958 resultados para SN 2006ov


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在 30MeV/u4 0 Ar +112 ,12 4 Sn反应中用平行板雪崩计数器实现了前冲余核的测量 .在不同的线性动量转移下用运动源模型拟合了后角的3 He,α和6He能谱 ,发现3 He的能谱斜率温度在12 4 Sn系统中高于112 Sn系统 ,而6He的温度在112 Sn系统中更高 ,α粒子在两个系统中没有明显差别 .用热核粒子蒸发过程衰变道的选择性对这种同位旋相关性进行了解释 .GEMINI的计算不能重现实验结果

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35MeV/u 36 ,40 Ar+ 112 ,12 4Sn反应中 ,在前角 5°和 2 0°观测到丰中子核与稳定核的产额比随粒子出射动能的增加而减小 ,而缺中子核与稳定核的产额比随动能的增加而增加 .对于某种元素 ,随着动能的减小 ,其平均中质比逐渐由弹核N/Z向靶核N/Z过渡 .这些现象表明在这样的入射能量下 ,周边或近周边碰撞过程中同位旋自由度没有完全达到平衡 .这种行为对两个靶核系统是相似的 ,但是同位素产额比的绝对值在 5°没有靶核相关性 ,而在 2 0°处却表现出明显的靶核相关性 .

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利用同位旋相关的量子分子动力学模型,研究了~(112)Sn+~(112)Sn和~(124)Sn+ ~(124)Sn两个反应系统在入射能量 E=40MeV/u时的多重碎裂。计算结果能与 实验值定性符合。观察到两个反应系统中,中等质量碎片多重性、中子多重性、 荷电粒子多重性与轻荷电粒子多重性之间的关联存在着明显的差别。另外,通 过与膨胀蒸发源模型及同位旋相关的渗透模型分析结果的比较,发现这种差别 主要是由同位旋相关的反应动力学所造成的。

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The reduced velocity correlation functions of the Intermediate Mass Fragments (IMFs) were measured in the reactions of Ar-36+ Sn-112,Sn-124 at 35MeV/u. The anti-correlation at small reduced velocities is more pronounced in Ar-36+ Sn-124 system than that in Ar-36+ Sn-112 system. The difference of the correlation functions between the two reactions is mainly contributed by the particle pairs with high momenta. A three-body Coulomb repulsive trajectory code (MENEKA) is employed to calculate the emission time scale of IMFs for-the both systems. The time scale is 150fm/c in the Ar-36+ Sn-112 system and 120fm/c in the Ar-36+ Sn-124 system, respectively. A calculation based on an Isospin dependence Quantum Molecular Dynamics code (IQMD) reveals that the emission time spectrum of IMFs is shifted slightly leftwards in Ar-36+ Sn-124 compared with that in the Ar-16+ Sn-112 system, indicating a shorter emission time scale. Correspondingly, the central density of the hot nuclei decreases faster in Ar-36+ Sn-124 than in Ar-36+ Sn-112

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Equilibration and equilibration rates have been measured by colliding Sn nuclei with different isospin asymmetries at beam energies of E/A = 35 MeV. Using the yields of mirror nuclei of Li-7 and Be-7, we have studied the diffusion of isospin asymmetry by combining data from asymmetric Sn-112 + Sn-124 and Sn-124 + Sn-112 collisions with those from symmetric Sn-112 + Sn-112 and Sn-124 + Sn-124 collisions. We use these measurements to probe isospin equilibration in central collisions where nucleon-nucleon collisions are strongly blocked by the Pauli exclusion principle. The results are consistent with transport theoretical calculations that predict a degree of transparency in these collisions, but inconsistent with the emission of intermediate mass fragments by a single chemically equilibrated source. Comparisons with quantum molecular dynamics calculations are consistent with results obtained at higher incident energies that provide constraints on the density dependence of the symmetry energy.

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Correlations between the behavior of the nuclear symmetry energy, the neutron skins, and the percentage of energy-weighted sum rule (EWSR) exhausted by the pygmy dipole resonance (PDR) in Ni-68 and Sn-132 are investigated by using different random phase approximation (RPA) models for the dipole response, based on a representative set of Skyrme effective forces plus meson-exchange effective Lagrangians. A comparison with the experimental data has allowed us to constrain the value of the derivative of the symmetry energy at saturation. The neutron skin radius is deduced under this constraint.

