138 resultados para Tito, Emperador de Roma, 40-81.


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测量了 25MeV/u40 Ar+115 In,58 Ni,27 A1反应前中角区出射碎片的角分布和 元素 Z分布.用改进的量子分子动力学(MQMD)模型研究了碎片的角分布和 Z 分布.理论计算值和实验值整体上符合得很好,但在前角区,MQMD模型低估 了碎片的产额,在中角区对于Z接近弹核的碎片,理论计算值比实验值偏高.碎 片产物的角分布和Z分布还与统计蒸发模型GEMINI进行了比较,结果表明,在 前角区平衡蒸发成份所占的比例很小,中角区所占的比例有所增加,但仍然是较 小的比例.同时发现平衡蒸发成份随着出射碎片核电荷数Z的减小而逐渐减 少.

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Size modification of Au nanoparticles (NPs), deposited on the Au-thick film surface and irradiated by slow highly charged ions (SHCI) 40Arq+ (3 6 q 6 12) with fixed low dose of 4.3 1011 ions/cm2 and various energy ranging from 74.64 to 290.64 keV at room temperature (293.15 K), was investigated by atomic force microscopy (AFM) and transmission electron microscopy (TEM). The effect of projectile kinetic energy on the modified size of NPs was explored by an appropriate choice of the fixed process parameters such as ion flux, irradiation temperature, incident angle, irradiation time, etc. The morphological changes of NPs were interpreted by models involving collisional mixing, Ostwald ripening (OR) and inverse Ostwald ripening (IOR) of spherical NPs on a substrate. A critical kinetic energy as well as a critical potential energy of the projectile in the Au NPs size modification process were observed.

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The highly charged ion Ar-40(16+) with the velocity (kinetic energy E (K)=150 keV, velocity V=8.5x10(5) m/s) smaller than Bohr velocity (V (Bohr)=2.9x10(6) m/s) was found to hove impacts on the surfaces of metals Ni, Mo, Au and Al, and the Ar atomic infrared light lines and X-rays spectra were simultaneously measured. The experimental results show that the highly charged ion that captures electrons is neutralized, and the multiply-excited hollow atom forms. The hollow atom cascade decay radiates lights from infrared to X-ray spectrum. The intensity of infrared lights shows that the metallic work functions play an important role in the neutralization process of highly charged ions during their interaction with metallic surfaces, which verifies the classical over-the-barrier model.

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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.

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为探讨甜高粱(Sorghum bicolor)在青海作为饲料作物种植的可能性,在青海高原上做了初步试验,结果显示:密度对茎秆高度、茎粗、产量有显著影响,对生育期、单株质量影响不显著,株行距为0.40 m×0.20m时,产量最高;浇水次数对甜高粱的生育期、茎秆高度、茎粗、单株质量、产量没有显著影响,表明甜高粱对水分依赖不高,具有很强的耐旱和抗旱性;地膜对甜高粱有极显著影响,使其生育期提前,茎秆高度增高,单株质量增加、产量提高;糖分含量在开花-收获期为15.93%~16.67%,比不盖地膜增加了29.19%~47.98%;大田示范密度0.50 m×0.20 m,开花-收获期666.7 m2产量达4 890.8 kg,投入产出比为1∶1.78,效益显著。研究表明,在青海高原东部农业区盖地膜种植饲用甜高粱,用作饲料是完全可行的。

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用速度不同的(动能EK=272和357keV,速度v=1.14×106和1.72×106m/s)的高电荷态离子40Ar17+分别入射金属Be表面,同时测量这种相互作用过程中产生的近红外光谱线和X射线谱。实验结果表明,在低速范围内(速度小于玻尔速度vBohr=2.19×106m/s),速度较小的40Ar17+离子在到达金属的表面临界距离Rc到进入表面(2—3原子层)的进程中,形成了较多的高激发态Ar原子,其退激辐射较强的光谱线,进而验证了经典过垒模型。

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Recent experiments have reached the neutron-rich Cr isotope with N = 40 and confirmed enhanced collectivity near this subshell. The current data focus on low-spin spectroscopy only, with little information on the states where high-j particles align their spins with the system rotation. By applying the projected shell model, we show that rotation alignment occurs in neutron-rich even-even Cr nuclei as early as spin 8 (h) over bar h and, owing to shell filling, the aligning particles differ in different isotopes. It is suggested that observation of irregularities in moments of inertia is a direct probe of the deformed single-particle scheme in this exotic mass region.

