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Space astrometry with Gaia: Advances in understanding our Galaxy 盖亚的空间天体测量:了解银河系的进展
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-10-22 DOI: 10.1016/j.physrep.2025.09.004
Michael Perryman
Gaia is a satellite mission of the European Space Agency which is creating a catalogue of extremely accurate positions, distances and space motions of two billion stars in our Galaxy, along with more than one hundred thousand solar system asteroids, and several million distant quasars, all on the same extragalactic reference system. Complementary information on each object’s multi-epoch photometry and spectra provides a vast and unprecedented data base of (model-dependent) fundamental physical quantities, such as each star’s mass, age, and chemical composition. I outline the field’s historical context, and explain the key principles involved in these space measurements. This is followed by a broad review of the many areas of solar system science, stellar structure and evolution, and topics in Galactic structure, evolution, and dynamics, that are being derived from these data.
盖亚是欧洲航天局的一项卫星任务,它正在创建一个目录,其中包含我们银河系中20亿颗恒星的极其精确的位置、距离和空间运动,以及10万多颗太阳系小行星和数百万颗遥远的类星体,所有这些都在同一个星系外参考系统中。每个天体的多历元光度和光谱的补充信息提供了一个巨大的、前所未有的(依赖于模型的)基本物理量的数据库,比如每颗恒星的质量、年龄和化学成分。我概述了该领域的历史背景,并解释了这些空间测量所涉及的关键原则。接下来是对太阳系科学,恒星结构和演化的许多领域的广泛回顾,以及银河系结构,演化和动力学的主题,这些都是从这些数据中得出的。
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引用次数: 0
The future of secure communications: Device independence in quantum key distribution 安全通信的未来:量子密钥分发中的设备独立性
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-10-17 DOI: 10.1016/j.physrep.2025.09.006
Seyed Arash Ghoreishi , Giovanni Scala , Renato Renner , Letícia Lira Tacca , Jan Bouda , Stephen Patrick Walborn , Marcin Pawłowski
In the ever-evolving landscape of quantum cryptography, Device-independent Quantum Key Distribution (DI-QKD) stands out for its unique approach to ensuring security based not on the trustworthiness of the devices but on nonlocal correlations. Beginning with a contextual understanding of modern cryptographic security and the limitations of standard quantum key distribution methods, this review explores the pivotal role of nonclassicality and the challenges posed by various experimental loopholes for DI-QKD. Various protocols, security against individual, collective and coherent attacks, and the concept of self-testing are also examined, as well as the entropy accumulation theorem, and additional mathematical methods in formulating advanced security proofs. In addition, the burgeoning field of semi-device-independent models (measurement DI-QKD, Receiver DI-QKD, and One-sided DI-QKD) is also analyzed. The practical aspects are discussed through a detailed overview of experimental progress and the open challenges towards the commercial deployment in the future of secure communications.
在不断发展的量子密码学领域,与设备无关的量子密钥分发(DI-QKD)以其独特的方法脱颖而出,该方法不是基于设备的可信度,而是基于非局部相关性来确保安全性。本文从对现代密码安全的背景理解和标准量子密钥分发方法的局限性开始,探讨了非经典性的关键作用以及各种实验漏洞对DI-QKD带来的挑战。还研究了各种协议,针对个人,集体和连贯攻击的安全性,以及自我测试的概念,以及熵积累定理,以及制定高级安全性证明的附加数学方法。此外,还分析了新兴的半器件无关模型领域(测量型DI-QKD、接收机型DI-QKD和单侧型DI-QKD)。通过对实验进展的详细概述和对未来安全通信商业部署的公开挑战,讨论了实际方面。
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引用次数: 0
Information theory for complex systems scientists: What, why, and how 复杂系统科学家的信息理论:什么,为什么,如何
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-10-14 DOI: 10.1016/j.physrep.2025.09.007
Thomas F. Varley
In the 21st century, many of the crucial scientific and technical issues facing humanity can be understood as problems associated with understanding, modeling, and ultimately controlling complex systems: systems comprised of a large number of non-trivially interacting components whose collective behavior can be difficult to predict. Information theory, a branch of mathematics historically associated with questions about encoding and decoding messages, has emerged as something of a lingua franca for those studying complex systems, far exceeding its original narrow domain of communication systems engineering. In the context of complexity science, information theory provides a set of tools which allow researchers to describe a variety of dependencies, including interactions between the component parts of a system, interactions between a system and its environment, and the mereological interaction between the parts and the “whole”.
