期刊目标和范围：《核与粒子科学年度评论》自 1952 年出版以来，涵盖了核与粒子科学领域的重大发展，包括最近的理论发展以及实验结果及其解释、核结构、重离子相互作用，在太阳和大气中微子中观察到的振荡，重夸克的物理学，粒子和核物理学对天体粒子物理学的影响，以及加速器设计和仪器的最新发展。

Since its inception in 1952, the Annual Review of Nuclear and Particle Science has focused on significant advancements in the field of nuclear and particle science. The journal covers recent theoretical developments, experimental results and their interpretations, nuclear structure, heavy ion interactions, neutrino oscillations observed in the sun and atmosphere, heavy quark physics, the impact of particle and nuclear physics on astroparticle physics, as well as the latest developments in accelerator design and instrumentation.

《Annual Review of Nuclear and Particle Science》自1952年出版以来，致力于核与粒子科学领域的重大进展。期刊内容涵盖了最新的理论发展、实验结果及其解释、核结构、重离子相互作用、在太阳和大气中观察到的中微子振荡、重夸克物理学、粒子和核物理学对天体粒子物理学的影响，以及加速器设计和仪器的最新进展。

Annual Review of Nuclear and Particle Science

Over the past few years new physics methods and algorithms as well as the latest supercomputers have enabled the study of the QCD thermodynamic phase transition using lattice gauge theory numerical simulations with unprecedented control over systematic errors. This is largely a consequence of the ability to perform continuum extrapolations with physical quark masses. Here we review recent progress in lattice QCD thermodynamics, focussing mainly on results that benefit from the use of physical quark masses: the crossover temperature, the equation of state, and fluctuations of the quark number susceptibilities. In addition, we place a special emphasis on calculations that are directly relevant to the study of relativistic heavy ion collisions at RHIC and the LHC.

R.A. Soltz

C. DeTar

F. Karsch

Swagato Mukherjee

P. Vranas

Lattice QCD Thermodynamics with Physical Quark Masses

We review collective flow, its anisotropies, and its event-to-event fluctuations in relativistic heavy-ion collisions, as well as the extraction of the specific shear viscosity of quark–gluon plasma from collective flow data collected in heavy-ion collision experiments at RHIC and the LHC. We emphasize the similarities between the Big Bang of our universe and the Little Bangs created in heavy-ion collisions.

Ulrich Heinz

Raimond Snellings

Collective Flow and Viscosity in Relativistic Heavy-Ion Collisions

相对论重离子碰撞中的集体流与粘度

The bulk motion of nuclear matter at the ultrahigh temperatures created in heavy ion collisions at the Relativistic Heavy Ion Collider and the Large Hadron Collider is well described in terms of nearly inviscid hydrodynamics, thereby establishing this system of quarks and gluons as the most perfect fluid in nature. A revolution in the field is under way, spearheaded by the discovery of similar collective, fluid-like phenomena in much smaller systems including p+ p, p+ A, d+Au, and 3 He+Au collisions. We review these exciting new observations and their profound implications for hydrodynamic descriptions of small and/or out-of-equilibrium systems.

James L. Nagle

William A. Zajc

Small System Collectivity in Relativistic Hadronic and Nuclear Collisions

相对论强子和核碰撞中的小系统集体性

▪ Abstract The proton drip-line defines the limit at which nuclei become unbound to the emission of a proton from their ground states. Low-Z nuclei lying beyond this limit only exist as short-lived resonances and cannot be detected directly. The location of the drip-line constrains the path of nucleosynthesis in explosive astrophysical scenarios such as novae and X-ray bursters, and consequently controls the rate of energy generation. In higher-Z regions of the drip-line, the potential energy barrier resulting from the mutual electrostatic interaction between the unbound proton and the core can cause nuclei to survive long enough to be detected. This review describes the recent major advances in the study of these exotic nuclei. Particular emphasis is placed on understanding the phenomenon of proton radioactivity and the unique insights it offers into the structure of nuclei lying beyond one of nature's fundamental limits to stability.

P. J. Woods

C. N. Davids

NUCLEI BEYOND THE PROTON DRIP-LINE

质子滴线外的核

Almost 30 years have passed since the successful detection of supernova neutrinos from SN 1987A. In the last decades, remarkable progress has been made in neutrino detection technique, through which it may be possible to detect neutrinos from a new source, pre-supernova (pre-SN) neutrinos. They are emitted from a massive star prior to core bounce. Because neutrinos escape from the core freely, they carry information about the stellar physics directly. Pre-SN neutrinos may play an important role in verifying our understanding of stellar evolution for massive stars. Observations of pre-SN neutrinos, moreover, may serve as an alarm regarding a supernova explosion a few days in advance if the progenitor is located in our vicinity, enabling us to observe the next galactic supernova. In this review, we summarize the current status of pre-SN neutrino studies from both of the theoretical and observational points of view.

