首页 > 最新文献

Progress in Particle and Nuclear Physics最新文献

英文 中文
Heavy quarks and jets as probes of the QGP 作为QGP探测器的重夸克和喷流
IF 9.6 2区 物理与天体物理 Q1 PHYSICS, NUCLEAR Pub Date : 2022-11-01 DOI: 10.1016/j.ppnp.2022.103990
Liliana Apolinário , Yen-Jie Lee , Michael Winn

Quark–Gluon Plasma (QGP), a QCD state of matter created in ultra-relativistic heavy-ion collisions, has remarkable properties including, for example, a low shear viscosity over entropy ratio. By detecting the collection of low-momentum particles that arise from the collision, it is possible to gain quantitative insight into the created matter. However, its fast evolution and thermalization properties remain elusive. Only the usage of high momentum objects as probes of QGP can unveil its constituents at different wavelengths. In this review, we attempt to provide a comprehensive picture of what was, so far, possible to infer about QGP given our current theoretical understanding of jets, heavy-flavor, and quarkonia. We will bridge the resulting qualitative picture to the experimental observations done at both the LHC and RHIC. We will focus on the phenomenological description of experimental observations, provide a brief analytical summary of the description of hard probes, and an outlook towards the main difficulties we will need to surpass in the following years. To benchmark QGP-related effects, we will also address nuclear modifications to the initial state and hadronization effects.

夸克-胶子等离子体(QGP)是一种在超相对论重离子碰撞中产生的物质的QCD状态,它具有显著的特性,例如,低剪切粘度比熵比。通过检测碰撞产生的低动量粒子的集合,有可能获得对被创造物质的定量洞察。然而,它的快速演变和热化性能仍然难以捉摸。只有使用高动量物体作为QGP的探测器才能揭示其不同波长的成分。在这篇综述中,我们试图提供一个全面的图景,到目前为止,根据我们目前对喷流、重味和夸克的理论理解,可能推断出QGP。我们将把所得到的定性图像与在大型强子对撞机和强子对撞机上进行的实验观测联系起来。我们将把重点放在实验观察的现象学描述上,对硬探针的描述进行简要的分析总结,并展望我们在接下来的几年里需要克服的主要困难。为了对qgp相关效应进行基准测试,我们还将讨论初始态核修饰和强子化效应。
{"title":"Heavy quarks and jets as probes of the QGP","authors":"Liliana Apolinário ,&nbsp;Yen-Jie Lee ,&nbsp;Michael Winn","doi":"10.1016/j.ppnp.2022.103990","DOIUrl":"https://doi.org/10.1016/j.ppnp.2022.103990","url":null,"abstract":"<div><p><span><span>Quark–Gluon Plasma (QGP), a QCD </span>state of matter created in ultra-relativistic heavy-ion collisions, has remarkable properties including, for example, a low shear viscosity over entropy ratio. By detecting the collection of low-momentum particles that arise from the collision, it is possible to gain quantitative insight into the created matter. However, its fast evolution and thermalization properties remain elusive. Only the usage of high momentum objects as probes of QGP can unveil its constituents at different wavelengths. In this review, we attempt to provide a comprehensive picture of what was, so far, possible to infer about QGP given our current theoretical understanding of jets, heavy-flavor, and quarkonia. We will bridge the resulting qualitative picture to the experimental observations done at both the LHC and </span>RHIC. We will focus on the phenomenological description of experimental observations, provide a brief analytical summary of the description of hard probes, and an outlook towards the main difficulties we will need to surpass in the following years. To benchmark QGP-related effects, we will also address nuclear modifications to the initial state and hadronization effects.</p></div>","PeriodicalId":412,"journal":{"name":"Progress in Particle and Nuclear Physics","volume":"127 ","pages":"Article 103990"},"PeriodicalIF":9.6,"publicationDate":"2022-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"3270351","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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: 28
Finite-density lattice QCD and sign problem: Current status and open problems 有限密度晶格QCD与符号问题:现状与开放问题
IF 9.6 2区 物理与天体物理 Q1 PHYSICS, NUCLEAR Pub Date : 2022-11-01 DOI: 10.1016/j.ppnp.2022.103991
Keitaro Nagata

Finite-density lattice QCD aims for the first-principle study of QCD at finite density, which describes the system consisting of many quarks. The main targets are systems such as quark–gluon plasma, nuclei, and neutron stars. Explaining macroscopic physics from the microscopic theory is a natural path in the development of physics. To understand the strong interaction completely, we have to solve finite-density QCD. Each of the systems mentioned above has open problems which cannot easily be accessed by experiment or observation, so it is important to make progress in finite-density lattice QCD.

In this article, we summarize the past development and current status of the field of finite-density lattice QCD. The difficulty in the study of theories with the sign problem is that the numerical methods which are correct in principle do not necessarily work in practice and it is hard to know when it fails. We will introduce various approaches in this article, but all of them have pitfalls, which lead to unphysical results unless we study carefully. We will explain what kinds of studies were done in the past, to what extent they succeeded, and what kinds of obstacles they encountered, and why the approaches are correct in principle can lead to wrong answers. In this way, we would like to provide lessons from the past for ambitious researchers who plan to work on the finite-density lattice QCD.