In this review aims to provide an accessible introduction to the core of modern information theory, aimed specifically at aspiring (and established) complex systems scientists. This includes standard measures, such as Shannon entropy, relative entropy, and mutual information, before building to more advanced topics, including: information dynamics, measures of statistical complexity, information decomposition, and effective network inference. In addition to detailing the formal definitions, we also make an effort to discuss how information theory can be interpreted and to develop the intuitions behind abstract concepts like “entropy”. The goal is to enable interested readers to understand what information is, and how it is used to better further their own research and education.
在21世纪,人类面临的许多关键科学和技术问题可以被理解为与理解、建模和最终控制复杂系统相关的问题:由大量非琐碎的相互作用组件组成的系统,其集体行为可能难以预测。信息论是数学的一个分支,历史上一直与信息的编码和解码问题有关,它已经成为研究复杂系统的人的通用语言,远远超出了它最初狭窄的通信系统工程领域。在复杂性科学的背景下,信息论提供了一套工具,使研究人员能够描述各种依赖关系,包括系统组成部分之间的相互作用,系统与其环境之间的相互作用,以及部分与“整体”之间的流变相互作用。在这篇综述的目的是提供一个可访问的介绍现代信息理论的核心,特别是针对有抱负的(和建立)复杂系统的科学家。这包括标准度量,如香农熵、相对熵和互信息,然后再构建更高级的主题,包括:信息动态、统计复杂性度量、信息分解和有效网络推理。除了详细说明形式定义之外,我们还努力讨论如何解释信息理论,并在“熵”等抽象概念背后发展直觉。目的是使感兴趣的读者了解什么是信息,以及如何利用信息更好地促进自己的研究和教育。
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引用次数: 0
Universal nonlinear dynamics in damped and driven physical systems: From Pendula via Josephson junctions to power grids 阻尼和驱动物理系统中的普遍非线性动力学:从钟摆到约瑟夫森结到电网
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-10-03 DOI: 10.1016/j.physrep.2025.09.005
Subrata Ghosh , Linuo Xue , Arindam Mishra , Suman Saha , Dawid Dudkowski , Syamal K. Dana , Tomasz Kapitaniak , Jürgen Kurths , Peng Ji , Chittaranjan Hens
Understanding the collective behavior of dynamical systems is essential for explaining various emergent phenomena in natural and engineered settings. A key step in this process is formulating an appropriate mathematical description of the individual systems and network of systems. In this context, a range of physical systems is considered here, including the classical pendula, superconducting Josephson junctions, power grids, and various others. Despite the diversity of the systems in terms of physical structure and their application domains, they exhibit strikingly similar dynamical features, namely, phase dynamics governed by inertia and damping, and in their response to external forcing. This observation creates interest and motivates a search for a unified theoretical framework capable of capturing the fundamentals of their dynamical behaviors exhibited across the systems. This review critically examines the up-to-date research activities on the dynamics of the second-order phase oscillator, henceforth claimed here as a universality class by its own merits as a simple nonlinear dynamical model representing a broad class of physical systems. It offers a common mathematical framework to develop a comprehensive understanding, from a general perspective, that bridges, the theoretical and experimental observations of pendulum motion, Josephson junctions, and power grids and their collective behaviors. While each of these systems has been discussed in disparate physical contexts, their underlying mathematical structures reveal strong commonalities. In particular, we highlight the importance of analyzing these systems through the lens of nonlinear phase dynamics to uncover their shared mechanisms and system-specific variety of behaviors as well. This survey mainly focuses on some specific interrelated themes: (i) collective phenomena and emergent synchronization; (ii) the role of heterogeneity in terms of system parameters and effects of noise on the emergent dynamics; (iii) multi-stability and complex transient regimes; (iv) the integration of machine learning for model discovery, control, and prediction; and (v) the broader applicability of phase oscillator models across diverse domains beyond the canonical systems considered here. By systematically comparing the dynamical behaviors of the varied physical systems within a cohesive mathematical framework of second-order phase oscillators, this review seeks for the universal and distinctive features of nonlinear dynamics of the three systems, their collective behaviors such as emergent synchrony, partial synchrony, or chimera states, and specifically explains real-life phenomena, and crowd synchrony that may lead to a collapse of a footbridge and the failure of a power grid. Besides our main emphasis on these systems, brief notes have been added on other systems where this second-order phase model explains their dynamical properties. A broad synthesis on the topic will not only deepen our
理解动力系统的集体行为对于解释自然和工程环境中的各种紧急现象至关重要。这个过程的一个关键步骤是对单个系统和系统网络进行适当的数学描述。在这种情况下,这里考虑了一系列物理系统,包括经典钟摆、超导约瑟夫森结、电网和其他各种系统。尽管系统在物理结构和应用领域方面存在多样性,但它们表现出惊人的相似的动力学特征,即由惯性和阻尼控制的相动力学,以及它们对外部力的响应。这种观察引起了人们的兴趣,并激发了人们对一个统一的理论框架的探索,这个理论框架能够捕捉到它们在整个系统中表现出的动力学行为的基本原理。本文对二阶相振子动力学的最新研究活动进行了批判性的考察,二阶相振子由于其本身的优点,作为一个简单的非线性动力学模型,代表了广泛的物理系统,因此在这里被称为一个普适类。它提供了一个通用的数学框架来发展一个全面的理解,从一般的角度来看,桥梁,钟摆运动的理论和实验观察,约瑟夫森结,电网和他们的集体行为。虽然这些系统中的每一个都在不同的物理环境中进行了讨论,但它们的底层数学结构显示出很强的共性。特别是,我们强调通过非线性相位动力学的镜头分析这些系统的重要性,以揭示它们的共同机制和系统特定的各种行为。本研究主要集中在一些具体的相互关联的主题上:(i)集体现象和紧急同步;(ii)就系统参数而言,非均质性所扮演的角色,以及噪音对涌现动力的影响;多稳定和复杂的暂态状态;(iv)整合机器学习用于模型发现、控制和预测;(v)相位振荡器模型在不同领域的更广泛的适用性,超出了这里考虑的规范系统。通过在二阶相振子的数学框架内系统地比较不同物理系统的动力学行为,本综述寻求三种系统的非线性动力学的普遍和独特特征,它们的集体行为,如涌现同步、部分同步或嵌合体状态,并具体解释了现实生活中的现象。人群同步可能会导致人行天桥的倒塌和电网的故障。除了我们主要强调这些系统外,还对其他系统进行了简要说明,其中二阶相模型解释了它们的动力学性质。对该主题的广泛综合不仅将加深我们的理论理解,而且还将为自然和工程环境中复杂动力系统的任何设计和控制提供建议。
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引用次数: 0
Quantum entanglement in cosmology 宇宙学中的量子纠缠
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-09-26 DOI: 10.1016/j.physrep.2025.09.001
Alessio Belfiglio , Orlando Luongo , Stefano Mancini
We discuss recent progress in the study of entanglement within cosmological frameworks, focusing on both momentum and position-space approaches and also reviewing the possibility to directly extract entanglement from quantum fields. Entanglement generation in expanding spacetimes can be traced back to the phenomenon of gravitational particle production, according to which the background gravitational field may transfer energy and momentum to quantum fields. The corresponding entanglement amount and its mode dependence are both sensitive to the field statistics and to the details of spacetime expansion, thus encoding information about the background. Gravitational production processes also play a key role in addressing the quantum-to-classical transition of cosmological perturbations. In order to directly extract entanglement from quantum fields, local interactions with additional quantum systems, working as detectors, have been suggested, leading to the formulation of the entanglement harvesting protocol. Despite harvesting procedures are currently unfeasible from an experimental point of view, various proposals for implementation exist and a proper modeling of detectors and local interactions is crucial to address entanglement extraction via realistic setups. In the final part of the work, we address entanglement characterization in position space, primarily focusing on black hole spacetimes. We first investigate a possible interpretation of Bekenstein–Hawking black hole entropy in terms of the entanglement entropy arising in discrete quantum field theories, on account of the area law. Then, we discuss the resolution of the black hole information paradox via the gravitational fine-grained entropy formula, which provides a new way to compute the entropy of Hawking radiation and allows to preserve unitarity in black hole evaporation processes.
