crystallographically controlled by the diamond. Normally they are not associated with cracks or dislocations and appear to be well isolated within the diamond matrix. The number density of inclusions is highly variable on any scale and may reach 10^(11) inclusions/cm^3 in the most densely populated zones. The total concentration of metal oxides in the diamonds varies between 20 and 1270 ppm (by weight).

SIMS analysis yields the average composition of about 100 inclusions contained in the sputtered volume. Comparison of analyses of different volumes of an individual diamond show roughly uniform composition (typically ±10% relative). The variation among the average compositions of different diamonds is somewhat greater (typically ±30%). Nevertheless, all diamonds exhibit similar characteristics, being rich in water, carbonate, SiO_2, and K_2O, and depleted in MgO. The composition of micro-inclusions in most diamonds vary within the following ranges: SiO_2, 30-53%; K_2O, 12-30%; CaO, 8-19%; FeO, 6-11%; Al_2O_3, 3-6%; MgO, 2-6%; TiO_2, 2-4%; Na_2O, 1-5%; P_2O_5, 1-4%; and Cl, 1-3%. In addition, BaO, 1-4%; SrO, 0.7-1.5%; La_2O_3, 0.1-0.3%; Ce_2O_3, 0.3-0.5%; smaller amounts of other rare-earth elements (REE), as well as Mn, Th, and U were also detected by instrumental neutron activation analysis (INAA). Mg/(Fe+Mg), 0.40-0.62 is low compared with other mantle derived phases; K/ AI ratios of 2-7 are very high, and the chondrite-normalized Ce/Eu ratios of 10-21 are also high, indicating extremely fractionated REE patterns.

SEM analyses indicate that individual inclusions within a single diamond are roughly of similar composition. The average composition of individual inclusions as measured with the SEM is similar to that measured by SIMS. Compositional variations revealed by the SEM are larger than those detected by SIMS and indicate a small variability in the composition of individual inclusions. No compositions of individual inclusions were determined that might correspond to mono-mineralic inclusions.

IR spectra of inclusion- bearing zones exhibit characteristic absorption due to: (1) pure diamonds, (2) nitrogen and hydrogen in the diamond matrix; and (3) mineral phases in the micro-inclusions. Nitrogen concentrations of 500-1100 ppm, typical of the micro-inclusion-bearing zones, are higher than the average nitrogen content of diamonds. Only type IaA centers were detected by IR. A yellow coloration may indicate small concentration of type IB centers.

The absorption due to the micro-inclusions in all diamonds produces similar spectra and indicates the presence of hydrated sheet silicates (most likely, Fe-rich clay minerals), carbonates (most likely calcite), and apatite. Small quantities of molecular CO_2 are also present in most diamonds. Water is probably associated with the silicates but the possibility of its presence as a fluid phase cannot be excluded. Characteristic lines of olivine, pyroxene and garnet were not detected and these phases cannot be significant components of the inclusions. Preliminary quantification of the IR data suggests that water and carbonate account for, on average, 20-40 wt% of the micro-inclusions.

The composition and mineralogy of the micro-inclusions are completely different from those of the more common, larger inclusions of the peridotitic or eclogitic assemblages. Their bulk composition resembles that of potassic magmas, such as kimberlites and lamproites, but is enriched in H_2O, CO_3, K_2O, and incompatible elements, and depleted in MgO.

It is suggested that the composition of the micro-inclusions represents a volatile-rich fluid or a melt trapped by the diamond during its growth. The high content of K, Na, P, and incompatible elements suggests that the trapped material found in the micro-inclusions may represent an effective metasomatizing agent. It may also be possible that fluids of similar composition are responsible for the extreme enrichment of incompatible elements documented in garnet and pyroxene inclusions in diamonds.

The origin of the fluid trapped in the micro-inclusions is still uncertain. It may have been formed by incipient melting of a highly metasomatized mantle rocks. More likely, it is the result of fractional crystallization of a potassic parental magma at depth. In either case, the micro-inclusions document the presence of highly potassic fluids or melts at depths corresponding to the diamond stability field in the upper mantle. The phases presently identified in the inclusions are believed to be the result of closed system reactions at lower pressures.