有限密度晶格QCD旨在研究有限密度下的QCD的第一性原理,它描述了由许多夸克组成的系统。主要目标是夸克-胶子等离子体、原子核和中子星等系统。从微观理论解释宏观物理是物理学发展的自然路径。为了完全理解强相互作用,我们必须求解有限密度QCD。上述每一个系统都存在着难以通过实验或观测得到的开放性问题,因此在有限密度晶格QCD方面取得进展是非常重要的。本文综述了有限密度点阵量子光控领域的发展历程和现状。符号问题理论研究的难点在于,原理上正确的数值方法不一定适用于实际,而且很难知道什么时候是错误的。我们将在本文中介绍各种方法,但它们都有缺陷,除非我们仔细研究,否则会导致非物理结果。我们将解释过去做了什么样的研究,他们在多大程度上成功了,他们遇到了什么样的障碍,以及为什么这些方法在原则上是正确的,可能会导致错误的答案。通过这种方式,我们希望为计划研究有限密度晶格QCD的雄心勃勃的研究人员提供过去的经验教训。
{"title":"Finite-density lattice QCD and sign problem: Current status and open problems","authors":"Keitaro Nagata","doi":"10.1016/j.ppnp.2022.103991","DOIUrl":"https://doi.org/10.1016/j.ppnp.2022.103991","url":null,"abstract":"<div><p>Finite-density lattice QCD<span> aims for the first-principle study of QCD at finite density, which describes the system consisting of many quarks. The main targets are systems such as quark–gluon plasma, nuclei, and neutron stars<span>. Explaining macroscopic physics from the microscopic theory is a natural path in the development of physics. To understand the strong interaction completely, we have to solve finite-density QCD. Each of the systems mentioned above has open problems which cannot easily be accessed by experiment or observation, so it is important to make progress in finite-density lattice QCD.</span></span></p><p>In this article, we summarize the past development and current status of the field of finite-density lattice QCD. The difficulty in the study of theories with the sign problem is that the numerical methods which are correct in principle do not necessarily work in practice and it is hard to know when it fails. We will introduce various approaches in this article, but all of them have pitfalls, which lead to unphysical results unless we study carefully. We will explain what kinds of studies were done in the past, to what extent they succeeded, and what kinds of obstacles they encountered, and why the approaches are correct in principle can lead to wrong answers. In this way, we would like to provide lessons from the past for ambitious researchers who plan to work on the finite-density lattice QCD.</p></div>","PeriodicalId":412,"journal":{"name":"Progress in Particle and Nuclear Physics","volume":"127 ","pages":"Article 103991"},"PeriodicalIF":9.6,"publicationDate":"2022-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"2703856","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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: 31
Promises and challenges of high-energy vortex states collisions 高能涡旋态碰撞的前景与挑战
IF 9.6 2区 物理与天体物理 Q1 PHYSICS, NUCLEAR Pub Date : 2022-11-01 DOI: 10.1016/j.ppnp.2022.103987
Igor P. Ivanov

Vortex states of photons, electrons, and other particles are non-plane-wave solutions of the corresponding wave equation with helicoidal wave fronts. These states possess an intrinsic orbital angular momentum with respect to the average propagation direction, which represents a new degree of freedom, previously unexplored in particle or nuclear collisions. Vortex states of photons, electrons, neutrons, and neutral atoms have been experimentally produced, albeit at low energies, and are being intensively explored. Anticipating future experimental progress, one can ask what additional insights on nuclei and particles one can gain once collisions of high-energy vortex states become possible. This review describes the present-day landscape of physics opportunities, experimental progress and suggestions relevant to vortex states in high energy collisions. The aim is to familiarize the community with this emergent cross-disciplinary topic and to provide a sufficiently complete literature coverage, highlighting some results and calculational techniques.

光子、电子和其他粒子的涡旋态是具有螺旋波前的相应波动方程的非平面波解。这些态具有相对于平均传播方向的固有轨道角动量,这代表了一种新的自由度,以前未在粒子或核碰撞中探索过。光子、电子、中子和中性原子的漩涡态已经在实验中产生,尽管能量很低,并且正在被深入探索。展望未来的实验进展,人们可以问,一旦高能涡旋态的碰撞成为可能,人们可以获得什么关于原子核和粒子的额外见解。本文综述了高能碰撞中涡旋态的物理学机遇、实验进展和相关建议。目的是使社区熟悉这个新兴的跨学科主题,并提供足够完整的文献覆盖,突出一些结果和计算技术。
{"title":"Promises and challenges of high-energy vortex states collisions","authors":"Igor P. Ivanov","doi":"10.1016/j.ppnp.2022.103987","DOIUrl":"https://doi.org/10.1016/j.ppnp.2022.103987","url":null,"abstract":"<div><p><span>Vortex states of photons, electrons, and other particles are non-plane-wave solutions of the corresponding wave equation with helicoidal </span>wave fronts<span>. These states possess an intrinsic orbital angular momentum<span> with respect to the average propagation direction, which represents a new degree of freedom, previously unexplored in particle or nuclear collisions. Vortex states of photons, electrons, neutrons, and neutral atoms have been experimentally produced, albeit at low energies, and are being intensively explored. Anticipating future experimental progress, one can ask what additional insights on nuclei and particles one can gain once collisions of high-energy vortex states become possible. This review describes the present-day landscape of physics opportunities, experimental progress and suggestions relevant to vortex states in high energy collisions. The aim is to familiarize the community with this emergent cross-disciplinary topic and to provide a sufficiently complete literature coverage, highlighting some results and calculational techniques.</span></span></p></div>","PeriodicalId":412,"journal":{"name":"Progress in Particle and Nuclear Physics","volume":"127 ","pages":"Article 103987"},"PeriodicalIF":9.6,"publicationDate":"2022-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"2703854","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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: 23
Foundations and applications of quantum kinetic theory 量子动力学理论的基础和应用
IF 9.6 2区 物理与天体物理 Q1 PHYSICS, NUCLEAR Pub Date : 2022-11-01 DOI: 10.1016/j.ppnp.2022.103989
Yoshimasa Hidaka , Shi Pu , Qun Wang , Di-Lun Yang

Many novel quantum phenomena emerge in non-equilibrium relativistic quantum matter under extreme conditions such as strong magnetic fields and rotations. The quantum kinetic theory based on Wigner functions in quantum field theory provides a powerful and effective microscopic description of these quantum phenomena. In this article we review some of recent advances in the quantum kinetic theory and its applications in describing these quantum phenomena.

