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71.
Proton (p) and two-proton (2p) emissions from the proton-rich nuclei with 10≦Z≦20 have been explored by the in-fight decay and implantation decay methods, respectively, in a series of experiments at the HIRFL-RIBLL facility. The in-flight 2p emissions from the excited states of 28,29S /26,27P and 17;18Ne were studied by complete-kinematics measurements. Mechanisms of 2p decay and related p-p correlations have been explored. Obvious 2p correlated emissions have been observed in the cases of 28,29S but not in 27,28P, indicating the 2p halo plays an important role in the diproton emission. In the 17;18Ne cases, a small 2p opening angles were deduced by the HBT analyses, implying the BCS-BEC crossover may occur in the dilute nuclear matter. Moreover, 27S/26P/25Si, 22Si/20Mg, 23Si/22Al/21Mg, 24Si/23Al, and 36;37Ca were implanted in a thin double-sided-silicon-strip detector and their -delayed p and 2p decays have been measured by a surrounding silicon detector array under the continuous-beam mode. Important information on the nuclear spectroscopy, such as energy, lifetime, branching-ratio, and so on, has been extracted, which helps us to understand the nuclear structures of proton-rich exotic nuclei close to the drip-line.  相似文献   
72.
从35 MeV/nucleon 40Ca+40Ca反应实验数据中提取了碎片Z从1到9的横向流,发现探测器阈值、探测系统的角分辨等实验条件对横向流电荷依赖的形状有显著的影响。在考虑实验条件并采用软的核物质状态方程(K=200 MeV)之后,CoMD模型计算结果很好地重现了实验中横向流电荷依赖的形状。这表明如果要更加精确地提取实验中的横向流,必须使用阈值更低、角分辨更好的探测系统。此外,结合Kohley等[Phys Rev C,2012,85:064605]从实验中提取的横向流,讨论了横向流电荷依赖的形状存在异同的原因。1 ≤ Z ≤ 6的横向流电荷依赖呈肩峰形状可能是实验条的影响引起的,而我们的实验中Z ≥ 6的横向流的减小可能是由于动量守恒对集体运动的抑制。The transverse flow in the reaction of 40Ca+40Ca at 35 MeV/nucleon has been determined for emitted isotopes with Z=1 to 9. A significant modification of the Z-dependent flow pattern caused by the experimental filters, the detector thresholds and the angular resolutions (△?) of the detector array, is observed. With the application of the appropriate experimental filters, the general trend of the experimental Z-dependent flow is well reproduced by the Constrained Molecular Dynamics (CoMD) simulation, employing an effective interaction corresponding to a soft EOS (K=200 MeV). This fact suggests that to determine the flow values more precisely, a detection system with lower energy threshold and better angular resolution is urgently required. Additionally, together with the parallel work of Z. Kohley et al.[Phys Rev C, 2012, 85:064605], the pattern of the experimental Z dependence of transverse flow is also discussed. The shoulder patterns of Z-dependent flow for 1 ≤ Z ≤ 6 can be attributed by the experimental filters, while the reduction of flow for Z ≥ 6 in our experiment can be caused by the suppression of collective motion under the momentum conservation.  相似文献   
73.
实验通过17F+p共振弹性散射研究了复合核18Ne激发态中与天体核反应14O(α, p)17F相关的共振态性质。利用兰州放射性束流线(RIBLL)对弹核碎裂反应产生的放射性束17F进行了分离和提纯。经过降能后,能量为4.22 AMeV 的17F束流轰击在T2终端的厚氢靶(CH2)n上。 两套∆E-E Si探测器望远镜放置在两个不同的探测角度θlab≈2.3°和14°上,对反冲质子的角度和能量进行了测量。实验观测到了复合核18Ne的几条质子共振能级。通过R-Matrix理论程序对激发函数进行拟合,得到了共振态的能量、 自旋、 宇称和衰变宽度等共振参数。Resonant properties in18Ne relevant to the stellar reaction of 14O(α, p)17F have been investigated through a resonant elastic scattering of 17F+p. The 17F RI beam was produced via a projectile fragmentation reaction, and subsequently separated and purified by Radioactive Ion beam Line in Lanzhou(RIBLL). After a series of energy degradation,a 4.22 AMeV 17F beam bombarded a thick(CH2)ntarget at T2 terminal. Energy and angle of the recoiled protons were measured by two sets of ∆E-E silicon telescope at θlab≈2.3°,14° respectively. Several resonances in 18Ne were observed,and their resonant parametersincluding energy,spin parity and decay width have been determined by an R-Matrix analysis of the experimental excitation function.  相似文献   
74.