我们讨论了宇宙学框架内纠缠研究的最新进展,重点关注动量和位置空间方法,并回顾了直接从量子场提取纠缠的可能性。膨胀时空中纠缠的产生可以追溯到引力粒子产生的现象,根据这种现象,背景引力场可能将能量和动量传递给量子场。相应的纠缠量及其模式依赖性对场统计量和时空展开的细节都很敏感,从而编码了背景信息。引力产生过程在解决宇宙学扰动的量子到经典跃迁方面也起着关键作用。为了直接从量子场中提取纠缠,已经提出了与作为探测器的附加量子系统的局部相互作用,从而形成了纠缠收获协议。尽管从实验的角度来看,收集过程目前是不可行的,但存在各种实施建议,并且通过实际设置解决纠缠提取的探测器和局部相互作用的适当建模至关重要。在工作的最后一部分,我们讨论了位置空间中的纠缠特性,主要关注黑洞时空。我们首先根据面积定律,从离散量子场论中产生的纠缠熵出发,研究了贝肯斯坦-霍金黑洞熵的一种可能解释。然后,我们讨论了用引力细粒度熵公式解决黑洞信息悖论,这为霍金辐射熵的计算提供了一种新的方法,并允许在黑洞蒸发过程中保持一致性。
{"title":"Quantum entanglement in cosmology","authors":"Alessio Belfiglio ,&nbsp;Orlando Luongo ,&nbsp;Stefano Mancini","doi":"10.1016/j.physrep.2025.09.001","DOIUrl":"10.1016/j.physrep.2025.09.001","url":null,"abstract":"<div><div>We discuss recent progress in the study of entanglement within cosmological frameworks, focusing on both momentum and position-space approaches and also reviewing the possibility to directly extract entanglement from quantum fields. Entanglement generation in expanding spacetimes can be traced back to the phenomenon of gravitational particle production, according to which the background gravitational field may transfer energy and momentum to quantum fields. The corresponding entanglement amount and its mode dependence are both sensitive to the field statistics and to the details of spacetime expansion, thus encoding information about the background. Gravitational production processes also play a key role in addressing the quantum-to-classical transition of cosmological perturbations. In order to directly extract entanglement from quantum fields, local interactions with additional quantum systems, working as detectors, have been suggested, leading to the formulation of the entanglement harvesting protocol. Despite harvesting procedures are currently unfeasible from an experimental point of view, various proposals for implementation exist and a proper modeling of detectors and local interactions is crucial to address entanglement extraction via realistic setups. In the final part of the work, we address entanglement characterization in position space, primarily focusing on black hole spacetimes. We first investigate a possible interpretation of Bekenstein–Hawking black hole entropy in terms of the entanglement entropy arising in discrete quantum field theories, on account of the area law. Then, we discuss the resolution of the black hole information paradox via the gravitational fine-grained entropy formula, which provides a new way to compute the entropy of Hawking radiation and allows to preserve unitarity in black hole evaporation processes.</div></div>","PeriodicalId":404,"journal":{"name":"Physics Reports","volume":"1146 ","pages":"Pages 1-47"},"PeriodicalIF":29.5,"publicationDate":"2025-09-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145134896","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
Vegetation dynamics: Modeling, mechanisms, and emergent properties 植被动力学:建模、机制和涌现特性
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-09-22 DOI: 10.1016/j.physrep.2025.09.003
Li-Feng Hou , Li Li , Renfei Chen , Yong-Ping Wu , Guo-Lin Feng , Gui-Quan Sun
As a core component of terrestrial ecosystems, vegetation plays an irreplaceable role in regulating climate and maintaining ecological balance. However, vegetation dynamics often exhibit strong spatial heterogeneity and nonlinear responses, necessitating the development of an integrated modeling and analysis framework to reveal their underlying mechanisms and guide restoration efforts. This review systematically summarizes recent advances and key methodologies in vegetation dynamics research, focusing on four major dimensions: modeling mechanisms, nonlinear behaviors, ecosystem resilience assessment, and restoration pathway optimization. We first examine reaction–diffusion models based on representative ecological mechanisms such as scale-dependent feedbacks, motility-induced phase separation, and belowground interactions, and introduce stochastic and data-driven models to better capture the uncertainty and multi-source complexity inherent in natural systems. The review also explores nonlinear phenomena such as multistability, regime shifts, and localized structures, employing bifurcation analysis and amplitude equations to investigate pattern selection and system stability. We further review a range of early warning signal indicators based on critical slowing down, spatial patterns, and entropy, and introduce machine learning approaches to enhance predictive capability. Furthermore, we comprehensively review various optimal intervention methods including terminal control, boundary control, and sparse control. Finally, we discuss current challenges and future opportunities in theoretical integration, practical implementation, and cross-scale coordination. This review aims to provide systematic theoretical support and practical guidance for ecological modeling, restoration engineering, and global environmental governance.