在强磁场和旋转等极端条件下,非平衡态相对论量子物质中出现了许多新的量子现象。以量子场论中的维格纳函数为基础的量子动力学理论为这些量子现象提供了有力而有效的微观描述。本文综述了近年来量子动力学理论及其在描述这些量子现象中的应用的一些进展。
{"title":"Foundations and applications of quantum kinetic theory","authors":"Yoshimasa Hidaka ,&nbsp;Shi Pu ,&nbsp;Qun Wang ,&nbsp;Di-Lun Yang","doi":"10.1016/j.ppnp.2022.103989","DOIUrl":"https://doi.org/10.1016/j.ppnp.2022.103989","url":null,"abstract":"<div><p><span>Many novel quantum phenomena emerge in non-equilibrium relativistic quantum matter under extreme conditions such as strong magnetic fields and rotations. The quantum </span>kinetic theory<span> based on Wigner functions in quantum field theory provides a powerful and effective microscopic description of these quantum phenomena. In this article we review some of recent advances in the quantum kinetic theory and its applications in describing these quantum phenomena.</span></p></div>","PeriodicalId":412,"journal":{"name":"Progress in Particle and Nuclear Physics","volume":"127 ","pages":"Article 103989"},"PeriodicalIF":9.6,"publicationDate":"2022-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"2703855","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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: 33
Physics with CEBAF at 12 GeV and future opportunities 物理学与CEBAF在12 GeV和未来的机会
IF 9.6 2区 物理与天体物理 Q1 PHYSICS, NUCLEAR Pub Date : 2022-11-01 DOI: 10.1016/j.ppnp.2022.103985
J. Arrington , M. Battaglieri , A. Boehnlein , S.A. Bogacz , W.K. Brooks , E. Chudakov , I. Cloët , R. Ent , H. Gao , J. Grames , L. Harwood , X. Ji , C. Keppel , G. Krafft , R.D. McKeown , J. Napolitano , J.W. Qiu , P. Rossi , M. Schram , S. Stepanyan , X. Zheng

We summarize the ongoing scientific program of the 12 GeV Continuous Electron Beam Accelerator Facility (CEBAF) and give an outlook into future opportunities. The program addresses important topics in nuclear, hadronic, and electroweak physics, including nuclear femtography, meson and baryon spectroscopy, quarks and gluons in nuclei, precision tests of the standard model and dark sector searches. Potential upgrades of CEBAF and their impact on scientific reach are discussed, such as higher luminosity, the addition of polarized and unpolarized positron beams, and doubling the beam energy.

我们总结了12gev连续电子束加速器设施(CEBAF)正在进行的科学计划,并对未来的机会进行了展望。该计划涉及核、强子和电弱物理中的重要主题,包括核飞影学、介子和重子光谱学、原子核中的夸克和胶子、标准模型的精确测试和暗区搜索。讨论了CEBAF的潜在升级及其对科学研究范围的影响,如更高的亮度,增加极化和非极化正电子束,以及光束能量加倍。
{"title":"Physics with CEBAF at 12 GeV and future opportunities","authors":"J. Arrington ,&nbsp;M. Battaglieri ,&nbsp;A. Boehnlein ,&nbsp;S.A. Bogacz ,&nbsp;W.K. Brooks ,&nbsp;E. Chudakov ,&nbsp;I. Cloët ,&nbsp;R. Ent ,&nbsp;H. Gao ,&nbsp;J. Grames ,&nbsp;L. Harwood ,&nbsp;X. Ji ,&nbsp;C. Keppel ,&nbsp;G. Krafft ,&nbsp;R.D. McKeown ,&nbsp;J. Napolitano ,&nbsp;J.W. Qiu ,&nbsp;P. Rossi ,&nbsp;M. Schram ,&nbsp;S. Stepanyan ,&nbsp;X. Zheng","doi":"10.1016/j.ppnp.2022.103985","DOIUrl":"https://doi.org/10.1016/j.ppnp.2022.103985","url":null,"abstract":"<div><p><span>We summarize the ongoing scientific program of the 12 GeV Continuous Electron Beam<span> Accelerator Facility (CEBAF) and give an outlook into future opportunities. The program addresses important topics in nuclear, hadronic, and electroweak physics, including nuclear femtography, meson and </span></span>baryon<span><span> spectroscopy, quarks and gluons in nuclei, precision tests of the </span>standard model<span> and dark sector searches. Potential upgrades of CEBAF and their impact on scientific reach are discussed, such as higher luminosity, the addition of polarized and unpolarized positron beams, and doubling the beam energy.</span></span></p></div>","PeriodicalId":412,"journal":{"name":"Progress in Particle and Nuclear Physics","volume":"127 ","pages":"Article 103985"},"PeriodicalIF":9.6,"publicationDate":"2022-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"1635564","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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: 31
Novel approaches in hadron spectroscopy 强子光谱学的新方法
IF 9.6 2区 物理与天体物理 Q1 PHYSICS, NUCLEAR Pub Date : 2022-11-01 DOI: 10.1016/j.ppnp.2022.103981
Miguel Albaladejo , Łukasz Bibrzycki , Sebastian M. Dawid , César Fernández-Ramírez , Sergi Gonzàlez-Solís , Astrid N. Hiller Blin , Andrew W. Jackura , Vincent Mathieu , Mikhail Mikhasenko , Victor I. Mokeev , Emilie Passemar , Alessandro Pilloni , Arkaitz Rodas , Jorge A. Silva-Castro , Wyatt A. Smith , Adam P. Szczepaniak , Daniel Winney , (Joint Physics Analysis Center)

The last two decades have witnessed the discovery of a myriad of new and unexpected hadrons. The future holds more surprises for us, thanks to new-generation experiments. Understanding the signals and determining the properties of the states requires a parallel theoretical effort. To make full use of available and forthcoming data, a careful amplitude modeling is required, together with a sound treatment of the statistical uncertainties, and a systematic survey of the model dependencies. We review the contributions made by the Joint Physics Analysis Center to the field of hadron spectroscopy.