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用热蒸发方法沉积了薄膜滤光片.并将样品分别在去离子水中浸泡10天和30天.通过分光光度计、光学暗场显微镜、及扫描电子显微镜等多种测试手段,对诱导透射滤光片在潮湿环境下的稳定性进行了研究.实验发现,在潮湿环境下滤光片产生的膜层分离都是从薄膜中微缺陷点处开始发生和发展的,微缺陷是影响滤光片环境稳定性的重要原因之一,其中杂质和针孔是滤光片中两种最常见的微缺陷.EDS能谱分析进一步表明,薄膜中杂质缺陷成分即为Al2O3膜料本身,所以不能推测,薄膜沉积中的喷溅可能是微缺陷产生的根本原因,抑制喷溅可以有效提高薄膜滤光

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Pt-Sn/A1_2O_3负载型双金属催化剂由于其独特的催化性能而被广泛应地用于催化重整工业当中。尽管它对于长链烷烃的脱氢取得较为理想的效果,但用于异丁烷等小分子脱氢却不够理想。Pt-Sn/Al_2O_3负载型双金属催化剂用于异丁烷脱氢,其初活性较高,但对异丁烯的选择性较低,且稳定性较差,易失活。本研究工作就是以Pt-Sn/Al_2O_3负载型双金属催化剂为基础,通过添加碱金属、稀土元素来调变其脱氢性能,一方面提高催化剂的稳定性,另一方面提高对异丁烯的选择性。本文所需要的所有催化剂均是应用传统的共浸法制得。我们首先研究了经碱金属调变的催化剂的脱氢性能。我们发现加入碱金属,尽管催化剂的初活性略有降低,但催化剂对异丁烯的选择性却明显升高,其抗积炭性能也有显著提高。在这三种碱金属当中,K的调变效果最好。我们借助于现代化的测试手段(XRD、XPS、TPR、DTA-TG)对催化剂及其积炭样品进行了表征。结果表明,所有金属组分均以高分散状态存在于载体之上,碱金属钾的加入并没有将离子态的锡还原为金属态。由于K~+是很强的电子施主,它能够减缓活性中心铂的缺电子状态(由于载体效应的存在,铂受载体的拉动效应,它往往以不同程度缺电子状态存在),从而减缓了活性中心与烃类之间的相互作用,有利于抑制积炭的产生。我们应用DTA-TG研究催化剂的积炭样品发现,碱金属能够抑制了烃类的深度脱氢。碱金属还中和了载体表面的酸性中心,这既抑制了异构化等副反应的发生,提高了对异丁烯的选择性,又抑制了积炭反应的发生。稀土元素对Pt-Sn - K/Al_2O_3催化剂的影响比较复杂。在种稀土元素当中(La、Ce、Pr、Nd、Sm、Eu),Sm、Ce的调变效果较好,而Eu的调变效果最差。钐的载量不宜太多,以0.30%为宜,太多,一方面有可能将离子态的锡还原成金属态而使催化剂失活,另一方面可能会导致载体晶型有所改变而影响金属组分与载体间的相互作用。TPR结果表明,稀土元素对催化剂的强弱吸附中心的影响是不同的。弱中心上,它作为受电子体,使得铂的缺电子状态加剧,削弱了活性中心与载体之间的相互作用;在强吸附中心上,稀土元素是给电子体,减缓了活性中心铂的缺电子状态,增强了其与载体的相互作用,这两方面共同作用的结果,增强了催化剂的抗积炭能力,提高了催化剂的稳定性。由于铟与锡属于同一周期,且在周期表中处于相临的位置,因此我们考察了铟的不同载量对Pt-In/A1_2O_3催化剂脱氢性能的影响。铟载量跟锡载量相同的情况下,Pt-Sn/Al_2O_3催化剂的活性要比Pt-Sn/Al_2O_3催化剂的活性高,但其对异丁烯的选择性和抗积炭能力却要比Pt-Sn/Al_2O_3催化剂差。另外,随着铟载量的逐渐增加,催化剂的活性逐渐下降,对异丁烯的选择性逐渐升高,异构化逐渐降低。这说明铟在催化剂中起了两方面的作用。首先,它能中和载体表面的酸性中心,再者,对铂活性中心起着一种电子效应。另外我们还考察了碱金属钾对Pt-In/Al_2O_3催化剂的调变作用