核核碰撞中不稳定轻核的方位角各向异性发射

利用符合的粒子粒子关联测量，研究了２５ＭｅＶ／ｕ^４０Ａｒ＋^１９７Ａｕ反应中不稳定轻核的在平面发射和出平面发射．对于中速的不稳定轻核，观测到在平面发射几率增大，这表明该反应系统中存在旋转效应．该现象随碰撞参数增大更为强烈，而随着不稳定核激发态能量的升高稍有变弱     

46．7MeV／A~（12）C轰击~（159）Tb、~（197）Au和~（209

用４６．７ＭｅＶ／Ａ１２Ｃ轰击１５９Ｔｂ、１９７Ａｕ和２０９Ｂｉ，测量关联裂片的速度和角度．研究了线动量转移、质量和出平面角分布，提取了核温度．应用级联两体统计衰变理论进行了拟合与解释，结果表明：在入射能约为５０ＭｅＶ／Ａ的中能重离子碰撞中，以非完全熔合方式形成了核温度高达４－５ＭｅＶ的类复合核，其后通过裂变、蒸发级联统计两体衰变而退激．     

Fermi能区核－核碰撞的平衡前中子发射

利用ＢＵＵ模型模拟核－核碰撞３６Ａｒ＋１０８Ａｇ（３５Ｍｅｖ／ｕ）、１４Ｎ＋１０８Ａｇ（３５ＭｅＶ／ｕ）中的平衡前中子发射．模拟结果与唯象的运动源拟合给出的中等速度源成份相吻合．这说明中等速度源成份产生于核－核碰撞的早期，对应平衡前发射．并从级联碰撞的角度定量地研究了平衡前发射的持续时间     

30MeV/u~(40)Ar ~(159)Tb反应中中等质量碎片的发射时标与发射机制

报道３０ＭｅＶ／ｕ４０Ａｒ＋１５９Ｔｂ反应中碎片碎片关联函数的实验结果．利用三体弹道模型从关联函数提取了中等质量碎片发射时间．中等质量碎片的平均发射时间随碎片能量而变化，从低能时的约５００ｆｍ／ｃ下降至高能时的约１００ｆｍ／ｃ．中等质量碎片发射时间随束流能量的升高而下降，表明随着束流能量的升高中等质量碎片发射机制逐渐从相继两体衰变向多重碎裂发射过渡．对于４０Ａｒ＋１５９Ｔｂ反应，此过渡能区在３５—４５ＭｅＶ／ｕ之间     

25MeV/u~(40)Ar ~(93)Nb反应中热核的激发能和核温度

利用半导体望远镜探测器和ＰＰＡＣ对２５ＭｅＶ／ｕ４０Ａｒ＋９３Ｎｂ反应中的带电粒子和余核进行了关联测量，对所得α粒子能谱用三源模型进行了拟合，并由余核飞行时间和粒子多重性得到热核激发能．通过对温度的修正，发现在本实验中有激发能Ｅ＊／Ａ为４．３ＭｅＶ，温度Ｔｉｎｉｔ为６．９ＭｅＶ的热核形成。通过与其它实验结果的对比可以看出核物质在轻系统和重系统中行为的差异。     

关于相对论性α粒子的双温度发射问题

本文对高能核核碰撞中相对论性α粒子的角分布，并与２．１ＧｅＶ／ｕ＾１６Ｏ和１．７ＧｅＶ／ｕ＾５６Ｆｅ与核乳胶相互作用的有关实验结果作了比较。     

40Ar+197Au(25MeV/u)产生的热核激发能与核温度的关系

对25MeV/u ⁴⁰Ar+¹⁹⁷Au反应系统裂变与后角轻粒子发射进行了符合测量,用裂变碎片折叠角和裂变碎片的飞行时间再构转移到类熔合核的线性动量.通过对线性动量转移和轻带电粒子能谱测量,给出从中心碰撞到周边碰撞产生的类熔合核的初始激发能、角动量和核温度,讨论它们的关系.发现了中心碰撞形成的类复合核的核温度已经接近饱和状态,接近多重碎裂的“准相变区”.     

Fermi能区核–核碰撞的平衡前中子发射

利用BUU模型模拟核-核碰撞³⁶Ar+¹⁰⁸Ag(35Mev/u)、¹⁴N+¹⁰⁸Ag(35MeV/u)中的平衡前中子发射.模拟结果与唯象的运动源拟合给出的中等速度源成份相吻合.这说明中等速度源成份产生于核-核碰撞的早期,对应平衡前发射.并从级联碰撞的角度定量地研究了平衡前发射的持续时间.     