描述了RIBLL终端大型探测器之一的大面积闪烁光纤阵列探测器(LASFA)的工作原理和结构特点, 报道了LASFA的研制以及单元性能的改进与测试。 LASFA具有很高的时间分辨和空间分辨能力, 可以很好地测量RIBLL终端各种轻带电粒子的信息。 The principles and structure characteristics of Large Area Scintillating Fiber Array(LASFA) detector at RIBLL (Radioactive Ion Beam Line in Lanzhou) are described. The development of LASFA and the characteristics of the scintillating fibers unit are reported. LASFA can be used to detect the light charged particles at RIBLL terminal due to its good time and spatial resolutions.  相似文献   
75.
10.6MeV/u 84Kr+27Al反应中角动量对断点前粒子多重性的影响   总被引:1,自引:0,他引:1  
用推广的裂变扩散模型研究了角动量对10.6MeV/u 84Kr(27Al,二体裂变)反应断点前粒子多重性的影响,发现阶点前粒子多重性和断点时间随着角动量的减小逐渐增大,而且绝大多数粒子是在鞍点前发射的. 对实验中二体裂变反应发生的角动量范围进行权重平均,得到了与实验一致的断点前粒子多重性. 同时还研究了影响断点前粒子多重性和断点时间的诸多因素.  相似文献   
76.
在原子核输运理论的框架内,结合统计蒸发理论,发展了一种计算中能重离子周边反应同位素分布的新方法.碰撞过程中的初始碎片由QMD理论模拟计算得到的,初始碎片的蒸发用GEMINIcode得到.计算结果很好地拟合了44MeV/u40Ar+181Ta反应的同位素分布(Z从6到10).计算结果表明压缩系数为200MeV时,能很好地解释实验结果.  相似文献   
77.
利用HIRFL提供的50MeV/u的13C束流轰击Be靶, 通过RIBLL选择出放射性核素11Li. 实验采用透射法测量了25—45MeV/u的11Li在28Si靶上的反应总截面. 采用双参数Gauss密度分布形式, 利用Glauber模型很好地拟合了高能和中能区的11Li实验数据, 并从密度分布中提取了核的物质均方根半径.  相似文献   
78.
兰州重离子加速器冷却储存环上强子物理研究计划及现状   总被引:2,自引:0,他引:2  
An internal target experiment at HIRFL-CSRm is planned for hadron physics, which focuses on hadron spectroscopy, polarized strangeness production and medium effect. A conceptual design of Hadron Physics Lanzhou Spectrometer (HPLUS) is discussed. Related computing framework involves event generation, simulation, reconstruction and final analysis. The R & D works on internal target facilities and sub-detectors are presented briefly.  相似文献   
79.
利用HIRFL提供的50MeV/u 13C束流轰击Be靶, 通过RIBLL选择出丰中子放射性核8He. 利用透射法测量了8He的去双中子截面和去四中子截面. 利用Ogawa等人的理论结合原有8He的反应总截面数据, 得到8He的核芯为4He的结论.  相似文献   
80.
A prototype of time-of-flight positron emission computed tomography (TOF-PET) has been developed for acquiring the coincident detection of 511 keV γ-rays produced from positron annihilation. It consists of two 80.5 mm×80.5 mm LYSO scintillator arrays (composed of 35×35 pixel finger crystals) with the position sensitive photomultiplier tubes R2487 as the readout. Each array is composed of 2 mm×2 mm×15 mm finger crystals and the average pixel pitch is 2.30 mm. The measured results indicate that the TOF information has the potential to significantly enhance the image quality by improving the noise variance in the image reconstruction. The best spatial resolution (FWHM) of the prototype for the pairs of 511 keV γ-rays is 1.98 mm and 2.16 mm in the x and y directions, respectively, which are smaller than the average pixel pitch of 2.30 mm.  相似文献   
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