双奇核~(184)Au中πi_(913/2)νi_(13/2)转动带的结构特征研究

利用重离子熔合蒸发反应和在束γ谱学实验方法 ,研究了双奇核184 Au的高自旋态能级结构 .扩展了基于πh9/ 2 ν7/ 2 - [5 14 ]和πi13/ 2 νi13/ 2 2准粒子组态下的转动带能级纲图 ,建立了两个转动带之间以及πh9/ 2 ν7/ 2 - [5 14 ]带与基态的谱学连接 .从而确定了πi13/ 2 νi13/ 2 带能级的自旋和宇称 ,证实了此转动带在低自旋区出现旋称反转 .分析了πi13/ 2 νi13/ 2 带和相邻核转动带的准粒子顺排特征 ,指出此带的第一回弯以及相邻核转动带在低频观测到的顺排异常可能与h9/ 2 质子顺排有关 .

~(179)Au的1/2[660](πi_(13/2))转动带

利用能量为 16 4— 180MeV的 3 5Cl束流 ,通过重离子核反应 14 9Sm(3 5Cl ,5n)研究了 179Au的高自旋态能级结构 .实验进行了γ射线的激发函数、X γ和γ γ t符合测量 .基于对实验测量结果的分析 ,首次建立了 179Au的 1 2 [6 6 0 ](πi13 2 )转动带 .结合已有的实验数据 ,着重讨论了奇AAu核中1 2 [6 6 0 ](πi13 2 )转动带的带头激发能随中子数的变化

35MeV/u~(40)Ar+~(197)Au反应中复合核的激发能与温度

利用大面积位置灵敏气体探测器对 35MeV u4 0Ar +197Au反应中形成的裂片进行了符合测量 ,由此得到了裂变复合核的速度分布 .在大质量转移假设下扣除前平衡发射粒子的影响 ,得到复合核的激发能 .另外利用望远镜探测器对反应中出射的轻带电粒子也进行了符合测量 ,并由后角α ,p ,d ,t的能谱提取了复合核的温度 .温度与激发能的关系没有表现出理论预言的相变特征 .

双奇核~(182)Au高自旋态能级结构及旋称反转

利用~(152)Sm(~(35)Cl,5nγ)~(182)Au核反应产生并研究了双奇核~(182)Au的高自旋态,首次建立了双奇核~(182)Au基于πh_(9/2)(×)Vi(13/2)和πi_(13/2)(×)Vi_(13/2)准粒子组态上的转动带能级纲图,发现在低自旋区,两个转动带能级均出现旋称反转.用推转壳模型对~(182)Au的转动带能级进行了理论研究,发现当采用形变和对力自洽计算后,从理论上可以定性地解释~(182)Au核中两个转动带出现的旋称反转现象。

~(17)N+~(197)Au反应中碎片与中子的符合测量

在 3 3 .4MeV/u17N束轰击197Au靶产生的反应中 ,利用放置于不同角度组合的 1 7个中子探测器 ( 4°— 83°)和 1 4个半导体望远镜 ( 2 .3°— 9.0°)对反应产物碎片与中子进行了符合测量 .经对所得实验角分布积分得到Z =3— 6元素的同位素产额分布 .在参加者 -旁观者模型框架下 ,采用17N原子核内部的不同密度分布计算了同位素产额分布并与实验数据做比较

用于~(18)N在~9Be、~(197)Au靶上破裂反应研究的探测器系统

描述了用于放射性核束 18N在 9Be、197Au靶上破裂反应研究的探测器系统构成、性能、特点及在线实验的初步结果。

35MeV/u~(40)Ar+~(197)Au反应中热核的碎裂密度

许多提取核反应过程中熵产生的方法只适用于高能核反应过程 ,而约化d的产额方法可以用于较低能量的重离子核反应中 .对于 3 5MeV/u40 Ar+ 197Au的核反应过程 ,利用这种方法所得的熵和约化带电粒子多重性提取的熵结果一致 .对于后角热核发射体系 ,实验提取的核温度为 ( 4.7± 1 .2 )MeV ,熵为S/A =2 .5± 0 .5,根据实验提取的熵和核温度可以确定其碎裂密度小于 0 .1 ρ0