重离子反应中核子前平衡发射的同位旋效应

考虑了同位旋相关的对称能、库仑能及核子—核子碰撞截面，对反应４０Ａｒ＋４０Ａｒ（Ｅ＝２５ＭｅＶ／ｕ，ｂ＝０）进行了量子分子动力学模拟，讨论了同位旋效应对核子发射的影响．观察到前平衡发射的中子和质子的比率大于反应系统的中质比，发现对称能有利于中子的发射而阻碍质子的发射，而同位旋相关的核子—核子碰撞截面对中子和质子的发射都有利，但似乎更有利于质子的发射。     

30MeV/u 40Ar+159Tb反应中前角区复杂碎片的来源

在前角测量了30MeV/u ⁴⁰Ar+¹⁵⁹Tb反应中两裂片符合下的轻粒子和复杂碎片,利用线性动量转移和总横向动量方法对三体符合事件进行了碰撞参数分类. 实验结果表明,在中心碰撞中复杂碎片主要来自于平衡类靶核的统计发射,并伴随有非平衡中途成份;而周边碰撞中前角区复杂碎片主要来自于弹核碎裂成份. 在半中心碰撞中则存在类弹、类靶和中途三种成份.     

The correlation functions and emission time scales for light particles and light fragments in 40Ar+197Au reactions at 25 MeV/nucleon

Two-particle correlation functions were measured for the emission of protons, deuterons, tritons, α, and lithium fragment at small relative momenta in ⁴⁰Ar-induced reactions on ¹⁹⁷Au at 25 MeV/nucleon. Based on three-body trajectory calculations the emission time scales for the particles were extracted from p-d, d-d, t-t, and lithium-lithium correlation functions. The mean emission time was found to decrease with increasing sum of the kinetic energies of the particle in a correlated pairs, indicating the emission of more energetic particles at earlier stages of the reaction than at later stages. The time scale for the emission of lithium fragments emission suggests that sequential binary disassembly occurs in ⁴⁰Ar+¹⁹⁷Au reaction at MeV/nucleon. Mean emission temperature of 3.5_−0.8^+1.3 and 3.6±0.4 MeV were also extracted from the relative populations of the excited and ground states of the respective emitted nuclides ⁸Be and ⁴He.     

Isospin Effect on Relative State Population Temperature in the Reactions 40Ar+ 112,124Sn at 30MeV/u

An array of 13 detector telescopes has been used for detecting small-angle particle-particle correlations in the reactions ⁴⁰Ar+^112,124Sn at 30MeV/u. The α-α correlation functions were extracted from two-particle coincident events. A three-body trajectory code MENEKA was used to calculate the background correlation function. The detection efficiency was calculated by using the Monte-Carlo method. After subtracting the background correlation and making the detection efficiency correction, the temperatures of 4.18±0.25 0.21 MeV and 4.10±0.22 0.20MeV are obtained from relative populations of ⁸Be states for the reaction systems with different isospin,⁴⁰Ar+¹¹²Sn and ⁴⁰Ar+¹²⁴Sn, respectively. From the relationship between the state population temperature and outgoing particle energies, it is found that the emission temperature decreases with increase of the particle energies for both studied reaction systems. For the neutron deficient system ⁴⁰Ar+¹¹²Sn the emission temperature is 5.13±0.30 0.26MeV for the lower emitting particle energies and 3.87±0.37 0.29MeV for the higher emitting particle energies. And for the neutron rich system ⁴⁰Ar+¹²⁴Sn the emission temperature is 5.39±0.30 0.26MeV for the lower emitting particle energies and 3.32± 0.28 0.23MeV for the higher emitting particle energies. This kind of isospin dependence is discussed.     

Proton and α sequential emission in the 16O + 58Ni deep inelastic reaction: A semi-classical approach

The 132 MeV ¹⁶O + ⁵⁸Ni reaction has been experimentally investigated by using coincident charged particle techniques. A closed-form theoretical approach, describing in a simple picture the non-equilibrium component and the evaporative one of the angular correlation between light particles and reaction residues emitted in a peripheral heavy-ion collision, is applied — in the hypotesis of a sequential process — to the (C,N,O)-α and (C,N,O)-p differential multiplicities for the ¹⁶O + ⁵⁸Ni at 8.25 MeV/A deep inelastic collision. From this analysis some reaction mechanism information is deduced.     