植被作为陆地生态系统的核心组成部分,在调节气候、维持生态平衡方面具有不可替代的作用。然而,植被动态往往表现出强烈的空间异质性和非线性响应,需要建立一个综合的建模和分析框架,以揭示其潜在机制,指导恢复工作。本文从植被动力学建模机制、非线性行为、生态系统恢复力评估和恢复路径优化四个方面,系统地总结了植被动力学研究的最新进展和关键方法。我们首先研究了基于代表性生态机制的反应-扩散模型,如尺度依赖反馈、运动诱导的相分离和地下相互作用,并引入随机和数据驱动模型,以更好地捕捉自然系统固有的不确定性和多源复杂性。本文还探讨了非线性现象,如多稳定性、状态转移和局部结构,采用分岔分析和振幅方程来研究模式选择和系统稳定性。我们进一步回顾了一系列基于临界减速、空间模式和熵的预警信号指标,并引入了机器学习方法来增强预测能力。在此基础上,对终端控制、边界控制和稀疏控制等最优干预方法进行了综述。最后,我们在理论整合、实践实施和跨规模协调方面讨论了当前面临的挑战和未来的机遇。本文旨在为生态建模、修复工程和全球环境治理提供系统的理论支持和实践指导。
{"title":"Vegetation dynamics: Modeling, mechanisms, and emergent properties","authors":"Li-Feng Hou ,&nbsp;Li Li ,&nbsp;Renfei Chen ,&nbsp;Yong-Ping Wu ,&nbsp;Guo-Lin Feng ,&nbsp;Gui-Quan Sun","doi":"10.1016/j.physrep.2025.09.003","DOIUrl":"10.1016/j.physrep.2025.09.003","url":null,"abstract":"<div><div>As a core component of terrestrial ecosystems, vegetation plays an irreplaceable role in regulating climate and maintaining ecological balance. However, vegetation dynamics often exhibit strong spatial heterogeneity and nonlinear responses, necessitating the development of an integrated modeling and analysis framework to reveal their underlying mechanisms and guide restoration efforts. This review systematically summarizes recent advances and key methodologies in vegetation dynamics research, focusing on four major dimensions: modeling mechanisms, nonlinear behaviors, ecosystem resilience assessment, and restoration pathway optimization. We first examine reaction–diffusion models based on representative ecological mechanisms such as scale-dependent feedbacks, motility-induced phase separation, and belowground interactions, and introduce stochastic and data-driven models to better capture the uncertainty and multi-source complexity inherent in natural systems. The review also explores nonlinear phenomena such as multistability, regime shifts, and localized structures, employing bifurcation analysis and amplitude equations to investigate pattern selection and system stability. We further review a range of early warning signal indicators based on critical slowing down, spatial patterns, and entropy, and introduce machine learning approaches to enhance predictive capability. Furthermore, we comprehensively review various optimal intervention methods including terminal control, boundary control, and sparse control. Finally, we discuss current challenges and future opportunities in theoretical integration, practical implementation, and cross-scale coordination. This review aims to provide systematic theoretical support and practical guidance for ecological modeling, restoration engineering, and global environmental governance.</div></div>","PeriodicalId":404,"journal":{"name":"Physics Reports","volume":"1145 ","pages":"Pages 1-87"},"PeriodicalIF":29.5,"publicationDate":"2025-09-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145109673","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
High entropy superconductors 高熵超导体
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-09-22 DOI: 10.1016/j.physrep.2025.09.002
Yahua He , Kaiyu Ma , Jing You , Md. Shahriar A. Hossain , Muhammad Nadeem , Xiaolin Wang
High entropy materials have emerged as a focal point of scientific investigation in recent decades due to their exceptional properties, which offer substantial improvements in various domains, including alloy development, catalysis, and condensed matter physics. High entropy superconductors (HESs), in particular, have attracted significant interest due to their entropy-driven superior superconducting properties, making them promise for practical applications. Beyond the advancements seen in cuprates, nickelates, hydrides, iron-based superconductors, and twisted 2D material-based superconductors, HESs demonstrate robust superconductivity under extreme conditions such as high pressure and radiation. These distinctive attributes have established HESs as a unique class within the superconducting landscape, providing a novel platform for discovering new superconductors. This review marks the 10th anniversary of HESs, following their discovery in 2014, and provides a comprehensive overview of HESs, categorizing them into five key systems: high entropy alloys, layered BiS2 compounds, NaCl-type structures, REBCO cuprates (RE: rare earth elements), and other variants. It traces the development of HESs and systematically analyzes the impact of high entropy on superconductivity. The review highlights notable features of HESs, such as their exceptional mechanical properties, radiation resistance, and robust superconductivity under high pressure—features that have often been underappreciated. Furthermore, it advocates for expanding research on HESs, emphasizing the importance of developing functional HESs for practical applications.