35MeV/u~(40)Ar+~(197)Au中的熵产生

根据量子统计模型 (QSM )的计算分析 ,找到了一个提取核反应过程中熵产生的新的可观测量 .核反应过程中约化d的产额d/ (d +t+3 He+4 He)和熵有单调的函数关系 ,并且和体系的碎裂密度 (ρ/ ρ0 )及体系的N/Z都无关 ,可以作为提取核反应过程中熵产生的一个观测量 .和目前已经有的其他方法相比 ,约化d产额这一提取熵方法可以用于较低能量的重离子核反应中 ,并且数据处理分析简单 .对于 35MeV/u4 0 Ar +197Au的核反应过程所提取的熵和利用约化带电粒子多重性提取的熵结果一致 .结合后角类靶热核发射体系实验提取的同位素核温度为 4 7±1 2MeV及S/A =2 5± 0 5 ,根据熵和核温度的关联关系 ,可以确定其Breakup密度接近但小于 0 1(ρ/ ρ0 )

35MeV/u~(40)Ar+~(197)Au反应中热核的统计发射研究

利用硅半导体＋ＣｓＩ（Ｔ１）闪烁体望远镜测量３５ＭｅＶ／ｕ４０Ａｒ＋１９７Ａｕ中发射的轻带电粒子，用能谱斜率方法和双同位素产额比方法提取了核温度参量．研究了热核发射过程中的统计发射规律．

通过改变Si(Au)探测器灵敏区厚度鉴别带电粒子的方法及应用研究

重点研讨通过改变探测器偏压，进而改变探测器的ＰＮ 结（有效探测灵敏区）厚度，实现对带电粒子的种类和能量鉴别的实验方法及其实际应用。实验测量了３ＭｅＶ质子和６．０５ＭｅＶ α粒子在金硅面垒探测器Ｓｉ（Ａｕ）中的能损与探测器偏压关系曲线。同时利用刻度过的探测器鉴别氘离子束轰击氘钛（ＴｉＤＸ）靶发射的带电粒子能谱。在很强的本底情况下通过调节探测器偏压（灵敏区厚度）实现了对能量相近的不同带电粒子的有效鉴别和测量。

Size modification of Au nanoparticles induced by slow highly charged ions Ar-40(q+) irradiation

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.

Relativistic Distorted-Wave Collision Strengths of Ni-, Cu- and Zn-like Au Ions

Excitation energies and electron impact excitation strengths from the ground states of Ni-, Cu- and Zn-like Au ions are calculated. The collision strengths are computed by a 213-levels expansion for the Ni- like Au ion, 405-levels expansion for the Cu-like Au ion and 229-levels expansion for the Zn-like Au ion. Configuration interactions are taken into account for all levels included. The target state wavefunctions are calculated by using the Grasp92 code. The continuum orbits are computed in the distorted-wave approximation, in which the direct and exchange potentials among all the electrons are included. Excellent agreement is found when the results are compared with previous calculations and recent measurements.

20—50MeV O5+离子引起Au的L壳层X射线产生截面研究

在北京13 MV串列加速器上利用20—50MeV O5+离子研究Au的L壳层X射线产生截面. 实验结果表明σ（Ll）/σ（Lα） ，σ（Lβ）/σ（Lα） 和σ（Lγ）/σ（Lα）与EＣＰSSR理论计算结果符合比较好.在实验中由于较高的能量,在能量点存在能移现象.

Search for signature inversion in the pi i(13/2) circle times upsilon i1(3/2) bands in Au-182,Au-184,Au-186

Search for low-spin signature inversion in the pi i(13/2) circle times nu i(13/2) bands in odd-odd Au-182,Au-184,Au-186 has been conducted through the standard in-beam gamma-spectroscopy techniques. The experiments for Au-182 and 186Au have been performed in the Japan Atomic Energy Agency (JAEA) via the Sm-152(Cl-35,5n)Au-182 and Yb-172(F-19,5n)Au-186 reactions, respectively. A study of Au-184 has been made using a multi-detector array GASP in LNL, Italy, via the Tb-159(Si-29,4n)Au-184 reaction. The pi i(13/2) circle times nu i(13/2) bands in these three nuclei have been identified and extended up to high-spin states. In particular, the inter-band connection between the pi i(13/2) nu i(13/2) band and the ground-state band in 184 Au has been established, leading to a firm spin-and-parity assignment for the pi i(13/2) circle times nu i(13/2) band. The low-spin signature inversion is found in the pi i(13/2) circle times nu i(13/2) bands in Au-182,Au-184,Au-186 according to our spin-assignment and the signature crossing observed at high-spin states.

Photons from quark and hadron phases in Au plus Au collisions

Based on a relativistic hydrodynamic model describing the evolution of the chemically equilibrating quark-gluon plasma system with finite baryon density in a 3+1-dimensional spacetime, we compute photons from the quark phase, hadronic phase and initial non-thermal contributions. It is found that due to the effects of the initial quark chemical potential, chemical equilibration and rapid expansion of the system, the photon yield of the quark-gluon plasma is strongly suppressed, and photons from hadronic matter and initial non-thermal contributions almost reproduce experimental data.