Effects of elastic and inelastic NN scattering cross sections on pi(-)/pi(+) ratios in heavy-ion collisions at intermediate energies

Based on the isospin-dependent Boltzmann-Uehling-Uhlenbeck transport model and the scaling model according to nucleon effective mass, effects of elastic and inelastic NN scattering cross sections on pi(-)/pi(+) in the neutron-rich reaction of Ca-48 + Ca-48 at a beam energy of 400 MeV/nucleon are studied. It is found that cross-section effects of both NN elastic and inelastic scatterings affect Delta(1232), pi(-) and pi(+) production, as well as the value of pi(-)/pi(+).

alpha-decay half-lives and Q(alpha) values of superheavy nuclei

The alpha-decay half-lives of recently synthesized superheavy nuclei (SHN) are investigated by employing a unified fission model (UFM) where a new method to calculate the assault frequency of alpha emission is used. The excellent agreement with the experimental data indicates the UFM is a useful tool to investigate these alpha decays. It is found that the alpha-decay half-lives become more and more insensitive to the Q(alpha) values as the atomic number increases on the whole, which is favorable for us to predict the half-lives of SHN. In addition, a formula is proposed to compute the Q(alpha) values for the nuclei with Z >= 92 and N >= 140 with a good accuracy, according to which the long-lived SHN should be neutron rich. Several weeks ago, two isotopes of a new element with atomic number Z = 117 were synthesized and their alpha-decay chains have been observed. The Q(alpha) formula is found to work well for these nuclei, confirming its predictive power. The experimental half-lives are well reproduced by employing the UFM with the experimental Q(alpha) values. This fact that the experimental half-lives are compatible with experimental Q(alpha) values supports the synthesis of a new element 117 and the experimental measurements to a certain extent.

Medium effects on pi(-)/pi(+) in heavy-ion collisions at intermediate energies

Based on the isospin-dependent transport model IBUU and on the scaling model according to nucleon effective mass, effects of elastic and inelastic NN scattering cross-sections on pi(-)/pi(+) in the neutron-rich reaction Ca-48 + Ca-48 at a beam energy of 400MeV/nucleon are studied. It is found that cross-section effects of both NN elastic and inelastic scatterings affect Delta(1232), pi(-) and pi(+) productions as well as the value of pi(-)/pi(+).

TRITON-(HE)-H-3 RELATIVE AND DIFFERENTIAL FLOWS AND THE HIGH DENSITY BEHAVIOR OF NUCLEAR SYMMETRY ENERGY

Using a transport model coupled with a phase-space coalescence after-burner we study the triton-He-3 relative and differential transverse flows in semi-central Sn-132 + Sn-124 reactions at a beam energy of 400 MeV/nucleon. We find that the triton-He-3 pairs carry interesting information about the density dependence of the nuclear symmetry energy. The t-He-3 relative flow can be used as a particularly powerful probe of the high-density behavior of the nuclear symmetry energy.

激光离子源用于A>170重丰中子新核素的研究

本文概述了 A > 170 质量区重丰中子同位素研究的主要工作和意义；介绍了 A > 170 重丰中子同位素合成、分离和鉴别方法；详细论述了激光离子源的原理、设计及其同传统离子源相比所具有的优越性；在文章结尾，设计了一个物理实验，实验目的在于：1）寻找 ~(181)Yb新核素；2）揭示天体物理学中~(180m)Ta 的产生问题。我们对反应截面进行了分析，并对产额进行了估计，证明了此实验设计的合理性，进而说明了带激光离子源的同位素分离器适用于产生截面很低的新核素和衰变研究。本文重点讨论了激光离子源的各方面问题：介绍了激光多步共振电离原理和激光离子源原理；具体分析了热毛细管式激光离子源元素选择性的产生及其影响的因素；讨论了在设计、加工过程中的具体问题；描述了所使用的激光技术；通过在线实验验证了热毛细管式激光离子源的元素选择性和分离效率。

形变核179Pt在束γ谱学和重丰中子新核素的合成及其衰变性质研究

本论文分为两部分，分别沿自旋和同位旋自由度开展研究工作。第一部分介绍原子核高自旋态研究的相关背景知识、基础理论等，描述在束γ谱学研究的实验技术和方法，分析和讨论形变核179Pt转动带能级结构的特性，并采用相关理论对其进行分析。通过融合蒸发反应149sm（35cl，P4n）布居奇A核179Pt的高自旋激发态。指认179Pt的组态为1／2-［521］，5／2-［512〕和7／2＋〔633〕的三条转动带。在hco＝0．27 Mev附近，观测到1／2-〔521］带内顺排角动量突然增大，建议该现象是由一对113／2中子发生顺排造成的。另外观察到在7／2＋〔633］带中出现较大的旋称劈裂。建议由于三轴形变加强了波函数中来自几＝1／2轨道的组分，从而导致较大的旋称劈裂的出现。论文第二部分介绍重丰中子核衰变性质研究以及新核素合成、鉴别工作的相关背景知识、理论基础及实验技术。并对相关的研究工作分别进行阐述。通过快中子反应合成并鉴别了新核素19705和新的同核异能素186rnTa，利用γ（x）谱学方法首次建立了19705的部分衰变纲图。测得它们的半衰期分别为2.8士0.6 min和1.50.1 min，并与理论计算结果进行了比较；进行了原子核基态β延发裂变（pDF）的实验研究，经测量首次发现了230Ac的两个pDF事件，测得23OAc的pDF几率为(1.19±0.40)

