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Speedups in nonequilibrium thermal relaxation: Mpemba and related effects 非平衡热松弛中的加速:Mpemba和相关效应
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-12-08 DOI: 10.1016/j.physrep.2025.10.009
Gianluca Teza , John Bechhoefer , Antonio Lasanta , Oren Raz , Marija Vucelja
Most of our intuition about the behavior of physical systems is shaped by observations at or near thermal equilibrium. However, even a basic phenomenon such as a thermalquench can lead to states far from thermal equilibrium, where counterintuitive,anomalous effects can occur. A prime example of anomalous thermal relaxation is the Mpemba effect, in which a system prepared at a hot temperature cools down to the temperature of the cold environment faster than an identical system prepared at a warm temperature. Although originally reported for water more than 2000 years ago by Aristotle, the recent observation of analogous relaxation speedups in a variety of systems has motivated the search for generic explanations from the point of view of nonequilibrium statistical mechanics. Here, we review anomalous relaxation effects, which all share a nonmonotonic dependence of relaxation time versus initial “distance” from the final state or from the phase transition. We review the early water experiments and classify the zoology of anomalous relaxation phenomena related to the Mpemba effect. We then introduce general concepts and provide a modern definition of the effect, focusing on the theoretical frameworks of stochastic thermodynamics, kinetic theory, Markovian dynamics, and phase transitions. We discuss the recent experimental and numerical developments that followed these theoretical advances. These developments paved the way for the prediction and observation of novel phenomena, such as the inverse Mpemba effect. The review is self-contained and introduces anomalous relaxation phenomena in single- and many-body systems, both classical and quantum. We also discuss the broader relevance of the Mpemba effect, including its relation with equilibrium and dynamical phase transitions and its experimental implications. We end with perspectives that connect anomalous speedups to new ideas for designing optimal heating/cooling protocols, heat engines, and efficient samplers.
我们对物理系统行为的大多数直觉都是由在热平衡或接近热平衡时的观察形成的。然而,即使是像热猝灭这样的基本现象也可能导致远离热平衡的状态,在这种状态下可能发生违反直觉的异常效应。反常热松弛的一个主要例子是Mpemba效应,在高温下制备的系统比在温暖温度下制备的相同系统更快地冷却到寒冷环境的温度。虽然亚里士多德早在2000多年前就报道了水的弛豫加速,但最近在各种系统中对类似弛豫加速的观察,促使人们从非平衡统计力学的角度寻求一般解释。在这里,我们回顾了反常弛豫效应,它们都具有弛豫时间与与最终状态或相变的初始“距离”的非单调依赖关系。我们回顾了早期的水实验,并对与姆潘巴效应有关的异常弛豫现象进行了动物学分类。然后,我们介绍了一般概念并提供了效应的现代定义,重点介绍了随机热力学、动力学理论、马尔可夫动力学和相变的理论框架。我们讨论了随着这些理论进步而来的最近的实验和数值发展。这些发展为预测和观察新现象铺平了道路,例如逆姆潘巴效应。这篇综述是独立的,介绍了单体和多体系统中的反常弛豫现象,包括经典和量子。我们还讨论了Mpemba效应的广泛相关性,包括它与平衡和动态相变的关系及其实验意义。我们以将异常加速与设计最佳加热/冷却协议,热机和高效采样器的新想法联系起来的观点结束。
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引用次数: 0
Review of neutral naturalness 回顾中性自然性
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-12-04 DOI: 10.1016/j.physrep.2025.12.001
Brian Batell , Matthew Low , Ethan T. Neil , Christopher B. Verhaaren
The hierarchy between the mass parameter of the Higgs boson and larger mass scales becomes ever more puzzling as experiments explore higher energies. Neutral naturalness is the umbrella term for symmetry-based explanations for these hierarchies whose quark symmetry partners are not charged under the SU(3)c color gauge group of the Standard Model. Though the first manifestations of this idea predate the physics runs of the Large Hadron Collider, since the Higgs discovery this paradigm has grown and developed to include a wide variety of concrete realizations with connections to intriguing collider signals. Determining the phenomenology of such models often requires the characterization—typically relying on lattice calculations—of a new confining gauge symmetry. This presents additional motivation to further develop our understanding of nonperturbative field theory as well as to pursue specific lattice studies. The wide range of suggested hidden sectors also produces a variety of dark matter candidates, intersections with astrophysics and cosmology, and ties to neutrinos and flavor. In this review, we orient the reader within both this growing collection of specific models and the physical phenomena they produce. We also survey the often less familiar dynamics of hidden-sector glueballs and quirks. In addition to providing a guide to past efforts, we reveal interesting directions for further study.
