Quark-Gluon Plasma

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出版者:Elsevier Science Ltd
作者:Kapusta, Joseph I. (EDT)/ Muller, Berndt (EDT)/ Rafelski, Johann (EDT)
出品人:
页数:836
译者:
出版时间:2003-12
价格:$ 350.30
装帧:HRD
isbn号码:9780444511102
丛书系列:
图书标签:
  • 夸克胶子等离子体
  • 相对论重离子碰撞
  • 强相互作用
  • 量子色动力学
  • 高温物质
  • 相变
  • 粒子物理学
  • 核物理学
  • 重离子物理
  • 实验物理
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具体描述

The purpose of this volume is to trace the development of the theoretical understanding of quark-gluon plasma, both in terms of the equation of state and thermal correlation functions and in terms of its manifestation in high energy nuclear collisions. Who among us has not wondered how tall a mountain is on a neutron star, what happens when matter is heated and compressed to higher and higher densities, what happens when an object falls into a black hole, or what happened eons ago in the early universe? The study of quark-gluon plasma is related in one way or another to these and other thought provoking questions. Oftentimes the most eloquent exposition is given in the original papers. To this end a selection is made of what are the most important pioneering papers in this field. The early 1950s was an era when high energy multiparticle production in cosmic ray interactions attracted the attention of some of the brightest minds in physics, and so it should be no surprise that the first reprinted papers deal with the introduction of statistical models of particle production. The quark model arose in the 1960s, while QCD as such was recognized as the theory of the strong interactions in the 1970's. The behavior of matter at high temperatures and supranuclear densities became of wide interest in the nuclear and particle physics communities starting in the 1970s, which is when the concept of quark-gluon plasma became established. The history of the field has been traced up to the early 1990s. There are three reasons for stopping at that point in time. First, most of the key theoretical concepts and formalisms arose before 1993, although many of them continue to be developed today and hopefully well into the future. Second, papers written after 1992 are much more readily available than those writen before due to the advent of the World Wide Web and its electronic preprint databases and journals. Finally, in making this collection of reprints available as hardcopy one is limited in the number of pages, and some papers in the present selection should have been deleted in order to make room for post-1993 papers. For the same reason the subject focus must of necessity be limited, which means that in this reprint collection two wide subject areas are not addressed: the behavior of nuclear matter under extreme conditions is not reported, nor is quark matter in neutron stars. The broad categories into which the material has been placed, reflect the diverse studies of quark-gluon plasma and its manifestation. They are: phase-space models of particle production, perturbative QCD plasma, lattice gauge theory, fluid dynamics and flow, strangeness, heavy flavor (charm), electromagnetic signals, parton cascade and minijets, parton energy loss and jet quenching, Hanbury Brown-Twiss (HBT) interferometry, disoriented chiral condensates, phase transition dynamics and cosmology, and color superconductivity. Each chapter is prefaced by an introduction, which contains a list of significant papers which is more complete than the reprinted papers, though by no means exhaustive. It also contains citations to most relevant papers published up to the date of completion of this volume (fall 2002). It is hoped that the short reviews will help bring the reader up to date on the latest developments. The selection of papers cited in each chapter, and in particular the ones selected for reprinting, is solely the responsibility of the Editors. It is based on their best judgement and experience in this field dating back to the mid-1970s. In order to be reprinted a paper must have been pioneering in the sense of originality and impact on the field. Generally they have been cited over a hundred times by other papers published in refereed journals. The final selection was reviewed and discussed among the Editors repeatedly. Just because a paper is not included does not mean they do not know of it or do not have a high regard for it. All of the papers cited or reprinted are original research contributions. There are three other types of publications listed. The first is a compilation of books. The second is a list of reviews, many of which contain a significant amount of original material. The third is a list of the proceedings of the series of Quark Matter meetings, the primary series of international conferences in this field that is attended by both theorists and experimentalists.

