[公式省略]-玻色子传播子的热和重子密度修正

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Alejandro Ayala , José Jorge Medina-Serna , Isabel Domínguez , Ivonne Maldonado , María Elena Tejeda-Yeomans
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引用次数: 0

摘要

为了探索外围重离子碰撞产生的涡旋运动如何转化为反应富重子区的强子自旋,我们计算了有限温度和有限重子密度下的σ-介子传播子。该传播子编码了主要由核子组成的介质的性质,并可用于模拟日冕中强子之间的主要相互作用。我们计算了单环σ自能的近似值,该近似值解释了大的核子质量。从自能实部得到色散关系,表明σ-质量有不可忽略的热化学和重子化学贡献。从虚部,我们还计算了谱密度,我们表明它包含了与朗道阻尼相关的分支切断的一部分。我们也给出了小动量和大动量情况下的色散关系和极点剩余的近似,并补充了计算,提供了传播子满足的和规则。本研究的目的是确定计算反应的电晕区的涡旋运动如何被转移到Λ超子的自旋上所需的元素之一,这些超子可以通过σ介子交换与核子相互作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Thermal and baryon density modifications to the σ-boson propagator
Motivated by the search of the way the vortical motion produced in peripheral heavy-ion collisions is transferred to the spin of hadrons in the baryon-rich zone of the reaction, we compute the σ-meson propagator at finite temperature and baryon density. This propagator encodes the properties of a medium consisting mainly of nucleons and can be used to model the main interactions between hadrons in the corona. We compute the one-loop σ self-energy in an approximation that accounts for the large nucleon mass. From the real part of the self-energy, we find the dispersion relation and show that the σ-mass receives a non-negligible thermal and baryon chemical dependent contribution. From the imaginary part, we also compute the spectral density, which we show to contain a piece coming from the branch cut associated with Landau damping. We also present approximations for the dispersion relation and the residue at the pole in the small- and large-momentum regimes and complement the calculation, providing the sum rules satisfied by the propagator. This study aims to determine one of the elements needed to compute how the vortical motion in the corona region of the reaction is transferred to the spin of Λ hyperons that can interact with nucleons by σ-meson exchange.
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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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