随着实验探索更高的能量,希格斯玻色子的质量参数和更大的质量尺度之间的层次关系变得越来越令人困惑。中性自然性是对这些层次的基于对称性的解释的总称,这些层次的夸克对称伙伴在标准模型的SU(3)c色规群下不带电。虽然这个想法的第一个表现早于大型强子对撞机的物理运行,但自从希格斯发现以来,这个范式已经发展壮大,包括了各种各样的具体实现,这些实现与有趣的对撞机信号有关。要确定这类模型的现象学,通常需要对一种新的限定规范对称进行表征(通常依赖于点阵计算)。这为进一步发展我们对非微扰场论的理解以及进行具体的晶格研究提供了额外的动力。广泛的隐藏扇区也产生了各种各样的暗物质候选者,与天体物理学和宇宙学的交叉点,以及与中微子和风味的联系。在这篇综述中,我们将引导读者了解这些不断增长的特定模型和它们产生的物理现象。我们还调查了隐藏领域的胶球和怪癖的动态,这些动态通常不太为人所知。除了对过去的努力提供指导外,我们还揭示了进一步研究的有趣方向。
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引用次数: 0
Vertical structure and dynamics of a galactic disk 星系盘的垂直结构和动力学
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-12-02 DOI: 10.1016/j.physrep.2025.11.003
Chanda J. Jog
Most of the visible mass in a typical spiral galaxy is distributed in a thin disk, with a radial extent much larger than its thickness. While the planar disk structure, including non-axisymmetric features such as spiral structure, has been studied extensively, the vertical structure normal to the disk plane has not received comparable attention. This review aims to give a comprehensive, pedagogic introduction to the rich topic of vertical structure of a galactic disk in hydrostatic equilibrium, and discuss the theoretical developments in this field in the context of recent observations. A realistic multi-component disk plus halo model of a galaxy has been developed and studied by us in detail. This takes account of both stars and interstellar gas, treated as isothermal components with different velocity dispersions, which are gravitationally coupled; further, the disk is in the gravitational field of the dark matter halo. This review focuses on this model and the results from it in different physical cases.
The gas and halo crucially affect the resulting self-consistent stellar distribution such that it is vertically constrained to be closer to the mid-plane, and has a steeper profile than in the standard one-component case, in agreement with modern observations. The scale height of a typical stellar disk increases with galactocentric radius; that is, the disk flares, by a factor of few within the visible radial extent of the disk. These robust results question the sech2 profile and a constant scale height, routinely used in the literature for convenience. In an important application, the observed HI gas scale height is used as a constraint on the model which helps determine the shape and the density profile of the dark matter halo for galaxies. Finally, we outline some key, open questions which can be addressed in the near future using the above model, and new observational data — for example, from the IFU surveys and JWST. These promise to give a better understanding of this topic.
在典型的螺旋星系中,大部分可见质量分布在一个薄圆盘上,其径向范围远远大于其厚度。平面盘面结构,包括螺旋结构等非轴对称特征,已经得到了广泛的研究,而垂直于盘面的垂直结构却没有得到足够的重视。本文旨在对流体静力平衡中星系盘的垂直结构这一丰富的主题进行全面的教学介绍,并在最近的观测背景下讨论这一领域的理论发展。我们建立并详细研究了一个真实的多组分星系盘加晕模型。这考虑了恒星和星际气体,它们被视为具有不同速度色散的等温成分,它们是引力耦合的;此外,这个圆盘处于暗物质晕的引力场中。本文将重点介绍该模型及其在不同物理情况下的结果。气体和光晕对最终的自洽恒星分布产生了至关重要的影响,使其在垂直方向上受到约束,更靠近中间平面,并且比标准的单组分情况具有更陡峭的轮廓,这与现代观测一致。典型恒星盘的尺度高度随着星系中心半径的增大而增大;也就是说,在可见的圆盘径向范围内,圆盘耀斑的因子很少。这些强大的结果质疑sech2剖面和恒定尺度高度,通常在文献中使用方便。在一个重要的应用中,观测到的HI气体尺度高度被用作模型的约束,这有助于确定星系暗物质晕的形状和密度分布。最后,我们概述了一些关键的、悬而未决的问题,这些问题可以在不久的将来使用上述模型和新的观测数据(例如来自IFU调查和JWST的数据)来解决。这些承诺提供了一个更好的理解这个主题。
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引用次数: 0
Dissipative optical solitons: From scalar 1D- to 2D- and 3D-, topological and vector solitons 耗散光孤子:从标量一维到二维和三维,拓扑和矢量孤子
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-12-02 DOI: 10.1016/j.physrep.2025.11.005
Nikolay N. Rosanov, Sergey V. Fedorov, Nikolay A. Veretenov