近几十年来,高熵材料因其独特的性能而成为科学研究的焦点,在包括合金开发、催化和凝聚态物理在内的各个领域提供了实质性的改进。特别是高熵超导体(HESs),由于其熵驱动的优越超导特性而引起了极大的兴趣,使它们有望在实际应用中得到应用。除了在铜酸盐、镍酸盐、氢化物、铁基超导体和基于扭曲二维材料的超导体方面取得的进展外,HESs在高压和辐射等极端条件下也表现出强大的超导性。这些独特的属性使HESs成为超导领域中独特的一类,为发现新的超导体提供了一个新的平台。本文回顾了2014年发现的HESs十周年,并对HESs进行了全面概述,将其分为五个关键体系:高熵合金、层状BiS2化合物、nacl型结构、REBCO铜酸盐(RE:稀土元素)和其他变体。它追溯了HESs的发展,系统地分析了高熵对超导性的影响。这篇综述强调了HESs的显著特征,例如其卓越的机械性能、耐辐射性能和高压下的强大超导性——这些特征通常被低估了。此外,它主张扩大HESs的研究,强调开发实际应用的功能性HESs的重要性。
{"title":"High entropy superconductors","authors":"Yahua He ,&nbsp;Kaiyu Ma ,&nbsp;Jing You ,&nbsp;Md. Shahriar A. Hossain ,&nbsp;Muhammad Nadeem ,&nbsp;Xiaolin Wang","doi":"10.1016/j.physrep.2025.09.002","DOIUrl":"10.1016/j.physrep.2025.09.002","url":null,"abstract":"<div><div>High entropy materials have emerged as a focal point of scientific investigation in recent decades due to their exceptional properties, which offer substantial improvements in various domains, including alloy development, catalysis, and condensed matter physics. High entropy superconductors (HESs), in particular, have attracted significant interest due to their entropy-driven superior superconducting properties, making them promise for practical applications. Beyond the advancements seen in cuprates, nickelates, hydrides, iron-based superconductors, and twisted 2D material-based superconductors, HESs demonstrate robust superconductivity under extreme conditions such as high pressure and radiation. These distinctive attributes have established HESs as a unique class within the superconducting landscape, providing a novel platform for discovering new superconductors. This review marks the 10th anniversary of HESs, following their discovery in 2014, and provides a comprehensive overview of HESs, categorizing them into five key systems: high entropy alloys, layered BiS<sub>2</sub> compounds, NaCl-type structures, <em>RE</em>BCO cuprates (<em>RE:</em> rare earth elements), and other variants. It traces the development of HESs and systematically analyzes the impact of high entropy on superconductivity. The review highlights notable features of HESs, such as their exceptional mechanical properties, radiation resistance, and robust superconductivity under high pressure—features that have often been underappreciated. Furthermore, it advocates for expanding research on HESs, emphasizing the importance of developing functional HESs for practical applications.</div></div>","PeriodicalId":404,"journal":{"name":"Physics Reports","volume":"1144 ","pages":"Pages 1-44"},"PeriodicalIF":29.5,"publicationDate":"2025-09-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145108469","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
The anomalous magnetic moment of the muon in the Standard Model: an update 标准模型中介子的异常磁矩:更新
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-09-10 DOI: 10.1016/j.physrep.2025.08.002
R. Aliberti , T. Aoyama , E. Balzani , A. Bashir , G. Benton , J. Bijnens , V. Biloshytskyi , T. Blum , D. Boito , M. Bruno , E. Budassi , S. Burri , L. Cappiello , C.M. Carloni Calame , M. Cè , V. Cirigliano , D.A. Clarke , G. Colangelo , L. Cotrozzi , M. Cottini , A.S. Zhevlakov
We present the current Standard Model (SM) prediction for the muon anomalous magnetic moment, aμ, updating the first White Paper (WP20) [1]. The pure QED and electroweak contributions have been further consolidated, while hadronic contributions continue to be responsible for the bulk of the uncertainty of the SM prediction. Significant progress has been achieved in the hadronic light-by-light scattering contribution using both the data-driven dispersive approach as well as lattice-QCD calculations, leading to a reduction of the uncertainty by almost a factor of two. The most important development since WP20 is the change in the estimate of the leading-order hadronic-vacuum-polarization (LO HVP) contribution. A new measurement of the e+eπ+π cross section by CMD-3 has increased the tensions among data-driven dispersive evaluations of the LO HVP contribution to a level that makes it impossible to combine the results in a meaningful way. At the same time, the attainable precision of lattice-QCD calculations has increased substantially and allows for a consolidated lattice-QCD average of the LO HVP contribution with a precision of about 0.9%. Adopting the latter in this update has resulted in a major upward shift of the total SM prediction, which now reads aμSM=116592033(62)×1011 (530 ppb). When compared against the current experimental average based on the E821 experiment and runs 1–6 of E989 at Fermilab, one finds aμexpaμSM=38(63)×1011, which implies that there is no tension between the SM and experiment at the current level of precision. The final precision of E989 (127 ppb) is the target of future efforts by the Theory Initiative. The resolution of the tensions among data-driven dispersive evaluations of the LO HVP contribution will be a key element in this endeavor.