在过去的二十年里,无数新的、意想不到的强子被发现。由于新一代的实验,未来会给我们带来更多的惊喜。理解信号和确定状态的性质需要并行的理论努力。为了充分利用现有的和即将到来的数据,需要仔细的振幅建模,同时对统计不确定性进行合理的处理,并对模型依赖性进行系统的调查。综述了联合物理分析中心在强子光谱学领域所作的贡献。
{"title":"Novel approaches in hadron spectroscopy","authors":"Miguel Albaladejo ,&nbsp;Łukasz Bibrzycki ,&nbsp;Sebastian M. Dawid ,&nbsp;César Fernández-Ramírez ,&nbsp;Sergi Gonzàlez-Solís ,&nbsp;Astrid N. Hiller Blin ,&nbsp;Andrew W. Jackura ,&nbsp;Vincent Mathieu ,&nbsp;Mikhail Mikhasenko ,&nbsp;Victor I. Mokeev ,&nbsp;Emilie Passemar ,&nbsp;Alessandro Pilloni ,&nbsp;Arkaitz Rodas ,&nbsp;Jorge A. Silva-Castro ,&nbsp;Wyatt A. Smith ,&nbsp;Adam P. Szczepaniak ,&nbsp;Daniel Winney ,&nbsp;(Joint Physics Analysis Center)","doi":"10.1016/j.ppnp.2022.103981","DOIUrl":"https://doi.org/10.1016/j.ppnp.2022.103981","url":null,"abstract":"<div><p>The last two decades have witnessed the discovery of a myriad of new and unexpected hadrons<span>. The future holds more surprises for us, thanks to new-generation experiments. Understanding the signals and determining the properties of the states requires a parallel theoretical effort. To make full use of available and forthcoming data, a careful amplitude modeling is required, together with a sound treatment of the statistical uncertainties, and a systematic survey of the model dependencies. We review the contributions made by the Joint Physics Analysis Center to the field of hadron spectroscopy.</span></p></div>","PeriodicalId":412,"journal":{"name":"Progress in Particle and Nuclear Physics","volume":"127 ","pages":"Article 103981"},"PeriodicalIF":9.6,"publicationDate":"2022-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"3139627","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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: 26
Cosmic nucleosynthesis: A multi-messenger challenge 宇宙核合成:多信使挑战
IF 9.6 2区 物理与天体物理 Q1 PHYSICS, NUCLEAR Pub Date : 2022-11-01 DOI: 10.1016/j.ppnp.2022.103983
Roland Diehl , Andreas J. Korn , Bruno Leibundgut , Maria Lugaro , Anton Wallner
<div><p>The origins of the elements and isotopes of cosmic material is a critical aspect of understanding the evolution of the universe. Nucleosynthesis typically requires physical conditions of high temperatures and densities. These are found in the Big Bang, in the interiors of stars, and in explosions with their compressional shocks and high neutrino and neutron fluxes<span>. Many different tools are available to disentangle the composition of cosmic matter, in material of extraterrestrial origins such as cosmic rays, meteorites<span><span>, stardust grains, lunar and terrestrial sediments, and through astronomical observations across the electromagnetic spectrum. Understanding </span>cosmic abundances<span> and their evolution requires combining such measurements with approaches of astrophysical, nuclear theories and laboratory experiments, and exploiting additional cosmic messengers, such as neutrinos and gravitational waves. Recent years have seen significant progress in almost all these fields; they are presented in this review.</span></span></span></p><p><span><span>The Sun and the solar system are our reference system for abundances of elements and isotopes. Many direct and indirect methods are employed to establish a refined abundance record from the time when the Sun and the Earth were formed. Indications for nucleosynthesis in the local environment when the Sun was formed are derived from meteoritic material and inclusion of radioactive atoms in deep-sea sediments. Spectroscopy at many wavelengths and the neutrino flux from the hydrogen fusion processes in the Sun have established a refined model of how the </span>nuclear energy production<span> shapes stars. Models are required to explore nuclear fusion of heavier elements. These stellar evolution<span><span> calculations have been confirmed by observations of nucleosynthesis products in the ejecta of stars and </span>supernovae, as captured by stardust grains and by characteristic lines in spectra seen from these objects. One of the successes has been to directly observe </span></span></span><span><math><mi>γ</mi></math></span><span> rays from radioactive material synthesised in stellar explosions, which fully support the astrophysical models. Another has been the observation of radioactive afterglow and characteristic heavy-element spectrum from a neutron-star merger, confirming the neutron rich environments encountered in such rare explosions. The ejecta material captured by Earth over millions of years in sediments and identified through characteristic radio-isotopes suggests that nearby nucleosynthesis occurred in recent history, with further indications for sites of specific nucleosynthesis. Together with stardust and diffuse </span><span><math><mi>γ</mi></math></span> rays from radioactive ejecta, these help to piece together how cosmic materials are transported in interstellar space and re-cycled into and between generations of stars. Our description of cosmic compositional e
