微观方法中奇数-偶数核变形的加拉格尔-莫兹科夫斯基分裂

IF 3.4 2区 物理与天体物理 Q1 Physics and Astronomy
L. Bonneau, N. Kontowicz, J. Bartel, H. Molique, Meng-Hock Koh (辜明福), N. Minkov
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引用次数: 0

摘要

背景:长期以来,人们基本上是在 "转子+双准粒子 "图景中描述轴向增殖变形奇多核中的低洼带头态。这种方法可以解释所谓的加拉格尔-莫兹科夫斯基(Gallagher-Moszkowski)双带头态(K=Ωn±Ωp,中子和质子角动量在对称轴上的投影之和与差)的出现。根据 Gallagher 和 Moszkowski 提出的经验法则,自旋对齐构型的能量低于自旋不对齐构型。Robledo、Bernard 和 Bertsch 最近的一项研究[Phys. Rev. C 89, 021303(R) (2014)]显示,在 Gogny 能量密度函数中,非成对核子的自洽阻断计算在大约一半的情况下无法重现这一规则,并指出该函数的密度依赖项是导致这一失败的原因。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Gallagher-Moszkowski splitting in deformed odd-odd nuclei within a microscopic approach

Gallagher-Moszkowski splitting in deformed odd-odd nuclei within a microscopic approach
Background: Low-lying bandhead states in axially prolate deformed odd-odd nuclei have long been described essentially within the rotor+two-quasiparticle picture. This approach allows one to explain the appearance of so-called Gallagher-Moszkowski doublets of bandheads with K=Ωn±Ωp, sum and difference of neutron and proton angular momentum projections on the symmetry axis. According to an empirical rule stated by Gallagher and Moszkowski the spin-aligned configuration lies lower in energy than the spin-antialigned configuration. A recent study by Robledo, Bernard, and Bertsch [Phys. Rev. C 89, 021303(R) (2014)] within the Gogny energy-density functional with self-consistent blocking of the unpaired nucleons showed that calculations fail to reproduce this rule in about half of the cases, and points to the density-dependent term of the functional as responsible of this failure.
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来源期刊
Physical Review C
Physical Review C 物理-物理:核物理
CiteScore
5.70
自引率
35.50%
发文量
0
审稿时长
1-2 weeks
期刊介绍: Physical Review C (PRC) is a leading journal in theoretical and experimental nuclear physics, publishing more than two-thirds of the research literature in the field. PRC covers experimental and theoretical results in all aspects of nuclear physics, including: Nucleon-nucleon interaction, few-body systems Nuclear structure Nuclear reactions Relativistic nuclear collisions Hadronic physics and QCD Electroweak interaction, symmetries Nuclear astrophysics
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