用相互作用玻色子模型对O(6)核进行微观计算

T. Mizusaki, T. Otsuka
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引用次数: 30

摘要

我们利用OAI映射方法,提出了基于壳模型相互作用的相互作用玻色子模型(IBM)的微观计算。我们用Hartree-Fock - Bogoluibov (HFB)守恒数和质子-中子tam - dancoff方法确定了与IBM玻色子对应的集体对,并考虑了与非集体自由度的耦合。本文对Te、Xe和Ba同位素进行了实际计算。其中,Xe同位素在许多现象学研究中显示出0(6)对称性。我们提出了清晰的0(6)对称的光谱和波函数,这是显微镜下获得的。中、中重核的低洼谱显示出简单而规则的结构,尽管这些核由许多相互作用的质子和中子组成,其动力学本质上是非常复杂的。这就是所谓的集体运动。特别是,在偶偶核的情况下,能级和电磁跃迁有相当简单和共同的特征。对它们的理解一直是核结构的主要问题之一。许多理论被提倡、发展和扩展。其中,由Arima和Iachello在20世纪70年代首次提出的相互作用玻色子模型(IBM), 1)- 6)已经证明是相当成功的。在IBM中,核子集体对是用玻色子来表示的。这个概念可以简化核子多体系统的处理。此外,这一分析有利于群体理论处理。最初,s和d玻色子是s (J = 0)和d (J = 2)核子对的对应物,是作为IBM的构建块引入的。因为这些玻色子不能区分质子和中子的自由度,所以这些玻色子对应的核子对是不明确的。但是,s和d玻色子跨越U(6)空间,其包含0(3)子群的基团链在物理上对应于振动、旋转和“不稳定”核作为极限情况。这些群链是U(5)、SU(3)和0(6)极限。与其他集体模型不同,IBM可以为我们提供除了U(5)和SU(3)原子核之外的0(6)原子核的清晰描述。有许多原子核,它们的光谱显示了这些群理论极限的模式。此外,由于原始IBM空间的维数最多约为100,因此通过对角化哈密顿量可以很容易地处理三个极限之间的中间情况。在这一阶段,进行了许多现象学工作,表明许多偶偶核的低洼态可以用IBM的六个参数统一解释。这些参数被认为是
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Microscopic Calculations for O(6) Nuclei by the Interacting Boson Model
We present microscopic calculations of the Interacting Boson Model (IBM) based on the shell model interaction by using the OAI mapping approach. We determine the col­ lective pairs, which correspond to the IBM bosons, by the number conserved Hartree-Fock­ Bogoluibov (HFB) and the proton-neutron Tamm-Dancoff methods, and we take into consid­ eration couplings to the non-collective degrees of freedom. The present realistic calculations are carried out for the Te, Xe and Ba isotopes. Among them, the Xe isotopes are known by numerous phenomenological works to show the 0(6) symmetry. We present the clear 0(6) symmetry in the spectra and the wave function which are microscopically obtained. Low-lying spectra of medium and medium-heavy nuclei show simple and regular structures, although these nuclei consist of many interacting protons and neutrons and their dynamics is intrinsically very complicate. This is known to be the collec­ tive motion. Especially, in the case of even-even nuclei, there are quite simpler and common features in energy levels and electro-magnetic transitions. The understand­ ing of them has been one of the main problems in nuclear structure. Many theories have been advocated, developed and extended. Among them, the Interacting Boson Model (IBM), l)- 6 ) which was first introduced by Arima and Iachello in the 1970's, has shown to be rather successful. In the IBM, nucleon collective pairs are approximated in terms of bosons. This notion can simplify the treatment of the nucleon many-body system. Furthermore this ansatz facilitates the group theoretical treatment. Originally s and d bosons, which are counterparts of S(J = 0) and D(J = 2) nucleon pairs, are introduced as the building blocks of the IBM. Because these bosons do not distinguish the proton and neutron degrees of freedom, the nucleon pair counterparts of these bosons are ambiguous. But, the s and d bosons span a U(6) space and its group chains containing the 0(3) subgroup correspond physically to vibrational, rotational and '"'( unstable nuclei as limiting cases. These group chains are U(5), SU(3) and 0(6) limits. Unlike to other collective models, the IBM can give us a clear description of the 0(6) nuclei besides the U(5) and SU(3) nuclei. There are many nuclei, the spectra of which show the pattern of these group theoretical limits. Furthermore the intermediate situations between three limits are easily tractable by diagonalization of the Hamiltonian because the dimension of the original IBM space is at most about one hundred. At this stage, many phenomenological works were carried out, which showed that the low-lying states of many even-even nuclei can be explained by using six parameters of the IBM in a unified way. These parameters are considered to
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