宇宙物质的元素和同位素的起源是理解宇宙演化的一个关键方面。核合成通常需要高温和高密度的物理条件。它们存在于宇宙大爆炸,恒星内部,以及具有压缩激波和高中微子和中子通量的爆炸中。有许多不同的工具可以用来解开宇宙物质的组成,包括宇宙射线、陨石、星尘颗粒、月球和陆地沉积物等地外物质,以及通过电磁频谱的天文观测。了解宇宙丰度及其演化需要将这些测量方法与天体物理学、核理论和实验室实验相结合,并利用其他宇宙信使,如中微子和引力波。近年来,几乎所有这些领域都取得了重大进展;这篇综述介绍了它们。太阳和太阳系是我们元素和同位素丰度的参考系统。许多直接和间接的方法被用来建立一个精确的丰度记录,从太阳和地球形成的时候开始。太阳形成时当地环境中核合成的迹象来自陨石物质和深海沉积物中放射性原子的包裹体。许多波长的光谱学和太阳中氢聚变过程产生的中微子通量建立了一个精细的模型,说明核能的产生是如何塑造恒星的。探索重元素的核聚变需要模型。这些恒星演化的计算已经通过观察恒星和超新星喷出物中的核合成产物得到了证实,这些产物被星尘颗粒捕获,并通过从这些物体中看到的光谱特征线得到了证实。其中一项成功是直接观察到恒星爆炸中合成的放射性物质产生的γ射线,这完全支持了天体物理模型。另一个是对中子星合并的放射性余辉和特征重元素光谱的观察,证实了在这种罕见的爆炸中遇到的富含中子的环境。地球在沉积物中捕获了数百万年的喷出物,并通过特征放射性同位素进行了鉴定,这表明在最近的历史中发生了附近的核合成,并进一步指出了特定核合成的地点。再加上星尘和来自放射性喷射物的弥漫性γ射线,这些有助于拼凑出宇宙物质是如何在星际空间中运输的,以及如何在几代恒星之间再循环的。我们对宇宙成分演化的描述需要这样的观测支持,因为它建立在几个假设之上,而这些假设似乎受到了最近对星系演化过程中常见的剧烈事件的认识的挑战。这篇综述介绍了宇宙物质的流动和核合成的各个地点,这是通过结合许多技术和观察来理解的,朝着目前关于宇宙如何被元素丰富的知识发展。
{"title":"Cosmic nucleosynthesis: A multi-messenger challenge","authors":"Roland Diehl ,&nbsp;Andreas J. Korn ,&nbsp;Bruno Leibundgut ,&nbsp;Maria Lugaro ,&nbsp;Anton Wallner","doi":"10.1016/j.ppnp.2022.103983","DOIUrl":"https://doi.org/10.1016/j.ppnp.2022.103983","url":null,"abstract":"&lt;div&gt;&lt;p&gt;The origins of the elements and isotopes of cosmic material is a critical aspect of understanding the evolution of the universe. Nucleosynthesis typically requires physical conditions of high temperatures and densities. These are found in the Big Bang, in the interiors of stars, and in explosions with their compressional shocks and high neutrino and neutron fluxes&lt;span&gt;. Many different tools are available to disentangle the composition of cosmic matter, in material of extraterrestrial origins such as cosmic rays, meteorites&lt;span&gt;&lt;span&gt;, stardust grains, lunar and terrestrial sediments, and through astronomical observations across the electromagnetic spectrum. Understanding &lt;/span&gt;cosmic abundances&lt;span&gt; and their evolution requires combining such measurements with approaches of astrophysical, nuclear theories and laboratory experiments, and exploiting additional cosmic messengers, such as neutrinos and gravitational waves. Recent years have seen significant progress in almost all these fields; they are presented in this review.&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;&lt;p&gt;&lt;span&gt;&lt;span&gt;The Sun and the solar system are our reference system for abundances of elements and isotopes. Many direct and indirect methods are employed to establish a refined abundance record from the time when the Sun and the Earth were formed. Indications for nucleosynthesis in the local environment when the Sun was formed are derived from meteoritic material and inclusion of radioactive atoms in deep-sea sediments. Spectroscopy at many wavelengths and the neutrino flux from the hydrogen fusion processes in the Sun have established a refined model of how the &lt;/span&gt;nuclear energy production&lt;span&gt; shapes stars. Models are required to explore nuclear fusion of heavier elements. These stellar evolution&lt;span&gt;&lt;span&gt; calculations have been confirmed by observations of nucleosynthesis products in the ejecta of stars and &lt;/span&gt;supernovae, as captured by stardust grains and by characteristic lines in spectra seen from these objects. One of the successes has been to directly observe &lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;span&gt;&lt;math&gt;&lt;mi&gt;γ&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt; rays from radioactive material synthesised in stellar explosions, which fully support the astrophysical models. Another has been the observation of radioactive afterglow and characteristic heavy-element spectrum from a neutron-star merger, confirming the neutron rich environments encountered in such rare explosions. The ejecta material captured by Earth over millions of years in sediments and identified through characteristic radio-isotopes suggests that nearby nucleosynthesis occurred in recent history, with further indications for sites of specific nucleosynthesis. Together with stardust and diffuse &lt;/span&gt;&lt;span&gt;&lt;math&gt;&lt;mi&gt;γ&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt; rays from radioactive ejecta, these help to piece together how cosmic materials are transported in interstellar space and re-cycled into and between generations of stars. Our description of cosmic compositional e","PeriodicalId":412,"journal":{"name":"Progress in Particle and Nuclear Physics","volume":"127 ","pages":"Article 103983"},"PeriodicalIF":9.6,"publicationDate":"2022-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"3139628","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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: 10
Holographic approach to compact stars and their binary mergers 致密恒星及其双星合并的全息方法
IF 9.6 2区 物理与天体物理 Q1 PHYSICS, NUCLEAR Pub Date : 2022-09-01 DOI: 10.1016/j.ppnp.2022.103972
Carlos Hoyos , Niko Jokela , Aleksi Vuorinen