In this review we present the current status of the theory of dissipative optical solitons — light packets localized due to the balance of inflow (positive dissipation) and outflow (negative dissipation) of energy, and give references on the experiments in the field. We mention various mechanisms of radiation localization and the premises leading to this concept, and briefly compare the physics and properties of conservative, under conditions of negligible dissipation, and dissipative, with the balance of energy inflow and outflow, optical solitons. We shortly discuss the general properties of electromagnetic pulses and the formulation of paraxial radiation propagation in dissipative media. The characteristics of two important classes of spatial and spatiotemporal dissipative optical solitons are described in detail: those in driven wide-aperture nonlinear interferometers and in relative laser schemes without and with driving. An example of what is apparently the only exactly solvable problem in the field is given, clearly demonstrating the connection of these solitons with optical bistability and switching waves. The nontrivial internal structure of the solitons under consideration, related to the distribution of radiation energy fluxes, is explained, and the results of the analysis of the interaction of solitons and the formation of soliton complexes are presented. Particular attention is paid to the nature of the motion of these structures and its connection with their symmetry. Similarly, studied are the issues of topological optics of dissipative solitons, related to the presence of uncertainties (topological singularities) of the field phase and/or polarization state. Vector solitons are considered for 1D, 2D and 3D cases revealing their connections with the scalar ones and underlying their new dynamical features. Quantum fluctuations in dissipative solitons and extremely short solitons are considered more briefly.
本文综述了耗散光孤子理论的研究现状,即由于能量流入(正耗散)和流出(负耗散)平衡而局部化的光包,并对该领域的实验进行了参考。我们提到了辐射局部化的各种机制和导致这一概念的前提,并简要地比较了在可忽略耗散条件下的保守性和光孤子的物理和性质,以及能量流入和流出的平衡。我们简要地讨论了电磁脉冲的一般性质和耗散介质中近轴辐射传播的公式。详细描述了两类重要的时空耗散光孤子的特性:驱动型大孔径非线性干涉仪中的孤子,以及非驱动型和有驱动型激光方案中的孤子。给出了一个显然是该领域唯一可以精确解决的问题的例子,清楚地证明了这些孤子与光双稳性和开关波的联系。解释了所考虑的孤子的非平凡内部结构与辐射能量通量的分布有关,并给出了孤子相互作用和孤子复合体形成的分析结果。特别注意的是这些结构的运动性质及其与对称性的联系。同样,研究了耗散孤子的拓扑光学问题,涉及到场相位和/或偏振态的不确定性(拓扑奇点)的存在。一维、二维和三维情况下的矢量孤子揭示了它们与标量孤子的联系,并揭示了它们新的动力学特征。耗散孤子和极短孤子中的量子涨落被更简单地考虑。
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引用次数: 0
Precision cross-sections for advancing cosmic-ray physics and other applications: A comprehensive programme for the next decade 推进宇宙射线物理学和其他应用的精密截面:下一个十年的综合方案
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-11-15 DOI: 10.1016/j.physrep.2025.11.002
D. Maurin , L. Audouin , E. Berti , P. Coppin , M. Di Mauro , P. von Doetinchem , F. Donato , C. Evoli , Y. Génolini , P. Ghosh , I. Leya , M.J. Losekamm , S. Mariani , J.W. Norbury , L. Orusa , M. Paniccia , T. Poeschl , P.D. Serpico , A. Tykhonov , M. Unger , L. Šerkšnytė
Cosmic-ray physics in the GeV-to-TeV energy range has entered a precision era thanks to recent data from space-based experiments. However, the poor knowledge of nuclear reactions, in particular for the production of antimatter and secondary nuclei, limits the information that can be extracted from these data, such as source properties, transport in the Galaxy and indirect searches for particle dark matter. The Cross-Section for Cosmic Rays at CERN workshop series has addressed the challenges encountered in the interpretation of high-precision cosmic-ray data, with the goal of strengthening emergent synergies and taking advantage of the complementarity and know-how in different communities, from theoretical and experimental astroparticle physics to high-energy and nuclear physics. In this paper, we present the outcomes of the third edition of the workshop that took place in 2024. We present the current state of cosmic-ray experiments and their perspectives, and provide a detailed road map to close the most urgent gaps in cross-section data, in order to efficiently progress on many open physics cases, which are motivated in the paper. Finally, with the aim of being as exhaustive as possible, this report touches several other fields – such as cosmogenic studies, space radiation protection and hadrontherapy – where overlapping and specific new cross-section measurements, as well as nuclear code improvement and benchmarking efforts, are also needed. We also briefly highlight further synergies between astroparticle and high-energy physics on the question of cross-sections.