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We present a measurement of pi(+)pi(-)pi(+)pi(-) photonuclear production in ultraperipheral Au-Au collisions at root s(NN) = 200 GeV from the STAR experiment. The pi(+)pi(-)pi(+)pi(-) final states are observed at low transverse momentum and are accompanied by mutual nuclear excitation of the beam particles. The strong enhancement of the production cross section at low transverse momentum is consistent with coherent photoproduction. The pi(+)pi(-)pi(+)pi(-) invariant mass spectrum of the coherent events exhibits a broad peak around 1540 +/- 40 MeV/c(2) with a width of 570 +/- 60 MeV/c(2), in agreement with the photoproduction data for the rho(0)(1700). We do not observe a corresponding peak in the pi(+)pi(-) final state and measure an upper limit for the ratio of the branching fractions of the rho(0)(1700) to pi(+)pi(-) and pi(+)pi(-)pi(+)pi(-) of 2.5% at 90% confidence level. The ratio of rho(0)(1700) and rho(0)(770) coherent production cross sections is measured to be 13.4 +/- 0.8(stat.) +/- 4.4(syst.)%.

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Fragment yields for Z >= 5 from projectile fragmentation using primary beams of Ar-36,Ar-40 at 50 MeV/nucleon on Ni-64 target have been measured in RIBLL fragment separator. We compare the fragment cross sections with the predictions of the empirical EPAX parametrization of fragmentation cross-sections and Statistical Abration-Ablation model (SAA) by considering the RIBLL separator transmission rate. Isotope yield ratios between these two reactions were calculated and isoscaling parameters alpha and beta are extracted, their dependences on fragment atomic number Z and neutron number N were presented.

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本论文首先介绍了原子核高自旋态研究的一般概况以及其物理解释的基本理论,然后介绍了在束Y谱学及其实验技术。在此基础上分析和讨论了141Nd和142Pm核的高自旋态实验研究。利用能量为75-95 Mevl0F束流,通过反应128Te(19F,5ny)142Pm研究了双奇核142Pm的高自旋态能级结构。实验中进行了丫射线激发函数和Y-Y符合测量。建立了限Pm核高自旋态能级纲图,位于前人建议的一个2毫秒、8-同质异能态之上。由测量的丫射线激发函数和Y一Y符合关系,澄清了一个67微秒同质异能态及其衰变混乱的指定,本论文把67微秒同质异能态及其衰变指定给了142Pm,建议此同质异能态的激发能为2828.5 keV,推断此同质异能态的自旋宇称为13-。在本实验研究的同时,有人利用133Cs(13C,4n)142Pm反应报道了一个建立在2毫秒、8-同质异能态之上的142P亩高自旋态能级纲图;除了相应Y跃迁的多极性有较大差别外,他们报道的瞬Pm高自旋态能级纲图与我们建立在67微秒同质异能态上的基本一致。根据能级结构的系统性,识别了四个两准粒子态,一个为g7/2质子空穴耦合h11/2中子空穴激发,另外三个是h11/2质子藕合h11/2中子空穴多重态成员。根据经验壳模型计算建议了几个新建的关键能级的组态。67微秒同质异能态的组态被建议为一个四空穴态(πg_(7/2)~(-1)d_(5/2)~(-2)vh_(11/2)~(-1))_(13)-。通过130Te(16O,5nγ)141Nd反应布居了14tNd的高自旋态能级。对反应产生的在束丫射线进行了γ射线单谱和γ-γ符合测量。基于γ-γ符合关系,对原来的141Nd的高自旋态能级纲图做了很大修改,建立了14lNd核高自旋态能级纲图。新观察到了一个由八条γ射线组成的长E2级联跃迁,并指定给了141Nd。基于实验测量的γ跃迁各向异性,建议了141Nd部分能级的自旋值。根据经验壳模型和粒子震动祸合理论,用一个h11/2价中子空穴祸合142Nd核芯晕态激发定性地解释141Nd的能级结构,新发现的长E2级联跃迁很可能涉及两个hu/2质子激发。