In this review article, we describe the role of holography in deciphering the physics of dense QCD matter, relevant for the description of compact stars and their binary mergers. We review the strengths and limitations of the holographic duality in describing strongly interacting matter at large baryon density, walk the reader through the most important results derived using the holographic approach so far, and highlight a number of outstanding open problems in the field. Finally, we discuss how we foresee holography contributing to compact-star physics in the coming years.

在这篇综述文章中,我们描述了全息术在破译致密QCD物质物理学中的作用,这与描述致密恒星及其双星合并有关。我们回顾了全息二象性在描述大重子密度下强相互作用物质方面的优势和局限性,向读者介绍了迄今为止使用全息方法得出的最重要的结果,并强调了该领域的一些突出的开放问题。最后,我们讨论了我们如何预见全息在未来几年对致密恒星物理学的贡献。
{"title":"Holographic approach to compact stars and their binary mergers","authors":"Carlos Hoyos ,&nbsp;Niko Jokela ,&nbsp;Aleksi Vuorinen","doi":"10.1016/j.ppnp.2022.103972","DOIUrl":"https://doi.org/10.1016/j.ppnp.2022.103972","url":null,"abstract":"<div><p>In this review article, we describe the role of holography in deciphering the physics of dense QCD matter, relevant for the description of compact stars and their binary mergers. We review the strengths and limitations of the holographic duality in describing strongly interacting matter at large baryon density, walk the reader through the most important results derived using the holographic approach so far, and highlight a number of outstanding open problems in the field. Finally, we discuss how we foresee holography contributing to compact-star physics in the coming years.</p></div>","PeriodicalId":412,"journal":{"name":"Progress in Particle and Nuclear Physics","volume":"126 ","pages":"Article 103972"},"PeriodicalIF":9.6,"publicationDate":"2022-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"3270352","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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: 17
Nuclear weak rates and nuclear weak processes in stars 恒星中的核弱速率和核弱过程
IF 9.6 2区 物理与天体物理 Q1 PHYSICS, NUCLEAR Pub Date : 2022-09-01 DOI: 10.1016/j.ppnp.2022.103974
Toshio Suzuki
<div><p><span><span>Nuclear weak rates in stellar environments are obtained by taking into account recent advances in shell-model studies of spin-dependent excitation modes in nuclei including Gamow–Teller (GT) and spin-dipole transitions. They are applied to nuclear weak processes in stars such as cooling and heating of the cores of stars and nucleosynthesis in supernovae. The important roles of accurate weak rates for the study of </span>astrophysical processes are pointed out in the following cases. (1) The electron-capture (e-capture) and </span><span><math><mi>β</mi></math></span>-decay rates in <span><math><mrow><mi>s</mi><mi>d</mi></mrow></math></span>-shell are evaluated with the USDB Hamiltonian and used to study the evolution of O-Ne-Mg cores in stars with 8–10 M<span><math><msub><mrow></mrow><mrow><mo>⊙</mo></mrow></msub></math></span>. The important roles of the <span><math><mi>A</mi></math></span> <span><math><mo>=</mo></math></span><span> 23 and 25 pairs of nuclei for the cooling of the cores by nuclear Urca processes are investigated. (2) They are also used to study heating of the O-Ne-Mg core by double e-captures on </span><sup>20</sup>Ne in later stages of the evolution. Especially, the e-capture rates for a second-forbidden transition in <sup>20</sup><span>Ne are evaluated with the multipole expansion method by Walecka as well as the method of Behrens–B</span><span><math><mover><mrow><mtext>u</mtext></mrow><mrow><mo>̈</mo></mrow></mover></math></span>hring. Possible important roles of the transition in heating the O-Ne-Mg cores and implications on the final fate of the cores (core-collapse or thermonuclear explosion) are discussed. (3) The weak rates in <span><math><mrow><mi>p</mi><mi>f</mi></mrow></math></span><span><span>-shell nuclei are evaluated with a new Hamiltonian, GXPF1J, and applied to nucleosynthesis of iron-group elements in Type Ia supernova explosions. The over-production problem of neutron-rich </span>iron isotopes<span> compared with the solar abundances, which remained for the rates according to Fuller, Fowler and Newman, is much improved, and the over-production is now reduced to be within a factor of two. (4) The weak rates for nuclei with two-major shells are evaluated. For </span></span><span><math><mrow><mi>s</mi><mi>d</mi></mrow></math></span>-<span><math><mrow><mi>p</mi><mi>f</mi></mrow></math></span> shell in the island of inversion, the weak rates for the <span><math><mi>A</mi></math></span> <span><math><mo>=</mo></math></span> 31 pair of nuclei, which are important for nuclear Urca processes in neutron-star crusts, are evaluated with the effective interaction obtained by the extended Kuo–Krenciglowa (EKK) method. Neutron-rich nuclei with and near neutron number (<span><math><mi>N</mi></math></span>) of 50 are important for core-collapse processes in supernova explosions. The transition strengths and e-capture rates in <sup>78</sup>Ni are evaluated with a new shell-model Hamiltonian for the <span><math