143Pm高自旋态和重丰中子新核素的合成及衰变性质研究

本论文从内容上可以分为两大部分：第一部分：对近球形核~(143)Pm高自旋态进行的在束γ研究。这一部分是本文的重点。利用能量为82和90 MeV的~(19)F束流，通过融合蒸发反应~(128)Te (~(19)F,4nγ) ~(143)Pm布局~(143)Pm的高自旋态。利用联合在束装置(JIBGE)的10套带BGO反康的HPGe探测器进行了标准在束γ谱学测量，包括γ射线的激发函数、γ单谱、γ-γ-t符合谱以及DCO测量。在已有工作的基础上，建立了~(143)Pm激发能高达10.5 MeV，自旋约为(61/2)h的高自旋态能级结构。观测到了28条新的跃迁能级和48条新的γ射线。对两个已知的同质异能态寿命进行了提取，并在8 MeV激发能附近进行了高自旋态同质异能态的搜索。以~(142)Nd，~(144)Sm为核实，用零级弱耦合模型对~(143)Pm的晕态能级结构进行了定量的解释。计算表明，直到激发能Ex = 6.77 MeV，自旋宇称J~π = (37/2~+)的晕态能级都可以用弱耦合模型进行很好的解释。但是，对于更高激发能的能级，组态情况要复杂的多，有出现N = 82中子闭壳打破的可能。同时，利用大基壳模型OXBASH程序对其能级结构进行了计算和讨论，其结果支持弱耦合模型的假设。第二部分：利用中能重离子的多核子转移反应，(~(186)W-2p + 2n)，(~(238)U-2p + 2n)对丰中子核~(186)Hf和~(238)Th进行了合成和鉴别。测量它们的半衰期分别为(2.6 ± 1.2) min和 (9.4 ± 2.0) min，与用质子一中子准粒子随机相近似方法的预言值是相符的。同时，对β延发裂变先驱核~(230)Ac进行了实验研究。观测到了它的两个裂变事件，得到~(230)Acβ延发裂变几率为(1.19 ± 0.85) * 10~(-8)。从而使~(230)Ac成为世界上第一种被确认了的基态β延发裂变先驱核。

中子核和铅区核的结构研究

我们首先用Woods-Saxon势对一些丰中子核进行了系统的计算．计算表明在Woods-Saxon势中考虑一个对称能项，Woods-Saxon势就能够很好的描述丰中子核的密度分布，单粒子能级结构和中子质子的均方根半径．用Woods Saxon势的计算结果表明中子皮是丰中子远离β稳定线核的普遍现象。2S1/2轨道与1d 5/2轨道的交又和2s1d壳与1p壳的壳崩渍是中子晕形成的重要原因，也是中子晕与中子皮的一个重要区别．壳模型的计算能够很好的再现9《A《14和3《Z《5丰中子核的许多性质，这表明了，改进壳模型的有效相互作用，壳模型可能能够描述远离核的性质． 我们208Ti一类核和206Pb的一些性质进行了系统的壳模型计算．计算结果表明，K-H和SDI等有效相互作用对描述208Ti一类核和206Pb的高激发态仍然是有效的，计算结果也表明，如果208Hg可供利用的β衰变能比206Hg小，则可以预计208Hg的半寿命比206Hg要长.计算还证实了在反应209Bi（ρ，a )206Pb中激发的206Pb激发态结构，与205Tl低激发态结构相似，即这些态可以用h9/2轨道上的一个质子与205T1的低激发态的弱耦合来描述，此即所谓的对应的相似多重态的概念． 最后，我们对11Li等中子晕核的束缚机制提出了一种新的关联机制和讨论了用壳模型描述集体运动的方法．

Laser Driven Nuclear Physics at ELI–NP

High power lasers have proven being capable to produce high energy γ-rays, charged particles and neutrons, and to induce all kinds of nuclear reactions. At ELI, the studies with high power lasers will enter for the first time into new domains of power and intensities: 10 PW and 10^23 W/cm^2. While the development of laser based radiation sources is the main focus at the ELI-Beamlines pillar of ELI, at ELI-NP the studies that will benefit from High Power Laser System pulses will focus on Laser Driven Nuclear Physics (this TDR, acronym LDNP, associated to the E1 experimental area), High Field Physics and QED (associated to the E6 area) and fundamental research opened by the unique combination of the two 10 PW laser pulses with a gamma beam provided by the Gamma Beam System (associated to E7 area). The scientific case of the LDNP TDR encompasses studies of laser induced nuclear reactions, aiming for a better understanding of nuclear properties, of nuclear reaction rates in laser-plasmas, as well as on the development of radiation source characterization methods based on nuclear techniques. As an example of proposed studies: the promise of achieving solid-state density bunches of (very) heavy ions accelerated to about 10 MeV/nucleon through the RPA mechanism will be exploited to produce highly astrophysical relevant neutron rich nuclei around the N~126 waiting point, using the sequential fission-fusion scheme, complementary to any other existing or planned method of producing radioactive nuclei.