由于最近来自太空实验的数据,gev到tev能量范围内的宇宙射线物理学已经进入了一个精确的时代。然而,对核反应,特别是反物质和次级核的产生的知识贫乏,限制了可以从这些数据中提取的信息,例如源特性、银河系中的传输和对粒子暗物质的间接搜索。欧洲核子研究中心宇宙射线截面研讨会系列讨论了在解释高精度宇宙射线数据时遇到的挑战,其目标是加强新兴的协同作用,利用从理论和实验天体粒子物理学到高能和核物理学等不同领域的互补性和专业知识。在本文中,我们介绍了2024年举行的第三届研讨会的成果。我们介绍了宇宙射线实验的现状和他们的观点,并提供了一个详细的路线图,以填补截面数据中最紧迫的空白,以便有效地推进许多开放的物理案例,这是本文的动机。最后,为了尽可能详尽,本报告涉及其他几个领域- -例如宇宙形成研究、空间辐射保护和强子疗法- -在这些领域也需要重叠和具体的新横截面测量,以及核代码改进和基准工作。我们还简要地强调了天体粒子和高能物理在横截面问题上的进一步协同作用。
{"title":"Precision cross-sections for advancing cosmic-ray physics and other applications: A comprehensive programme for the next decade","authors":"D. Maurin ,&nbsp;L. Audouin ,&nbsp;E. Berti ,&nbsp;P. Coppin ,&nbsp;M. Di Mauro ,&nbsp;P. von Doetinchem ,&nbsp;F. Donato ,&nbsp;C. Evoli ,&nbsp;Y. Génolini ,&nbsp;P. Ghosh ,&nbsp;I. Leya ,&nbsp;M.J. Losekamm ,&nbsp;S. Mariani ,&nbsp;J.W. Norbury ,&nbsp;L. Orusa ,&nbsp;M. Paniccia ,&nbsp;T. Poeschl ,&nbsp;P.D. Serpico ,&nbsp;A. Tykhonov ,&nbsp;M. Unger ,&nbsp;L. Šerkšnytė","doi":"10.1016/j.physrep.2025.11.002","DOIUrl":"10.1016/j.physrep.2025.11.002","url":null,"abstract":"<div><div>Cosmic-ray physics in the GeV-to-TeV energy range has entered a precision era thanks to recent data from space-based experiments. However, the poor knowledge of nuclear reactions, in particular for the production of antimatter and secondary nuclei, limits the information that can be extracted from these data, such as source properties, transport in the Galaxy and indirect searches for particle dark matter. The <em>Cross-Section for Cosmic Rays at CERN</em> workshop series has addressed the challenges encountered in the interpretation of high-precision cosmic-ray data, with the goal of strengthening emergent synergies and taking advantage of the complementarity and know-how in different communities, from theoretical and experimental astroparticle physics to high-energy and nuclear physics. In this paper, we present the outcomes of the third edition of the workshop that took place in 2024. We present the current state of cosmic-ray experiments and their perspectives, and provide a detailed road map to close the most urgent gaps in cross-section data, in order to efficiently progress on many open physics cases, which are motivated in the paper. Finally, with the aim of being as exhaustive as possible, this report touches several other fields – such as cosmogenic studies, space radiation protection and hadrontherapy – where overlapping and specific new cross-section measurements, as well as nuclear code improvement and benchmarking efforts, are also needed. We also briefly highlight further synergies between astroparticle and high-energy physics on the question of cross-sections.</div></div>","PeriodicalId":404,"journal":{"name":"Physics Reports","volume":"1161 ","pages":"Pages 1-81"},"PeriodicalIF":29.5,"publicationDate":"2025-11-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145527942","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Topological physics in quantum critical systems 量子临界系统中的拓扑物理学
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-11-13 DOI: 10.1016/j.physrep.2025.10.005
Xue-Jia Yu , Limei Xu , Hai-Qing Lin
Topology forms a cornerstone in modern condensed matter and statistical physics, offering a new framework to classify the phases and phase transitions beyond the traditional Landau paradigm. However, it is widely believed that topological properties are destroyed when the bulk energy gap closes, making it highly nontrivial to consider topology in gapless quantum critical systems. To address these challenges, recent advancements have sought to generalize the notion of topology to systems without a bulk energy gap, including quantum critical points and critical phases, collectively referred to as gapless symmetry-protected topological states. Extending topology to gapless quantum critical systems challenges the traditional belief in condensed matter physics that topological edge states are typically tied to the presence of a bulk energy gap. Furthermore, it suggests that topology plays a crucial role in classifying quantum phase transitions even if they belong to the same universality class, fundamentally enriching the textbook understanding of phase transitions. Given its importance, here we give a pedagogical review of the current progress of topological physics in quantum critical systems. We introduce the topological properties of quantum critical points and generalize them to stable critical phases, both for noninteracting and interacting systems. Additionally, we discuss further generalizations and future directions, including higher dimensions, nonequilibrium phase transitions, and realizations in modern experiments.