恒星环境中的核弱速率是通过考虑原子核中自旋相关激发模式的壳模型研究的最新进展获得的,包括伽莫夫-泰勒(GT)和自旋偶极子跃迁。它们被应用于恒星的核弱过程,如恒星核心的冷却和加热以及超新星的核合成。在下列情况下,指出精确的弱率对研究天体物理过程的重要作用。(1)用USDB哈密顿量计算了sd壳层的电子俘获率和β衰变率,并用于研究8 ~ 10 M⊙恒星中O-Ne-Mg核的演化。研究了A = 23和25对原子核在原子核Urca过程冷却中所起的重要作用。(2)它们也被用来研究在演化后期对20Ne的双e俘获对O-Ne-Mg核的加热。特别地,用Walecka的多极展开法和behrens - b hring法计算了20Ne中第二禁跃迁的电子捕获率。讨论了这种转变在加热O-Ne-Mg核中可能起的重要作用,以及对核的最终命运(核塌缩或热核爆炸)的影响。(3)用新的哈密顿量GXPF1J评价了pf壳核的弱速率,并应用于Ia型超新星爆炸中铁族元素的核合成。富中子铁同位素的生产过剩问题与太阳丰度相比得到了很大的改善,根据富勒、福勒和纽曼的说法,太阳丰度的比率仍然存在,生产过剩的问题现在减少到两倍以内。(4)计算了双主壳核的弱速率。利用扩展的Kuo-Krenciglowa (EKK)方法得到的有效相互作用,对反演岛上的sd-pf壳的A = 31对核的弱速率进行了计算。中子数(N)为50或接近50的富中子核在超新星爆炸的核心坍缩过程中是重要的。利用pf-sdg壳层的新壳层模型哈密顿量计算了78Ni中的跃迁强度和电子捕获速率,并与随机相位近似(RPA)和有效速率公式得到的结果进行了比较。(5)用GT跃迁和第一禁跃迁的壳层模型计算了r过程核合成的等待点核N=126同工核的β衰变率和半衰期。指出了禁止跃迁对质子数(Z)较大的同色同位素的重要作用,发现其半衰期比通过Möller得到的有限范围液滴模型(FRDM)等标准模型得到的半衰期短。(6)用新的壳层模型哈密顿量得到了13C、16O和40Ar上的中微子核反应截面。讨论了对核合成、中微子探测、中微子振荡和中微子质量层次的影响。
{"title":"Nuclear weak rates and nuclear weak processes in stars","authors":"Toshio Suzuki","doi":"10.1016/j.ppnp.2022.103974","DOIUrl":"https://doi.org/10.1016/j.ppnp.2022.103974","url":null,"abstract":"&lt;div&gt;&lt;p&gt;&lt;span&gt;&lt;span&gt;Nuclear weak rates in stellar environments are obtained by taking into account recent advances in shell-model studies of spin-dependent excitation modes in nuclei including Gamow–Teller (GT) and spin-dipole transitions. They are applied to nuclear weak processes in stars such as cooling and heating of the cores of stars and nucleosynthesis in supernovae. The important roles of accurate weak rates for the study of &lt;/span&gt;astrophysical processes are pointed out in the following cases. (1) The electron-capture (e-capture) and &lt;/span&gt;&lt;span&gt;&lt;math&gt;&lt;mi&gt;β&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;-decay rates in &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;s&lt;/mi&gt;&lt;mi&gt;d&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;-shell are evaluated with the USDB Hamiltonian and used to study the evolution of O-Ne-Mg cores in stars with 8–10 M&lt;span&gt;&lt;math&gt;&lt;msub&gt;&lt;mrow&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mo&gt;⊙&lt;/mo&gt;&lt;/mrow&gt;&lt;/msub&gt;&lt;/math&gt;&lt;/span&gt;. The important roles of the &lt;span&gt;&lt;math&gt;&lt;mi&gt;A&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt; &lt;span&gt;&lt;math&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt; 23 and 25 pairs of nuclei for the cooling of the cores by nuclear Urca processes are investigated. (2) They are also used to study heating of the O-Ne-Mg core by double e-captures on &lt;/span&gt;&lt;sup&gt;20&lt;/sup&gt;Ne in later stages of the evolution. Especially, the e-capture rates for a second-forbidden transition in &lt;sup&gt;20&lt;/sup&gt;&lt;span&gt;Ne are evaluated with the multipole expansion method by Walecka as well as the method of Behrens–B&lt;/span&gt;&lt;span&gt;&lt;math&gt;&lt;mover&gt;&lt;mrow&gt;&lt;mtext&gt;u&lt;/mtext&gt;&lt;/mrow&gt;&lt;mrow&gt;&lt;mo&gt;̈&lt;/mo&gt;&lt;/mrow&gt;&lt;/mover&gt;&lt;/math&gt;&lt;/span&gt;hring. Possible important roles of the transition in heating the O-Ne-Mg cores and implications on the final fate of the cores (core-collapse or thermonuclear explosion) are discussed. (3) The weak rates in &lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;p&lt;/mi&gt;&lt;mi&gt;f&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;&lt;span&gt;&lt;span&gt;-shell nuclei are evaluated with a new Hamiltonian, GXPF1J, and applied to nucleosynthesis of iron-group elements in Type Ia supernova explosions. The over-production problem of neutron-rich &lt;/span&gt;iron isotopes&lt;span&gt; compared with the solar abundances, which remained for the rates according to Fuller, Fowler and Newman, is much improved, and the over-production is now reduced to be within a factor of two. (4) The weak rates for nuclei with two-major shells are evaluated. For &lt;/span&gt;&lt;/span&gt;&lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;s&lt;/mi&gt;&lt;mi&gt;d&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt;-&lt;span&gt;&lt;math&gt;&lt;mrow&gt;&lt;mi&gt;p&lt;/mi&gt;&lt;mi&gt;f&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;&lt;/span&gt; shell in the island of inversion, the weak rates for the &lt;span&gt;&lt;math&gt;&lt;mi&gt;A&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt; &lt;span&gt;&lt;math&gt;&lt;mo&gt;=&lt;/mo&gt;&lt;/math&gt;&lt;/span&gt; 31 pair of nuclei, which are important for nuclear Urca processes in neutron-star crusts, are evaluated with the effective interaction obtained by the extended Kuo–Krenciglowa (EKK) method. Neutron-rich nuclei with and near neutron number (&lt;span&gt;&lt;math&gt;&lt;mi&gt;N&lt;/mi&gt;&lt;/math&gt;&lt;/span&gt;) of 50 are important for core-collapse processes in supernova explosions. The transition strengths and e-capture rates in &lt;sup&gt;78&lt;/sup&gt;Ni are evaluated with a new shell-model Hamiltonian for the &lt;span&gt;&lt;math","PeriodicalId":412,"journal":{"name":"Progress in Particle and Nuclear Physics","volume":"126 ","pages":"Article 103974"},"PeriodicalIF":9.6,"publicationDate":"2022-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"3270353","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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: 5
Beyond-mean-field approaches for nuclear neutrinoless double beta decay in the standard mechanism 标准机制中核中微子双β衰变的超平均场方法
IF 9.6 2区 物理与天体物理 Q1 PHYSICS, NUCLEAR Pub Date : 2022-09-01 DOI: 10.1016/j.ppnp.2022.103965
J.M. Yao , J. Meng , Y.F. Niu , P. Ring

