146 resultados para MG-RAST


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利用金属型铸造制备了Mg-5Al-0.3Mn-xRE (x = 0~4, wt%,RE = Ce, Nd, Sm, Y和(CeLa)混合稀土)系列合金,研究了铸态合金的组织和力学性能。利用轧制和挤压技术对优化出的合金进行了变形加工处理,并研究了合金加工后的组织和力学性能。 对于铸态合金,稀土元素不仅可以细化合金的晶粒,而且形成不同类型的Al-RE化合物,含Ce的合金中生成Al11Ce3相,含Nd或Sm的合金中,主要生成Al11Nd3 (Al11Sm3)相和少量的Al2Nd (Al2Sm)相,含Y的合金中生成Al2Y相。另外,添加稀土可以改变Mg17Al12相的形貌,使其变得更加细小、弥散。添加适量的稀土可以明显提高铸态合金在室温和150℃下的力学性能,Mg-5Al-0.3Mn-1.5Ce, Mg-5Al-0.3Mn-2Nd和Mg-5Al-0.3Mn-2Sm合金在各自的体系中具有最佳的综合力学性能。合金力学性能提高的主要原因是细晶强化、Al-RE化合物第二相强化以及减弱Mg17Al12相对合金高温力学性能的不利影响。 对Mg-5Al-0.3Mn-(1.0, 1.5, 2.0)Ce,Mg-5Al-0.3Mn-2Nd,Mg-5Al-0.3Mn-1.5(CeLa)和Mg-5Al-0.3Mn-3Y合金在300-400℃下进行了热轧制或挤压变形,与铸态合金相比,轧制和挤压合金具有更高的力学性能。轧制合金的室温抗拉强度为290-340 MPa,较铸态合金提高约50%,屈服强度约为210-260 MPa,较铸态合金提高约2倍。挤压态合金的抗拉强度为260-270 MPa,屈服强度为160-190MPa,伸长率为20-22%;150℃的力学性能也得到了明显改善。 结合热力学计算、合金化元素之间的电负性差、化合物相的生成焓数据以及相图计算,阐述了稀土化合物相的生成机制,稀土元素与Al元素之间的电负性差大于其与Mg之间的电负性差,且Al-RE相的生成焓远低于Mg-RE和Mg-Al相的生成焓,因此在Mg-Al合金中加入RE后,RE优先与Al形成Al-RE化合物。从晶粒细化、化合物强化相的生成和演变、变形加工处理的位错交互作用等方面讨论了合金的强化机制,认为细晶强化、第二相强化及形变强化是提高合金力学性能的主要机制。

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本工作完成了磷酸盐化合物ABLa(PO_4)_2的合成,这些磷盐均可在900 ℃左右合成;对其进行了结构测试与表征,发现这些磷酸盐属于单斜晶系独居石结构,与LaPO_4同构,具有很相近的晶胞参数;系统地研究了RE~(3+)离子(RE = Ce,Tb,Dy)在ABLa(PO_4)_2基质中的发光与能量传递规律,研究了Ce~(3+)、Tb~(3+)离子发光中心与基质晶格之间的相互作用,计算了这些稀土离子之间能量传递的临界距离Rc(dd),结果表明ABLa(PO_4)_2基质中Ce~(3+)离子与基质晶格之间的相互作用属于中等程度耦合,Tb~(3+)离子与基质晶格之间的相互作用属于无辐射多声子过程,Ce~(3+)→Ce~(3+)、Ce~(3+)→Tb~(3+)能量迁移临界距离均与LaPO_4中相近,Ce~(3+) → Ce~(3+)相对于Ce~(3+) → Tb~(3+)属于快过程,Ce~(3+) → Ce~(3+)能量传递对ABLa(PO_4)_2:Ce,Tb荧光体的Tb~(3+)绿色发光起了重要的作用,ABLa(PO_4)_2基质是Ce~(3+),Ce~(3+)-Tb~(3+),Ce~(3+)-Dy~(3+)的优良发光基质;最后探讨了绿色荧光体ABLa(PO_4)_2:Ce,Tb的调制途径,主要研究了Ce~(3+)、Tb~(3+)离子的浓度效应,掺杂B_2O_3、Dy~(3+)、SiO_2对荧光体发光的影响及NH_4Cl的作用,结果表明Ce~(3+)、Tb~(3+)离子的适宜浓度分别为0.2~0.5和0.08~0.2,掺杂适量的B_2O_3、Dy~(3+)能很好地提高荧光体的发光,掺杂SiO_2、NH_4Cl不利荧光体发光。

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采用基于密度泛函理论(DFT)的第一性原理平面波赝势法(PWP)计算Mg,Si和Mn共掺GaN电子结构和光学性质,分析比较计算结果.计算表明:掺杂后体系均在能隙深处产生自旋极化杂质带,具有半金属性,能产生自旋注入.与Mn掺杂GaN比较,Mg共掺后能使居里温度(TC)升高,并在1.0eV出现源于Mn4+离子基态4T1(F)到4T2(F)态跃迁的较强的光吸收,而Mn掺杂GaN时位于1.3eV处的吸收峰消失;Si共掺后没能使TC升高,且在低能区无光吸收现象.