30MeV/u40Ar+159Tb反应中中等质量碎片的发射时标与发射机制

报道30MeV/u⁴⁰Ar+¹⁵⁹Tb反应中碎片-碎片关联函数的实验结果．利用三体弹道模型从关联函数提取了中等质量碎片发射时间．中等质量碎片的平均发射时间随碎片能量而变化，从低能时的约500fm/c下降至高能时的约100fm/c．中等质量碎片发射时间随束流能量的升高而下降，表明随着束流能量的升高中等质量碎片发射机制逐渐从相继两体衰变向多重碎裂发射过渡．对于⁴⁰Ar+¹⁵⁹Tb反应，此过渡能区在35—45MeV/u之间 关键词：     

Preequilibrium α-particle emission in heavy-ion reactions

The α-particle emission following ¹⁴N-induced reactions on various heavy targets at 85–115 MeV has been studied. Cross sections of heavy residual nuclei produced after α-emission were measured in the case of the ²⁰⁹Bi target and were found to be close to the angle-integrated cross sections of α-particles, indicating that the α-emission mainly takes place in a binary process. The measured angular distributions of α-particles are pronouncedly forward-peaked, while the energy spectra are always characterized by the Maxwellian distribution even at forward angles and reproduced excellently by the statistical evaporation formula when nuclear temperature is treated as a free parameter. The resultant value of the temperature is high (4–6 MeV) at forward angles and decreases monotonically with increasing emission angles.The energy and angular distributions of protons, deuterons and tritons were also measured in the ¹⁸¹Ta + ¹⁴N reaction at 115 MeV. The results are similar to those of α-particles. In particular, nuclear temperatures turned out nearly equal to each other, being consistent with the hot-spot interpretation for the relevant preequilibrium light-particle emission.     

Pre-equilibrium alpha emission accompanying deep-inelastic16O+58Ni collisions

α particles were measured in coincidence with projectile-like reaction products (oxygen and carbon) produced in deep-inelastic¹⁶O+⁵⁸Ni collisions at about 6 MeV/N bombarding energy. The kinematic analysis of the HI andα energies measured as a function ofΘ _α gives strong evidence for a sequential process: the target-like fragments are excited by the deep-inelastic collision and undergo subsequentα decay. In contrast, the angular correlations show a pronounced forward peak, indicative of direct or pre-equilibriumα emission. The emission time for the latter is estimated to be of the order of 2×10^?21 s. To resolve this conflict of co-existing statistical and direct features of the pre-equilibrium emission, the concept of a hot spot is proposed. From the angular correlation and from theα multiplicities, a local temperature ofT?3.5 MeV is deduced which agrees well with the temperature derived from the shape of theα spectra. The spot size is estimated to be 1/5 of the sphere.     

Final state interaction and direct features of the 9Be(τ, α)αα and 10B(d, α)αα reactions

Alpha-particle spectra and α-α correlations have been measured from the ⁹Be(τ, α)αα and ¹⁰B(d, α)αα reactions at several energies between 2.9 and 10.0 MeV. Significant difierences in the spectra from the reactions were observed at equal c.m. energies and momentum transfer values. However the continuous energy spectra have been successfully analyzed with two-body interactions as obtained from elastic α-α scattering, within a formalism adequate for a three-body state. DWBA fits have also been obtained for both reactions but they are satisfactory only for the ⁹Be(τ, α)⁸Be reaction.     

The neutron continuum from the9Be+α reaction

Spectra of the low energy neutron continuum between 0.1 and 2.4 MeV from the Be+α reaction were measured at 5.01, 5.44, 6.37 and 7.44 MeV bombarding energies and different angles of neutron emission. The intensity is strongly peaked in the forward direction and the neutron distributions show maxima between 0.3 and 0.6 MeV. The results are consistent with the assumption that the continuum is due to the sequential decay⁹Be(α, α′)⁹Be*→⁸Be+n. The shape and magnitude of the continuum from a²⁴¹Am-Be(α,n) source were determined as well.     

four-body break-up and states in Be

The four-body break-up d+¹¹B → α+n reaction has been studied by simultaneous detection of α-α and α-n coincidences at two bombarding energies, 10.425 and 12.0 MeV, in order to obtain information about the decay properties of the excited states in ⁹Be. Measured spectra reveal the importance of sequential decay mechanisms in the reaction. The decay structure of low-lying levels in ⁹Be has been discussed.     

Determination of angular momenta in the incomplete-fusion channels of the reactions Ta+22Ne and Ir+12C

By using the γ-ray-multiplicity technique, experiments were carried out to determine the input angular momenta lⁱⁿ corresponding to the heavy-ion induced incomplete-fusion reactions involving the emission of fast charged particles. The α-particle and Li-nuclei emission channels were investigated in the reaction ¹⁸¹Ta + ²²Ne at the average Ne-ion energy of 155 MeV and for the α-particle emission channel in the reaction ^natIr+¹²C at E = 100 MeV. The separation of the reaction channels was carried out using an X-ray spectrometer. The angular distributions of the fission fragments were measured in the reaction ¹⁸¹Ta(²²Ne, αf). The data obtained indicate that input angular momenta are equal to about 60 ? and 50 ? for the channels of Li emission and α-emission, respectively, being practically independent of the particle energy. For the α-emission channel the lⁱⁿ values are the same for both reactions within experimental errors. The lifetime of the system of interacting target and projectile nuclei, prior to the emission of an α-particle, has been estimated to be equal to 10^?20s.