好的,以下是一份关于“夸克-胶子等离子体”的书籍简介,内容将详细阐述该主题,同时避免提及您原先的书名,并力求自然流畅,不带有明显的机械生成痕迹。 --- 跨越物质极限:探索宇宙最极端状态的奥秘 本书旨在引导读者深入探究物质存在的最奇特、最极端的形态之一:由基本粒子——夸克和胶子——构成的流体。这不仅仅是一本面向专业物理学家的教科书,更是一部为所有对宇宙起源、基本粒子物理以及核物理前沿领域抱有浓厚兴趣的求知者准备的深度导览。 第一部分:基础的重构——从原子核到基本构件 要理解这种奇异物质的特性,我们必须首先回归到我们所熟知的一切物质的基石。我们从标准模型的粒子物理学基础讲起,详细阐述夸克和胶子的存在及其在强相互作用(QCD)框架下的行为。 强相互作用的精髓: 深入剖析量子色动力学(QCD)的数学结构,重点讨论渐近自由(Asymptotic Freedom)和夸克禁闭(Confinement)这两个核心概念。渐近自由解释了在极高能量或极短距离下,夸克和胶子如何近乎自由地运动;而夸克禁闭则解释了为何我们从未观测到孤立的自由夸克。 核子的结构: 探讨质子和中子的内部结构,它们并非不可分割的“点状”粒子,而是由价夸克、海夸克(Sea Quarks)以及胶子云层构成的复杂系统。理解这种“组装”的必要性,是理解如何“解开”这些粒子,进入等离子体状态的关键一步。 温度与密度的尺度: 设定理解的背景。我们讨论何为“临界温度”和“临界密度”,这些参数是区分普通核物质与极端物质状态的物理边界。我们通过宇宙学和天体物理学的视角,明确指出在何种环境下才能达到这种状态。 第二部分:相变之路——从强子到等离子体 本书的核心部分将聚焦于物质相变的物理过程,即强子物质(如原子核内部的物质)如何在高能、高密度的驱动下“融化”成夸克-胶子等离子体(QGP)。 加热的理论模型: 我们详细考察理论物理学家们如何计算这种相变。从格子QCD(Lattice QCD)的无模型计算到微扰QCD的尝试,对比不同方法在预测临界点上的异同。重点分析了临界点(Critical End Point)的理论意义及其在相图中的位置。 “熔化”的本质: 这种相变不是简单的固态变液态,而是一种拓扑结构和对称性的恢复。当温度和密度足够高时,QCD中的自发对称性被恢复,夸克和胶子获得了运动的自由度,物质的“颜色场”不再被限制在单个强子内部。 流体动力学描述: 一旦形成QGP,它不再表现为离散的粒子集合,而是表现出惊人的流体特性。我们引入相对论性流体动力学(Relativistic Hydrodynamics)来描述这种物质的膨胀和冷却过程,并探讨其极其低的粘滞度,将其比拟为“最完美的流体”。 第三部分:实验的视野——在地球上重现早期宇宙 理论的构建必须依赖于实验的验证。本书的后半部分将深入探讨人类如何通过最强大的粒子加速器,在地球上模拟宇宙诞生后最初的微秒内所存在的环境。 重离子碰撞: 详细介绍重离子加速器(如RHIC和LHC)的工作原理,特别是如何将金原子核(Gold)或铅原子核(Lead)加速到接近光速,然后使其迎头相撞。碰撞的能量密度是产生QGP的关键。 信号的提取与分析: 碰撞产生QGP后,它会迅速冷却并“冻结”成各种强子和轻子。我们探讨如何通过探测碰撞产生的各种“信使”来推断QGP的性质: 喷注衰减(Jet Quenching): 高能夸克或胶子在穿越QGP时会损失能量,形成“喷注”。分析这些喷注能量的损失,是测量QGP“粘度”和“密度”的直接证据。 夸美子生产(Quarkonia Suppression): 重夸克对(如粲夸克对)在形成QGP时会因“颜色屏蔽效应”而溶解。分析J/ψ等夸美子的产生率变化,是衡量QGP形成与否的关键指标。 集体流动的证据: 利用椭圆形碰撞的几何形状,分析产出粒子的角度分布(如各向异性流,Elliptic Flow),从而确认QGP具有流体的特性。 第四部分:宇宙的遥远回响——天体物理学的连接 QGP不仅是加速器中的短暂现象,它也与宇宙的宏大尺度演化紧密相连。 早期宇宙的演化: 将QGP的存在与宇宙大爆炸后的前几微秒联系起来,讨论早期宇宙的物质状态及其对后续结构形成的影响。 中子星的内部: 探讨极端密度下的物质状态是否可能在致密星体——中子星的内部有所体现。如果中子星的核心压力超过某一阈值,物质是否会演变为超密核物质,甚至更奇异的夸克物质态? 结语:开放的前沿 本书的最后部分将总结当前研究的未解之谜:我们对粘滞度的理解是否已经完善?临界点的精确位置在哪里?未来下一代探测器将如何帮助我们更精细地刻画这种宇宙中最炽热、最致密的物质形态? 本书通过严谨的物理学框架、翔实的实验数据分析,以及对理论模型构建的细致阐述,全面描绘了这一迷人且复杂的物理领域。它是一扇通往物质极限探索的窗口,邀请读者一同思考构成我们世界的最底层逻辑。

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