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The hydroconversion of n-paraffins is a key reaction in hydrodewaxing of lubricating base oil. In this paper, we investigate the performance of Pt/SAPO-11 catalysts for isomerization of n-paraffins by the model compound of n-dodecane. Under this experimental condition, yields of feed isomers as well as cracking products are a function of the total n-dodecane conversion. Primary products are methylundecane while multi-brancheds and cracking products are formed in successive reactions. The result shows that the addition of Sn increases the selectivity for isomerization reaction. The most ideal experimental data for hydroconversion of n-dodecane is that the selectivity of isomerized products gets 90% when conversion of n-dodecane is 90% for the Sn-promoted Pt/SAPO-11 catalyst.

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土壤中重金属的解吸直接影响重金属在环境中的形态转化和植物有效性。文章以我国东北地区草甸棕壤作为研究对象,通过对Sn、Hg、Sb、Bi单一及复合污染土壤中Sn、Hg、Sb、Bi的解吸动力学行为的研究,探索污染土壤中重金属Sn、Hg、Sb、Bi的解吸特性与规律。结果表明,不同污染类型的污染土壤中Sn、Hg、Sb、Bi这几种重金属的解吸量随着振荡时间的延长而不断增加。重金属Sn、Hg、Sb、Bi的解吸过程可分为快速反应阶段和慢速反应阶段。描述土壤Sn、Hg、Sb、Bi解吸动力学过程的最优模型为Elovich方程,其次为双常数方程,而一级动力学方程拟合效果不佳。此外,污染土壤中重金属Sn、Hg、Sb、Bi的解吸过程受共存重金属元素的影响。

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In this paper, five Pt3Sn1/C catalysts have been prepared using three different methods. It was found that phosphorus deposited on the surface of carbon with Pt and Sn when sodium hypophosphite was used as reducing agent by optimization of synthetic conditions such as pH in the synthetic solution and temperature. The deposition of phosphorus should be effective on the size reduction and markedly reduces PtSn nanoparticle size, and raise electrochemical active surface (EAS) area of catalyst and improve the catalytic performance. TEM images show PtSnP nanoparticles are highly dispersed on the carbon surface with average diameters of 2 nm. The optimum composition is Pt3Sn1P2/C (note PtSn/C-3) catalyst in my work. With this composition, it shows very high activity for the electrooxidation of ethanol and exhibit enhanced performance compared with other two Pt3Sn1/C catalysts that prepared using ethylene glycol reduction method (note PtSn/C-EG) and borohydride reduction method (note PtSn/-B). The maximum power densities of direct ethanol fuel cell (DEFC) were 61 mW cm(-2) that is 150 and 170% higher than that of the PtSn/C-EG and PtSn/C-B catalyst.

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利用电介质的平均能带模型计算了Bi2 Sr2 Can- 1CunO2n +4 (n =1,2 ,3)的化学键参数 .应用由共价性和极化率定义的化学环境因子计算了57Fe和119Sn在Bi2 Sr2 Can - 1CunO2n +4 中的M ssbauer同质异能位移 ,确定了57Fe和119Sn在Bi2 Sr2 Can- 1CunO2n +4 中的价态和占位情况 .

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The hetero atom substituted aluminophosphate molecular sieves Me-VPI-5(Me = Mgt Ti, Sn, Si) were synthesized hydrothermally. Rare earth ions are originally doped into these microporous materials by aqueous solution ion exchange procedures. The phase transitions of the microporous materials are investigated by high-temperature and high-pressure experimental techniques. The influence of the phase transitions on the rare earth ions' spectral structures is discussed, With the increase of temperature, Eu(II)Mg-VPI-5 is converted into Eu(II)Mg-AIPO(4)-8, then into tridymite phase. The pressure has a notable influence on Eu(II) ion's spectral structures. The spectral structures have changed regularly with the increase of pressure.

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用水热同晶置换法合成了杂原子磷酸铝分子筛Me-VPI-5(Me=Mg,Ti,Sn,Si).通过水相离子交换法掺杂稀土离子,考察了高温和高压下的相变行为.讨论了相变过程对稀土离子光谱的影响.随着温度升高,Eu(Ⅲ)Mg-VPI-5先转变为Eu(Ⅲ)-AlPO4-8,然后又转变成致密的磷石英相.压力对Eu(Ⅲ)光谱结构具有显著影响.随着压力增加,Eu(Ⅲ)光谱结构发生规律性变化.