The studies will be implemented predominantly in the E1 area of ELI-NP. However, many of them can be, in a first stage, performed in the E5 and/or E4 areas, where higher repetition laser pulses are available, while the harsh X-ray and electromagnetic pulse (EMP) environments are less damaging compared to E1.

A number of options are discussed through the document, having an important impact on the budget and needed resources. Depending on the TDR review and subsequent project decisions, they may be taken into account for space reservation, while their detailed design and implementation will be postponed.

The present TDR is the result of contributions from several institutions engaged in nuclear physics and high power laser research. A significant part of the proposed equipment can be designed, and afterwards can be built, only in close collaboration with (or subcontracting to) some of these institutions. A Memorandum of Understanding (MOU) is currently under preparation with each of these key partners as well as with others that are interested to participate in the design or in the future experimental program.

Radiological protection and nuclear engineering studies in multi-MW target systems

Tese de doutoramento, Física, Universidade de Lisboa, Faculdade de Ciências, 2014

Pauli distorted double folded potential

The enhancement in the production of even-Z nuclei observed in nuclear fission has also been observed in fragments produced from heavy ion collsions. Beams of 40Ar, 40Cl, and 40Ca at 25 MeV/nucleon were impinged on 58Fe and 58Ni targets. The resulting fragments were detected using the MSU 4pi detector array, which had additional silicon detectors for better isotopic resolution. Comparison of the ratios of yields for each element showed enhancement of even-Z fragment production. The enhancement was more pronounced for reactions with a greater difference in the N/Z of the compound system. However, this effect was less for systems that were more neutron rich. The average N/Z for fragments also displayed an odd-even effect with a lower average N/Z for the even-Z fragments. This is related to the greater availability of neutron-poor isotopes for even-Z nuclei

First Results with the RISING active stopper

This paper outlines some of the physics opportunities available with the GSI RISING active stopper and presents preliminary results from an experiment aimed at performing beta-delayed gamma-ray spectroscopic studies in heavy-neutron-rich nuclei produced following the projectile fragmentation of a 1 GeV per nucleon 208Pb primary beam. The energy response of the silicon active stopping detector for both heavy secondary fragments and beta-particles is demonstrated and preliminary results on the decays of neutron-rich Tantalum (Ta) to Tungsten (W) isotopes are presented as examples of the potential of this technique to allow new structural studies in hitherto experimentally unreachable heavy, neutron-rich nuclei. The resulting spectral information inferred from excited states in the tungsten daughter nuclei are compared with results from axially symmetric Hartree–Fock calculations of the nuclear shape and suggest a change in ground state structure for the N = 116 isotone 190W compared to the lighter isotopes of this element.

The effect of the tensor force on the predicted stability of superheavy nuclei

The effect of the tensor component of the Skyrme effective nucleon-nucleon interaction on the single-particle structure in superheavy elements is studied. A selection of the available Skyrme forces has been chosen and their predictions for the proton and neutron shell closures investigated. The inclusion of the tensor term with realistic coupling strength parameters leads to a small increase in the spin-orbit splitting between the proton 2f7/2 and 2f5/2 partners, opening the Z=114 shell gap over a wide range of nuclei. The Z=126 shell gap, predicted by these models in the absence of the tensor term, is found to be stongly dependent on neutron number with a Z=138 gap opening for large neutron numbers, having a consequent implication for the synthesis of neutron-rich superheavy elements. The predicted neutron shell structures remain largely unchanged by inclusion of the tensor component.

Astrophysical S factors for fusion reactions involving C, O, Ne, and Mg isotopes

Using the Sao Paulo potential and the barrier penetration formalism we have calculated the astrophysical factor S(E) for 946 fusion reactions involving stable and neutron-rich isotopes of C, O, Ne, and Mg for center-of-mass energies E varying from 2 to approximate to 18-30 MeV (covering the range below and above the Coulomb barrier). We have parameterized the energy dependence, S(E), by an accurate universal 9-parameter analytic expression and present tables of fit parameters for all the reactions. We also discuss the reduced 3-parameter version of our fit which is highly accurate at energies below the Coulomb barrier, and outline the procedure for calculating the reaction rates. The results can be easily converted to thermonuclear or pycnonuclear reaction rates to simulate various nuclear burning phenomena, in particular, stellar burning at high temperatures and nucleosynthesis in high density environments. (C) 2010 Elsevier Inc. All rights reserved

Universal aspects of light halo nuclei

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)