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Mg-doped GaN layers prepared by metalorganic chemical vapor deposition were annealed at temperatures between 550 and 950℃. Room temperature (RT) Hall and photoluminescence (PL) spectroscopy measurements were performed on the as-grown and annealed samples. After annealing at 850℃, a high hole concentration of 8 × 10~(17) cm~(-3) and a resistivity of 0. 8lΩ·cm are obtained. Two dominant defect-related PL emission bands in GaN.. Mg are investigated; the blue band is centered at 2. 8eV (BL) and the ultraviolet emission band is around 3.27eV (UVL). The relative intensity of BL to UVL increases after annealing at 550℃, but decreases when theannealing temperature is raised from 650 to 850℃, and finally increases sharply when the annealing temperature is raised to 950C. The hole concentration increases with increased Mg doping, and decreases for higher Mg doping concentrations. These results indicate that the difficulties in achieving high hole concentration of 10~(18)cm~(-3) appear to be related not only to hydrogen passivation, but also to self-compensation.

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用MOCVD技术在50mm蓝宝石衬底(0001)面上生长了GaN∶Mg外延膜,对样品进行热退火处理并作了Hall、双晶X射线衍射(DCXRD)和室温光致发光谱(PL)测试.Hall测试结果表明,950℃退火后空穴浓度达到5×1017cm-3以上,电阻率降到2.5Ω·cm;(0002)面DCXRD测试发现样品退火前、后的半峰宽均约为4′;室温PL谱中发光峰位于2.85eV处,退火后峰的强度比退火前增强了8倍以上,表明样品中大量被H钝化的受主Mg原子在退火后被激活.

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The annealing of Mg-doped GaN with Pt and Mo layers has been found to effectively improve the hole concentration of such material by more than 2 times as high as those in the same material without metal. Compared with the Ni and Mo catalysts, Pt showed good activation effect for hydrogen desorption and ohmic contact to the Ni/Au electrode. Despite the weak hydrogen desorption, Mo did not diffuse into the GaNepilayer in the annealing process, thus suppressing the carrier compensation phenomenon with respect to Ni and Pt depositions, which resulted in the high activation of Mg acceptors. For the GaN activated with the Ni, Pt, and Mo layers, the blue emission became dominant, followed by a clear peak redshift and the degradation of photoluminescence signal when compared with that of GaN without metal.

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利用SFC提供的束流对新建的转轮系统进行了检验实验,得到了相关的实验结果.实验证明了该装置的可靠性,为进一步开展超重核的研究完成了预实验.

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讨论了目前有关2 2 Na(p ,γ) 2 3Mg反应的实验研究工作 ,结合兰州放射性束流线上的放射性束流2 3Al的β+延发质子衰变实验的测量结果 ,给出了2 3Al延发衰变的质子能谱 ,并比较了近期实验给出的相关能级的自旋、宇称值 ,正是由于这种自旋、宇称和能级部分宽度的不确定性 ,导致了反应率计算的不确定性 .计算了同位旋相似态的共振强度 .对于测量到的新的延发衰变能级Ed =8.91 6MeV ,由于没有相应的能级宽度值 ,实验仅给出其相对共振强度值

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The excited states in 22Mg have been investigated by the resonant elastic scattering of 21Na + p. A 4.0 MeV/nucleon 21Na beam was separated by the Center for Nuclear Study (CNS) radioactive ion beam separator (CRIB) and then used to bombard a thick (CH2)n target. The energy spectra of recoiled protons were measured at scattering angles of θc.m. ≈ 172◦ , 146◦, and 134◦, respectively. A wide energy-range of excitation function in 22Mg (up to Ex ∼ 8.9 MeV) was obtained simultaneously with a thick-target method, and a state at 7.06 MeV was newly observed. The resonant parameters were deduced from an R-matrix analysis of the center-of-mass (c.m.) differential cross-section data with a SAMMY-M6-BETA code. The astrophysical resonant reaction rate for the 18Ne(α,p)21Na reactionwas recalculated based on the present parameters. Generally speaking, the present rates are much smaller than the previous ones.