Nuclear weak decays provide important probes to fundamental symmetries in nature. A precise description of these processes in atomic nuclei requires comprehensive knowledge on both the strong and weak interactions in the nuclear medium and on the dynamics of quantum many-body systems. In particular, an observation of the hypothetical double beta decay without emission of neutrinos (0νββ) would unambiguously demonstrate the Majorana nature of neutrinos and the existence of the lepton-number-violation process. It would also provide unique information on the ordering and absolute scale of neutrino masses. The next-generation tonne-scale experiments with sensitivity up to 1028 years after a few years of running will probably provide a definite answer to these fundamental questions based on our current knowledge on the nuclear matrix element (NME), the precise determination of which is a challenge to nuclear theory. Beyond-mean-field approaches have been frequently adapted for the study of nuclear structure and decay throughout the nuclear chart for several decades. In this review, we summarize the status of beyond-mean-field calculations of the NMEs of 0νββ decay assuming the standard mechanism of an exchange of light Majorana neutrinos. The challenges and prospects in the extension and application of beyond-mean-field approaches for 0νββ decay are discussed.

核弱衰变为研究自然界的基本对称性提供了重要的途径。要精确地描述原子核中的这些过程,需要对核介质中的强相互作用和弱相互作用以及量子多体系统的动力学有全面的了解。特别是,对假设的双β衰变而不发射中微子(0νββ)的观测将明确地证明中微子的马约拉纳性质和轻子数违反过程的存在。它还将提供关于中微子质量的顺序和绝对尺度的独特信息。基于我们目前对核基质元素(NME)的知识,经过几年的运行,下一代具有高达1028年灵敏度的吨级实验可能会为这些基本问题提供明确的答案,精确确定核基质元素对核理论来说是一个挑战。几十年来,在整个核图中,超平均场方法经常用于核结构和衰变的研究。在这篇综述中,我们总结了假设光马约拉纳中微子交换的标准机制下0νββ衰变的NMEs的超平均场计算的现状。讨论了0νββ衰变的超平均场方法在推广和应用中的挑战和前景。
{"title":"Beyond-mean-field approaches for nuclear neutrinoless double beta decay in the standard mechanism","authors":"J.M. Yao ,&nbsp;J. Meng ,&nbsp;Y.F. Niu ,&nbsp;P. Ring","doi":"10.1016/j.ppnp.2022.103965","DOIUrl":"https://doi.org/10.1016/j.ppnp.2022.103965","url":null,"abstract":"<div><p><span>Nuclear weak decays provide important probes to fundamental symmetries in nature. A precise description of these processes in atomic nuclei requires comprehensive knowledge on both the strong and weak interactions in the nuclear medium and on the dynamics of quantum many-body systems. In particular, an observation of the hypothetical double beta decay without emission of neutrinos (</span><span><math><mrow><mn>0</mn><mi>ν</mi><mi>β</mi><mi>β</mi></mrow></math></span><span>) would unambiguously demonstrate the Majorana nature of neutrinos and the existence of the lepton-number-violation process. It would also provide unique information on the ordering and absolute scale of neutrino masses. The next-generation tonne-scale experiments with sensitivity up to </span><span><math><mrow><mn>1</mn><msup><mrow><mn>0</mn></mrow><mrow><mn>28</mn></mrow></msup></mrow></math></span><span> years after a few years of running will probably provide a definite answer to these fundamental questions based on our current knowledge on the nuclear matrix element (NME), the precise determination of which is a challenge to nuclear theory. Beyond-mean-field approaches have been frequently adapted for the study of nuclear structure and decay throughout the nuclear chart for several decades. In this review, we summarize the status of beyond-mean-field calculations of the NMEs of </span><span><math><mrow><mn>0</mn><mi>ν</mi><mi>β</mi><mi>β</mi></mrow></math></span> decay assuming the standard mechanism of an exchange of light Majorana neutrinos. The challenges and prospects in the extension and application of beyond-mean-field approaches for <span><math><mrow><mn>0</mn><mi>ν</mi><mi>β</mi><mi>β</mi></mrow></math></span> decay are discussed.</p></div>","PeriodicalId":412,"journal":{"name":"Progress in Particle and Nuclear Physics","volume":"126 ","pages":"Article 103965"},"PeriodicalIF":9.6,"publicationDate":"2022-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"3451557","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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: 20
期刊
Progress in Particle and Nuclear Physics
全部 Acc. Chem. Res. ACS Applied Bio Materials ACS Appl. Electron. Mater. ACS Appl. Energy Mater. ACS Appl. Mater. Interfaces ACS Appl. Nano Mater. ACS Appl. Polym. Mater. ACS BIOMATER-SCI ENG ACS Catal. ACS Cent. Sci. ACS Chem. Biol. ACS Chemical Health & Safety ACS Chem. Neurosci. ACS Comb. Sci. ACS Earth Space Chem. ACS Energy Lett. ACS Infect. Dis. ACS Macro Lett. ACS Mater. Lett. ACS Med. Chem. Lett. ACS Nano ACS Omega ACS Photonics ACS Sens. ACS Sustainable Chem. Eng. ACS Synth. Biol. Anal. Chem. BIOCHEMISTRY-US Bioconjugate Chem. BIOMACROMOLECULES Chem. Res. Toxicol. Chem. Rev. Chem. Mater. CRYST GROWTH DES ENERG FUEL Environ. Sci. Technol. Environ. Sci. Technol. Lett. Eur. J. Inorg. Chem. IND ENG CHEM RES Inorg. Chem. J. Agric. Food. Chem. J. Chem. Eng. Data J. Chem. Educ. J. Chem. Inf. Model. J. Chem. Theory Comput. J. Med. Chem. J. Nat. Prod. J PROTEOME RES J. Am. Chem. Soc. LANGMUIR MACROMOLECULES Mol. Pharmaceutics Nano Lett. Org. Lett. ORG PROCESS RES DEV ORGANOMETALLICS J. Org. Chem. J. Phys. Chem. J. Phys. Chem. A J. Phys. Chem. B J. Phys. Chem. C J. Phys. Chem. Lett. Analyst Anal. Methods Biomater. Sci. Catal. Sci. Technol. Chem. Commun. Chem. Soc. Rev. CHEM EDUC RES PRACT CRYSTENGCOMM Dalton Trans. Energy Environ. Sci. ENVIRON SCI-NANO ENVIRON SCI-PROC IMP ENVIRON SCI-WAT RES Faraday Discuss. Food Funct. Green Chem. Inorg. Chem. Front. Integr. Biol. J. Anal. At. Spectrom. J. Mater. Chem. A J. Mater. Chem. B J. Mater. Chem. C Lab Chip Mater. Chem. Front. Mater. Horiz. MEDCHEMCOMM Metallomics Mol. Biosyst. Mol. Syst. Des. Eng. Nanoscale Nanoscale Horiz. Nat. Prod. Rep. New J. Chem. Org. Biomol. Chem. Org. Chem. Front. PHOTOCH PHOTOBIO SCI PCCP Polym. Chem.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1