Dominance of gluonic scale anomaly in confining pressure inside nucleon and D-term

IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Daisuke Fujii , Mamiya Kawaguchi , Mitsuru Tanaka
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引用次数: 0

Abstract

We explore the confining pressure inside the nucleon and the related gravitational form factor referred to as the D-term, using the skyrmion approach based on the scale-invariant chiral perturbation theory, where the skyrmion is described as the nucleon and a scalar meson couples to the scale anomaly through the low energy theorem. Within this model framework, the current quark mass and gluonic quantum contributions to the scale anomaly can be described by the pion and scalar meson masses, respectively, through matching with the underlying QCD. By considering the decomposition of the energy momentum tensor of nucleon, we examine the role of the scale anomaly contributions in the pressure inside the nucleon. As a result, the gluonic scale anomaly is found to dominate the confining pressure. Compared to the result based on the conventional chiral perturbation theory in the chiral limit, our result for the total pressure is capable of qualitatively improving the alignment with lattice QCD observations. Moreover, the pressure from the gluonic scale anomaly is widely distributed in position space, leading to its substantial contribution to the D-term.
核子和d项围压胶子尺度异常的优势
我们利用基于尺度不变手性微扰理论的斯基米子方法探索了核子内部的围压和相关的引力形式因子d项,其中斯基米子通过低能定理被描述为核子和一个标量介子对尺度异常的耦合。在这个模型框架内,当前夸克质量和胶子量子对尺度异常的贡献可以分别用介子质量和标量介子质量来描述,通过与底层QCD的匹配。通过考虑核子能量动量张量的分解,考察了尺度异常贡献在核子内部压力中的作用。结果表明,胶子尺度异常对围压起主导作用。与传统手性微扰理论在手性极限下的结果相比,我们的总压力结果能够定性地改善与晶格QCD观测的对准性。胶子尺度异常压力在位置空间上分布广泛,对d项的贡献较大。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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