拓扑学是现代凝聚态物理和统计物理的基石,它提供了一种超越传统朗道范式的相和相变分类的新框架。然而,人们普遍认为,当体能隙关闭时,拓扑性质会被破坏,这使得在无间隙量子临界系统中考虑拓扑变得非常重要。为了应对这些挑战,最近的进展试图将拓扑概念推广到没有大块能量间隙的系统,包括量子临界点和临界相,统称为无间隙对称保护拓扑状态。将拓扑扩展到无间隙量子临界系统挑战了凝聚态物理中拓扑边缘状态通常与体能隙存在相关的传统信念。此外,它表明拓扑在量子相变分类中起着至关重要的作用,即使它们属于同一个普适类,从根本上丰富了教科书对相变的理解。鉴于其重要性,我们在此对量子临界系统中拓扑物理学的当前进展进行了教学回顾。我们引入量子临界点的拓扑性质,并将其推广到非相互作用和相互作用系统的稳定临界相。此外,我们还讨论了进一步的推广和未来的方向,包括更高的维度,非平衡相变,以及在现代实验中的实现。
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引用次数: 0
Quantum complexity in gravity, quantum field theory, and quantum information science 引力、量子场论和量子信息科学中的量子复杂性
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-11-12 DOI: 10.1016/j.physrep.2025.11.001
Stefano Baiguera , Vijay Balasubramanian , Pawel Caputa , Shira Chapman , Jonas Haferkamp , Michal P. Heller , Nicole Yunger Halpern
Quantum complexity quantifies the difficulty of preparing a state or implementing a unitary transformation with limited resources. Applications range from quantum computation to condensed matter physics and quantum gravity. We seek to bridge the approaches of these fields, which define and study complexity using different frameworks and tools. We describe several definitions of complexity, along with their key properties. In quantum information theory, we focus on complexity growth in random quantum circuits. In quantum many-body systems and quantum field theory (QFT), we discuss a geometric definition of complexity in terms of geodesics on the unitary group. In dynamical systems, we explore a definition of complexity in terms of state or operator spreading, as well as concepts from tensor-networks. We also outline applications to simple quantum systems, quantum many-body models, and QFTs including conformal field theories (CFTs). Finally, we explain the proposed relationship between complexity and gravitational observables within the holographic anti-de Sitter (AdS)/CFT correspondence.
量子复杂性量化了用有限的资源准备状态或实现统一转换的难度。应用范围从量子计算到凝聚态物理和量子引力。我们试图将这些领域的方法连接起来,这些领域使用不同的框架和工具来定义和研究复杂性。我们描述了复杂性的几种定义,以及它们的关键属性。在量子信息理论中,我们关注随机量子电路的复杂性增长。在量子多体系统和量子场论中,我们讨论了复杂性在酉群上的测地线的几何定义。在动态系统中,我们从状态或算子扩展的角度探讨复杂性的定义,以及张量网络的概念。我们还概述了在简单量子系统、量子多体模型和包括共形场理论(CFTs)在内的qft中的应用。最后,我们在全息反德西特(AdS)/CFT对应中解释了复杂性与引力观测之间的关系。
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引用次数: 0
Cascading from N=2 supersymmetric Yang–Mills theory to confinement and chiral symmetry breaking in adjoint QCD 从N=2超对称杨-米尔斯理论级联到伴随QCD中的约束和手性对称性破缺
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-11-08 DOI: 10.1016/j.physrep.2025.10.007
Eric D’Hoker , Thomas T. Dumitrescu , Efrat Gerchkovitz , Emily Nardoni
<div><div>We argue that adjoint QCD in <span><math><mrow><mn>3</mn><mo>+</mo><mn>1</mn></mrow></math></span> dimensions, with any <span><math><mrow><mi>S</mi><mi>U</mi><mrow><mo>(</mo><mi>N</mi><mo>)</mo></mrow></mrow></math></span> gauge group and two Weyl fermion flavors (i.e. one adjoint Dirac fermion), confines and spontaneously breaks its chiral symmetries via the condensation of a fermion bilinear. We flow to this theory from pure <span><math><mrow><mi>N</mi><mo>=</mo><mn>2</mn></mrow></math></span> SUSY Yang–Mills theory with the same gauge group, by giving a SUSY-breaking mass <span><math><mi>M</mi></math></span> to the scalars in the <span><math><mrow><mi>N</mi><mo>=</mo><mn>2</mn></mrow></math></span> vector multiplet. This flow can be analyzed rigorously at small <span><math><mi>M</mi></math></span>, where it leads to a deconfined vacuum at the origin of the <span><math><mrow><mi>N</mi><mo>=</mo><mn>2</mn></mrow></math></span> Coulomb branch. The analysis can be extended to all <span><math><mi>M</mi></math></span> using an Abelian dual description that arises from the <span><math><mi>N</mi></math></span> multi-monopole points of the <span><math><mrow><mi>N</mi><mo>=</mo><mn>2</mn></mrow></math></span> theory. At each such point, there are <span><math><mrow><mi>N</mi><mo>−</mo><mn>1</mn></mrow></math></span> hypermultiplet Higgs fields <span><math><msubsup><mrow><mi>h</mi></mrow><mrow><mi>m</mi></mrow><mrow><mi>i</mi><mo>=</mo><mn>1</mn><mo>,</mo><mn>2</mn></mrow></msubsup></math></span>, which are <span><math><mrow><mi>S</mi><mi>U</mi><msub><mrow><mrow><mo>(</mo><mn>2</mn><mo>)</mo></mrow></mrow><mrow><mi>R</mi></mrow></msub></mrow></math></span> doublets. We provide a detailed study of the phase diagram as a function of <span><math><mi>M</mi></math></span>, by analyzing the semi-classical phases of the dual using a combination of analytic and numerical techniques. The result is a cascade of