我们提出了μ子异常磁矩的标准模型(SM)预测,更新了第一份白皮书(WP20)[1]。纯QED和电弱贡献得到了进一步的巩固,而强子贡献仍然是SM预测的大部分不确定性的原因。使用数据驱动色散方法和晶格- qcd计算在强子光-光散射贡献方面取得了重大进展,导致不确定性减少了近两倍。自WP20以来最重要的发展是对主阶强子-真空极化(LO HVP)贡献的估计发生了变化。CMD-3对e+e−→π+π−截面的新测量增加了LO HVP贡献的数据驱动色散评估之间的紧张关系,使其无法以有意义的方式结合结果。同时,栅格- qcd计算的可实现精度大大提高,并允许LO HVP贡献的统一栅格- qcd平均精度约为0.9%。在此更新中采用后者导致总SM预测的主要向上移动,现在读取为aμSM=116592033(62)×10−11 (530 ppb)。与目前基于E821实验和Fermilab E989 1-6次运行的实验平均值相比,我们发现aμexp−aμSM=38(63)×10−11,这意味着在目前的精度水平上,SM与实验之间不存在张力。E989 (127 ppb)的最终精度是理论倡议未来努力的目标。解决由数据驱动的对联合国人道主义事务办事处贡献的分散评价之间的紧张关系将是这项努力的一个关键因素。
{"title":"The anomalous magnetic moment of the muon in the Standard Model: an update","authors":"R. Aliberti ,&nbsp;T. Aoyama ,&nbsp;E. Balzani ,&nbsp;A. Bashir ,&nbsp;G. Benton ,&nbsp;J. Bijnens ,&nbsp;V. Biloshytskyi ,&nbsp;T. Blum ,&nbsp;D. Boito ,&nbsp;M. Bruno ,&nbsp;E. Budassi ,&nbsp;S. Burri ,&nbsp;L. Cappiello ,&nbsp;C.M. Carloni Calame ,&nbsp;M. Cè ,&nbsp;V. Cirigliano ,&nbsp;D.A. Clarke ,&nbsp;G. Colangelo ,&nbsp;L. Cotrozzi ,&nbsp;M. Cottini ,&nbsp;A.S. Zhevlakov","doi":"10.1016/j.physrep.2025.08.002","DOIUrl":"10.1016/j.physrep.2025.08.002","url":null,"abstract":"<div><div>We present the current Standard Model (SM) prediction for the muon anomalous magnetic moment, <span><math><msub><mrow><mi>a</mi></mrow><mrow><mi>μ</mi></mrow></msub></math></span>, updating the first White Paper (WP20) <span><span>[1]</span></span>. The pure QED and electroweak contributions have been further consolidated, while hadronic contributions continue to be responsible for the bulk of the uncertainty of the SM prediction. Significant progress has been achieved in the hadronic light-by-light scattering contribution using both the data-driven dispersive approach as well as lattice-QCD calculations, leading to a reduction of the uncertainty by almost a factor of two. The most important development since WP20 is the change in the estimate of the leading-order hadronic-vacuum-polarization (LO HVP) contribution. A new measurement of the <span><math><mrow><msup><mrow><mi>e</mi></mrow><mrow><mo>+</mo></mrow></msup><msup><mrow><mi>e</mi></mrow><mrow><mo>−</mo></mrow></msup><mo>→</mo><msup><mrow><mi>π</mi></mrow><mrow><mo>+</mo></mrow></msup><msup><mrow><mi>π</mi></mrow><mrow><mo>−</mo></mrow></msup></mrow></math></span> cross section by CMD-3 has increased the tensions among data-driven dispersive evaluations of the LO HVP contribution to a level that makes it impossible to combine the results in a meaningful way. At the same time, the attainable precision of lattice-QCD calculations has increased substantially and allows for a consolidated lattice-QCD average of the LO HVP contribution with a precision of about 0.9%. Adopting the latter in this update has resulted in a major upward shift of the total SM prediction, which now reads <span><math><mrow><msubsup><mrow><mi>a</mi></mrow><mrow><mi>μ</mi></mrow><mrow><mtext>SM</mtext></mrow></msubsup><mo>=</mo><mn>116</mn><mspace></mspace><mn>592</mn><mspace></mspace><mn>033</mn><mrow><mo>(</mo><mn>62</mn><mo>)</mo></mrow><mo>×</mo><mn>1</mn><msup><mrow><mn>0</mn></mrow><mrow><mo>−</mo><mn>11</mn></mrow></msup></mrow></math></span> (530<!--> <!