Pauli nonlocality and the nucleon effective mass

IF 3.1 2区 物理与天体物理 Q1 Physics and Astronomy
Dao T. Khoa, Doan Thi Loan, Nguyen Hoang Phuc
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Abstract

A study of the nucleon mean-field potential in nuclear matter (NM) is done within an extended Hartree-Fock (HF) formalism, using the CDM3Y6 density dependent version of the M3Y interaction which is associated with the nuclear incompressibility K252 MeV. The momentum dependence of nucleon optical potential (OP) in NM at the saturation density ρ0 is shown to be due mainly to its exchange term up to k2fm1, so that the Pauli nonlocality is expected to be the main origin of the nucleon effective mass at low momenta. Because nucleons in neutron-rich NM at ρρ0 are either weakly bound or unbound by the in-medium nucleon-nucleon interaction, the determination of the effective mass of nucleon scattered on targets with neutron excess at low energies should be of interest for the mean-field studies of neutron star matter. For this purpose, the folding model is used to calculate the nonlocal nucleon OP for the optical model analysis of elastic nucleon scattering on Ca40,48, Zr90, and Pb208 targets at energies E<50 MeV, to probe the model reliability and validate the Wentzel-Kramers-Brillouin (WKB) local approximation to obtain the local folded nucleon OP. The nucleon effective mass m* is then carefully deduced from the momentum dependence of the local folded nucleon OP which results from the Pauli nonlocality of the exchange term. The obtained m* values agree well with the nucleon effective mass given by the extended HF calculation of the single-particle potential in asymmetric NM. The neutron-proton effective mass splitting determined at ρρ0 from the central strength of the real folded nucleon OP for Ca48, Zr90, and Pb208 targets has been found to depend linearly on the neutron-proton asymmetry parameter as mnp*(0.167±0.018)δ, in a good agreement with the recent empirical constraints.

Abstract Image

保利非局域性与核子有效质量
利用与核不可压缩性 K≃252 MeV 有关的 M3Y 相互作用的 CDM3Y6 密度依赖版本,在扩展的哈特里-福克(HF)形式主义中对核物质(NM)中的核子均场势进行了研究。结果表明,在饱和密度ρ0 时,核子光学势(OP)的动量依赖性主要归因于高达 k≈2fm-1 的交换项,因此预计保利非位置性是低动量时核子有效质量的主要来源。由于ρ≈ρ0 时富含中子的 NM 中的核子要么受到中子-核子相互作用的弱束缚,要么没有受到束缚,因此测定低能时散射在中子过剩目标上的核子有效质量对于中子星物质的均场研究应该是有意义的。为此,我们利用折叠模型计算了非局部核子OP,用于能量为E<50 MeV时Ca40,48、Zr90和Pb208靶上弹性核子散射的光学模型分析,以探究模型的可靠性,并验证Wentzel-Kramers-Brillouin(WKB)局部近似以获得局部折叠核子OP。然后根据交换项的保利非局域性导致的局部折叠核子 OP 的动量依赖性仔细推导出核子有效质量 m*。得到的 m* 值与不对称 NM 单粒子势的扩展高频计算所给出的核子有效质量非常吻合。根据 Ca48、Zr90 和 Pb208 目标的真实折叠核子 OP 的中心强度确定的 ρ≈ρ0 处的中子-质子有效质量分裂与中子-质子不对称参数 mn-p*≈(0.167±0.018)δ 呈线性关系,这与最近的经验约束非常吻合。
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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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