first-order phase transitions, along which the Higgs fields <span><math><msubsup><mrow><mi>h</mi></mrow><mrow><mi>m</mi></mrow><mrow><mi>i</mi></mrow></msubsup></math></span> successively turn on, and which interpolates between the Coulomb branch at small <span><math><mi>M</mi></math></span>, where all <span><math><mrow><msubsup><mrow><mi>h</mi></mrow><mrow><mi>m</mi></mrow><mrow><mi>i</mi></mrow></msubsup><mo>=</mo><mn>0</mn></mrow></math></span>, and a maximal Higgs branch, where all <span><math><mrow><msubsup><mrow><mi>h</mi></mrow><mrow><mi>m</mi></mrow><mrow><mi>i</mi></mrow></msubsup><mo>≠</mo><mn>0</mn></mrow></math></span>, at sufficiently large <span><math><mi>M</mi></math></span>. We show that this maximal Higgs branch precisely matches the confining and chiral symmetry breaking phase of two-flavor adjoint QCD, including its broken and unbroken symmetries, its massless spectrum, and the expected large-<span><math><mi>N</mi></math></span> scaling of various observables. The spontaneous breaking pattern <span><math><mrow><mi>S</mi><mi>U</mi
我们认为在3+1维空间中,任意SU(N)规范群和两种Weyl费米子(即一种伴随狄拉克费米子)的伴随QCD,通过费米子双线性的凝聚限制并自发地破坏了其手性对称性。我们从具有相同规范群的纯N=2 SUSY Yang-Mills理论出发,通过给N=2向量多重中的标量一个SUSY破断质量M,推导出该理论。这种流动可以在小M处进行严格的分析,它在N=2库仑分支的原点处导致一个确定的真空。利用由N=2理论的N个多单极点产生的阿贝尔对偶描述,可以将分析推广到所有M个点。在每一个这样的点上,有N−1个超多重希格斯场hmi=1,2,它们是SU(2)R双重态。我们通过结合解析和数值技术分析对偶的半经典相,对相图作为M的函数进行了详细的研究。结果是一个一阶相变级联,希格斯场hmi依次开启,并在小M处的库仑分支(所有hmi=0)和最大希格斯分支(所有hmi≠0)之间插入,在足够大的M处。我们表明,这个最大希格斯分支精确匹配双味伴随QCD的限制和手性对称性破缺相,包括它的破缺对称性和未破缺对称性,它的无质量谱,以及各种观测值的大n尺度。对偶中hmi的复杂对准机制保证了SU(2)R→U(1)R的自发破断模式符合vfa - witten定理,并导致沿级联半径增加的P1 σ模型。
{"title":"Cascading from N=2 supersymmetric Yang–Mills theory to confinement and chiral symmetry breaking in adjoint QCD","authors":"Eric D’Hoker ,&nbsp;Thomas T. Dumitrescu ,&nbsp;Efrat Gerchkovitz ,&nbsp;Emily Nardoni","doi":"10.1016/j.physrep.2025.10.007","DOIUrl":"10.1016/j.physrep.2025.10.007","url":null,"abstract":"&lt;div&gt;&lt;div&gt;We argue that adjoint QCD in &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mn&gt;3&lt;/mn&gt;&lt;mo&gt;+&lt;/mo&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; dimensions, with any &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;S&lt;/mi&gt;&lt;mi&gt;U&lt;/mi&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;mi&gt;N&lt;/mi&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; gauge group and two Weyl fermion flavors (i.e. one adjoint Dirac fermion), confines and spontaneously breaks its chiral symmetries via the condensation of a fermion bilinear. We flow to this theory from pure &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;N&lt;/mi&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; SUSY Yang–Mills theory with the same gauge group, by giving a SUSY-breaking mass &lt;span&gt;&lt;math&gt;&lt;mi&gt;M&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt; to the scalars in the &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;N&lt;/mi&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; vector multiplet. This flow can be analyzed rigorously at small &lt;span&gt;&lt;math&gt;&lt;mi&gt;M&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;, where it leads to a deconfined vacuum at the origin of the &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;N&lt;/mi&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; Coulomb branch. The analysis can be extended to all &lt;span&gt;&lt;math&gt;&lt;mi&gt;M&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt; using an Abelian dual description that arises from the &lt;span&gt;&lt;math&gt;&lt;mi&gt;N&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt; multi-monopole points of the &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;N&lt;/mi&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; theory. At each such point, there are &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;N&lt;/mi&gt;&lt;mo&gt;−&lt;/mo&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; hypermultiplet Higgs fields &lt;span&gt;&lt;math&gt;&lt;msubsup&gt;&lt;mrow&gt;&lt;mi&gt;h&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;m&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;i&lt;/mi&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;mn&gt;1&lt;/mn&gt;&lt;mo&gt;,&lt;/mo&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;/mrow&gt;&lt;/msubsup&gt;&lt;/math&gt;&lt;/span&gt;, which are &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;S&lt;/mi&gt;&lt;mi&gt;U&lt;/mi&gt;&lt;msub&gt;&lt;mrow&gt;&lt;mrow&gt;&lt;mo&gt;(&lt;/mo&gt;&lt;mn&gt;2&lt;/mn&gt;&lt;mo&gt;)&lt;/mo&gt;&lt;/mrow&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;R&lt;/mi&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; doublets. We provide a detailed study of the phase diagram as a function of &lt;span&gt;&lt;math&gt;&lt;mi&gt;M&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;, by analyzing the semi-classical phases of the dual using a combination of analytic and numerical techniques. The result is a cascade of first-order phase transitions, along which the Higgs fields &lt;span&gt;&lt;math&gt;&lt;msubsup&gt;&lt;mrow&gt;&lt;mi&gt;h&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;m&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;i&lt;/mi&gt;&lt;/mrow&gt;&lt;/msubsup&gt;&lt;/math&gt;&lt;/span&gt; successively turn on, and which interpolates between the Coulomb branch at small &lt;span&gt;&lt;math&gt;&lt;mi&gt;M&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;, where all &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;msubsup&gt;&lt;mrow&gt;&lt;mi&gt;h&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;m&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;i&lt;/mi&gt;&lt;/mrow&gt;&lt;/msubsup&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;, and a maximal Higgs branch, where all &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;msubsup&gt;&lt;mrow&gt;&lt;mi&gt;h&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;m&lt;/mi&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mi&gt;i&lt;/mi&gt;&lt;/mrow&gt;&lt;/msubsup&gt;&lt;mo&gt;≠&lt;/mo&gt;&lt;mn&gt;0&lt;/mn&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;, at sufficiently large &lt;span&gt;&lt;math&gt;&lt;mi&gt;M&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;. We show that this maximal Higgs branch precisely matches the confining and chiral symmetry breaking phase of two-flavor adjoint QCD, including its broken and unbroken symmetries, its massless spectrum, and the expected large-&lt;span&gt;&lt;math&gt;&lt;mi&gt;N&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt; scaling of various observables. The spontaneous breaking pattern &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;S&lt;/mi&gt;&lt;mi&gt;U&lt;/mi","PeriodicalId":404,"journal":{"name":"Physics Reports","volume":"1158 ","pages":"Pages 1-99"},"PeriodicalIF":29.5,"publicationDate":"2025-11-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145465066","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Human mobility in epidemic modeling 流行病建模中的人类流动性
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-11-07 DOI: 10.1016/j.physrep.2025.10.010
Xin Lu , Jiawei Feng , Shengjie Lai , Petter Holme , Shuo Liu , Zhanwei Du , Xiaoqian Yuan , Siqing Wang , Yunxuan Li , Xiaoyu Zhang , Yuan Bai , Xiaojun Duan , Wenjun Mei , Hongjie Yu , Suoyi Tan , Fredrik Liljeros
Human mobility forms the backbone of contact patterns through which infectious diseases propagate, fundamentally shaping the spatio-temporal dynamics of epidemics and pandemics. While traditional models are often based on the assumption that all individuals have the same probability of infecting every other individual in the population, a so-called random homogeneous mixing, they struggle to catch the complex and heterogeneous nature of real-world human interactions. Recent advancements in data-driven methodologies and computational capabilities have unlocked the potential of integrating high-resolution human mobility data into epidemic modeling, significantly improving the accuracy, timeliness, and applicability of epidemic risk assessment, contact tracing, and intervention strategies. This review provides a comprehensive synthesis of the current landscape in human mobility-informed epidemic modeling. We explore several data sources and representations of human mobility, and examine the behavioral and structural roles of mobility and contact in shaping disease transmission dynamics. Furthermore, the review spans a wide range of epidemic modeling approaches, ranging from classical compartmental models to network-based, agent-based, and machine learning models. It also discusses how mobility integration enhances risk management and response strategies during epidemics. By synthesizing these insights, the review can serve as a foundational resource for researchers and practitioners, bridging the gap between epidemiological theory and the dynamic complexities of human interaction while charting clear directions for future research.