-->ppb). When compared against the current experimental average based on the E821 experiment and runs 1–6 of E989 at Fermilab, one finds <span><math><mrow><msubsup><mrow><mi>a</mi></mrow><mrow><mi>μ</mi></mrow><mrow><mtext>exp</mtext></mrow></msubsup><mo>−</mo><msubsup><mrow><mi>a</mi></mrow><mrow><mi>μ</mi></mrow><mrow><mtext>SM</mtext></mrow></msubsup><mo>=</mo><mn>38</mn><mrow><mo>(</mo><mn>63</mn><mo>)</mo></mrow><mo>×</mo><mn>1</mn><msup><mrow><mn>0</mn></mrow><mrow><mo>−</mo><mn>11</mn></mrow></msup></mrow></math></span>, which implies that there is no tension between the SM and experiment at the current level of precision. The final precision of E989 (127 ppb) is the target of future efforts by the Theory Initiative. The resolution of the tensions among data-driven dispersive evaluations of the LO HVP contribution will be a key element in this endeavor.</div></div>","PeriodicalId":404,"journal":{"name":"Physics Reports","volume":"1143 ","pages":"Pages 1-158"},"PeriodicalIF":29.5,"publicationDate":"2025-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145027658","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
Corrigendum to “Six decades of the FitzHugh–Nagumo model: A guide through its spatio-temporal dynamics and influence across disciplines” [Phys. Rep. 1096 (2024) 1–39] “FitzHugh-Nagumo模型的六十年:通过其时空动态和跨学科影响的指南”的勘误表[物理]。众议员1096 (2024)1-39]
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-08-26 DOI: 10.1016/j.physrep.2025.08.001
Daniel Cebrián-Lacasa , Pedro Parra-Rivas , Daniel Ruiz-Reynés , Lendert Gelens
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引用次数: 0
The fluctuation–dissipation relations: Growth, diffusion, and beyond 波动-耗散关系:增长、扩散和超越
IF 29.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2025-08-02 DOI: 10.1016/j.physrep.2025.07.004
Márcio Sampaio Gomes-Filho , Luciano Calheiros Lapas , Ewa Gudowska-Nowak , Fernando Albuquerque Oliveira
In this review, we scrutinize historical and modern results on the linear response of dynamical systems to external perturbations with a particular emphasis on the celebrated relationship between fluctuations and dissipation expressed by the fluctuation–dissipation theorem (FDT). The conceptual foundation of FDT originates from the definition of the equilibrium state and Onsager’s regression hypothesis. Over time, the fluctuation–dissipation relation has been vividly investigated also in systems far from equilibrium, which often exhibit wild fluctuations in measured parameters. In this review, we recall the major formulations of the FDT, including those proposed by Langevin, Onsager and Kubo. We discuss the role of fluctuations in a broad class of growth and diffusion phenomena and examine the violation of the FDT resulting from a transition from Euclidean to fractal geometry. Finally, we highlight possible generalizations of the FDT formalism and discuss situations where the relation breaks down and is no longer applicable.
在这篇综述中,我们仔细研究了动力系统对外部扰动的线性响应的历史和现代结果,特别强调了由波动-耗散定理(FDT)表达的著名的波动和耗散之间的关系。FDT的概念基础源于均衡状态的定义和Onsager的回归假设。随着时间的推移,涨落-耗散关系也在远离平衡的系统中得到了生动的研究,这些系统通常在测量参数中表现出剧烈的波动。在本文中,我们回顾了FDT的主要公式,包括Langevin, Onsager和Kubo提出的公式。我们讨论了波动在一类广泛的生长和扩散现象中的作用,并检查了从欧几里得几何到分形几何的过渡对FDT的破坏。最后,我们强调了FDT形式主义的可能概括,并讨论了关系破裂和不再适用的情况。
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引用次数: 0
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Physics Reports
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