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第一篇FEBIAD-II离子源根据物理实验的要求本文设计和加工了一套有别于中空阴极源的FEBIAD-II离子源系统,在文中对离子源结构和特点进行了分析。测试了离子源引出离子束的发散情况,得到了此离子源的工作温度,引出离子流与高压、引出板电压、网栅电流的关系曲线,进而给出本源的工作参数。第二篇少参数质量公式和核质量计算本文介绍一个少参数的原子核质量公式,并计算了28≤Z≤81的1440个原子核质量和S_(2n),与实验比较,核质量和S_(2n)的方均根偏差分别为1.01和0.57MeV。计算的双中子分离能曲线很好地重现了N=50、82的主壳效应,Z=40时N=56的亚壳效应,以及N≥60和90时的原子核发生大形变的特性

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论文分为两个部分。第一部分:研究在25MeV/u ~(40)Ar+~(115)In反应中轻粒子发射机制。实验中,利用研制的轻粒子探测器测量了发射的P、#alpha#能谱。用三源模型拟合了轻粒子能谱,所提取的参数与费米气体模型的计算结果进行比较,分析了发射源形成和衰变的一些特点。第二部分:研制一种大面积幅度、时间、位置灵敏闪烁探测器。它是HIRFL上建成的第一阶段放射性核束物理实验终端的主要设备之一,在首次放射性核束调试中收到良好的效果。本文的目的是用经典理论研究了热核形成及衰变的一些性质,在即将开展的放射性核束物理研究中, 利用研制的大型探测器对经典理论普适性进行检验

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本文首先回顾了重离子物理学的发展简史,并介绍了当前的一些关于重离子反应的理论方法,同时对于现在核物理的研究热点,热核的特性进行了概括性的叙述.由于裂变是作者工作的重点,因此在文章中,对裂变反应的理论也进行了介绍.为了能够清楚全面的说明我们的工作,本文对于实验装置和探测器也给出了详细的描述.最后,文章对25 MeVu Ar+Bi反应中的裂变进行了讨论.在这些讨论中,我们分析了反应中与裂变相关的数据,得到了碎片的质量,动能分布。同时运用与碎片相关联的4He粒子能谱提取了核温度和裂前裂后的4He粒子多重性,并利用这一数据计算了不同初始激发能下的裂点激发能和裂变时标.

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中等质量碎片(IMF)的发射是中能重离子碰撞的一大特点,且随着轰击能量的升高其产额迅速增加。通过测量30MeV/u 40Ar+natAg反应中出射的中等质量碎片,研究了高激发热核的发射机制、发射时标和时空演化规律。 对反应中发射碎片能谱的运动源拟合表明,前角区(11°—22°)中等质量碎片(IMF)来自于三种成分:类靶源、类弹源和中速源成分,其中类弹和中速成分占主导,关联测量的IMF能谱拟合得到,一个来自于类弹源而另一个来自于中速源成分的事件占有相当大的比例。 利用小相对角度内的两碎片关联测量,研究高激发核衰变中中等质量碎片的发射时标和寿命。IMF发射时间随能量的变化很大,从低能碎片的250 fm/c到高能粒子的100 fm/c,表明在此能量下,反应中出射的IMF主要来自于相继两体衰变。通过与其它实验的比较可知,随着束流能量的升高,IMF发射时间由相继两体衰变向多重碎裂过渡。 IMF时空演化研究表明,发射空间的大小对IMF关联函数的影响主要来自于发射源的核物质密度而几乎不依赖于发射源的质量数。