人类的流动构成了传染病传播的接触模式的主干,从根本上塑造了流行病和大流行的时空动态。虽然传统模型通常基于这样的假设,即所有个体感染人群中其他个体的概率相同,即所谓的随机同质混合,但它们很难捕捉到现实世界人类互动的复杂性和异质性。数据驱动方法和计算能力方面的最新进展,释放了将高分辨率人类流动性数据整合到流行病建模中的潜力,显著提高了流行病风险评估、接触者追踪和干预策略的准确性、及时性和适用性。这篇综述提供了一个全面综合的当前景观在人类流动知情的流行病建模。我们探索了几个数据源和人类流动性的表示,并检查了流动性和接触在塑造疾病传播动力学中的行为和结构作用。此外,该综述涵盖了广泛的流行病建模方法,从经典的隔间模型到基于网络的模型、基于代理的模型和机器学习模型。它还讨论了流动一体化如何在流行病期间加强风险管理和应对战略。通过综合这些见解,该综述可以作为研究人员和从业人员的基础资源,弥合流行病学理论与人类互动动态复杂性之间的差距,同时为未来的研究指明明确的方向。
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引用次数: 0
A review on computational assessment of biomedical markers in carotid arteries 颈动脉生物医学标志物的计算评估研究进展
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-11-04 DOI: 10.1016/j.physrep.2025.10.008
Kaveh Moghadasi , Mergen H. Ghayesh , Jiawen Li , Eric Hu , Robert Fitridge
This review aims to explore advanced computational assessment approaches for carotid artery research by providing a comprehensive overview focusing on different theoretical and modelling techniques. As a key vessel, the carotid artery supplies oxygenated blood to the head and the brain. The vertebral arteries are smaller than the carotid arteries and supply to posterior part of the brain. The carotid and vertebral arteries meet at the base of the skull, forming the Circle of Willis which provides collateral flow to the brain when one artery is occluded. Understanding the biomedical markers and structural response of the carotid artery is essential to evaluate progression and risks associated with atherosclerosis, which is a leading cause of stroke and other cardiovascular events. In addition to atherosclerosis, the analysis will be complemented by a discussion of other less common carotid artery conditions. The review comprises a comprehensive evaluation of biomechanical research of the carotid artery by categorising articles into three broad approaches, namely structure analysis, computational fluid dynamics, and fluid–structure interaction. By summarising recent advancements and identifying existing knowledge gaps, this paper highlights the potential of integrative modelling approaches to enhance diagnostics, risk assessment, and the development of targeted treatments for carotid artery diseases.
本文旨在通过对不同理论和建模技术的全面概述,探索颈动脉研究的先进计算评估方法。颈动脉作为重要血管,为头部和大脑提供含氧血液。椎动脉比颈动脉小,供应脑后部。颈动脉和椎动脉在颅骨底部汇合,形成威利斯圈,当其中一条动脉闭塞时,它向大脑提供侧支血流。了解颈动脉的生物医学标志物和结构反应对于评估与动脉粥样硬化相关的进展和风险至关重要,动脉粥样硬化是中风和其他心血管事件的主要原因。除了动脉粥样硬化外,本文还将讨论其他不太常见的颈动脉疾病。这篇综述包括对颈动脉生物力学研究的综合评价,将文章分为三大类,即结构分析、计算流体动力学和流固相互作用。通过总结最近的进展和确定现有的知识差距,本文强调了综合建模方法在加强颈动脉疾病的诊断、风险评估和靶向治疗发展方面的潜力。
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引用次数: 0
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