C. Kato

K. Ishidoshiro

T. Yoshida

Theoretical Prediction of Presupernova Neutrinos and Their Detection

超新星前中微子的理论预测及其探测

Major advances in experimental nuclear and particle physics are often motivated by the need to answer challenging questions. In 2009, Monreal and Formaggio were motivated by the problem of measuring the absolute mass of the neutrino to propose the technique that would come to be called cyclotron radiation emission spectroscopy (CRES). They needed to measure the energies of the electrons from tritium beta decay with extremely high precision, which could be achieved by measuring the frequency of the cyclotron radiation from many individual magnetically trapped electrons. The technique was put into practice first by the Project 8 Collaboration and then by the He6-CRES Collaboration for the study of nonstandard weak interactions. In this review, we present the CRES experiments that have been performed to date, describe the phenomenology of CRES that has so far been explored, and cover potential applications of CRES that have been proposed.

Noah S. Oblath

Brent A. VanDevender

Cyclotron Radiation Emission Spectroscopy

回旋辐射发射光谱学

Three double-ring B factories—PEP-II, KEKB, and SuperKEKB—were built with asymmetric beam energies to produce high luminosity at the Υ(4S) resonance producing copious B mesons and associated particle physics data, delivered to their respective particle physics detectors, BaBar, Belle, and Belle II. In PEP-II and KEKB, the primary goal was achieved to make the first measurements of charge parity (CP) violation in decays in the B meson system. PEP-II and KEKB have finished beam operations, but particle data analysis continues. SuperKEKB is extending those measurements. The beam operation of SuperKEKB with Belle II has recently started. These three accelerators have pushed the state of the art of accelerators of two-ring colliders, including small beam emittances, small interaction point beam sizes, large stored beam currents, crab cavities, top-up injection with the detectors on, bunch-by-bunch feedbacks, crab waist operation, high beam–beam parameters, high peak luminosity, and high integrated luminosity.

John T. Seeman

High-Luminosity B Factory e+e− Colliders

高亮度B工厂e+e−对撞机

Fast radio bursts (FRBs) are brief, highly dispersed bursts detected in the radio band that originate from cosmological distances. The only such event detected in the Milky Way Galaxy, FRB 20200428D—which was associated with an X-ray burst emitted by a magnetar named SGR J1935+2154—revealed the first case of a multiwavelength counterpart of an FRB. Counterparts in other wavelengths accompanying or following FRBs, as well as the bright emission associated with the progenitor of the FRB engine, have been proposed in various FRB models, but no robust detection has been made so far. In general, FRBs as we know them are not favored multimessenger emitters. Nonetheless, possible neutrino and gravitational wave emission signals associated with FRBs or FRB-like events have been discussed in the literature. Here I review these suggested multiwavelength and multimessenger counterparts of FRBs or FRB-like events and the observational progress in searching for these signals. Topics include multiwavelength (X-rays, γ-rays, optical) emission and neutrino emission from FRBs within the framework of the magnetar source models and possible FRB-like events associated with gravitational waves.

Bing Zhang

Multiwavelength and Multimessenger Counterparts of Fast Radio Bursts

快速射电暴的多波段和多信使对应体

Recent strategy updates by the international particle physics community have confirmed strong interest in a next-generation energy frontier collider after completion of the High-Luminosity LHC program and construction of a e + e − Higgs factory. Both hadron and muon colliders provide a path toward the highest energies, and both require significant and sustained development to achieve technical readiness and optimize the design. For hadron colliders, the energy reach is determined by machine circumference and the strength of the guiding magnetic field. To achieve a collision energy of 100 TeV while limiting the circumference to 100 km, a dipole field of 16 T is required and is within the reach of niobium–tin magnets operating at 1.9 K. Magnets based on high-temperature superconductors may enable a range of alternatives, including a more compact footprint, a reduction of the cooling power, or a further increase of the collision energy to 150 TeV. The feasibility and cost of the magnet system will determine the possible options and optimal configurations. In this article, I review the historical milestones and recent progress in superconducting materials, design concepts, magnet fabrication, and test results and emphasize current developments that have the potential to address the most significant challenges and shape future directions.

GianLuca Sabbi

High-Field Magnets for Future Hadron Colliders

未来强子对撞机用的高场磁体

Will neutrinos find uses outside basic science? It may be too early to say, but neutrino physicists have already imagined a variety of possibilities from the relatively modest to the more blue-sky. In this review, we survey the range of proposed applications, most involving nuclear reactors and other fission sources. We give special attention to the most recent proposals, including verifying submarine reactor integrity, safeguarding advanced nuclear power plants, and monitoring spent nuclear fuel. All of these concepts take advantage of the fact that neutrinos pass through barriers other signals cannot penetrate. That same fact creates the central challenge for neutrino applications: the size and complexity of detectors needed to collect a signal. Although the weakly interacting nature of neutrinos makes them fundamentally difficult to use, developments in detector technology are making some ideas more feasible.

短名	Annu. Rev. Nucl. Part. Sci.
Journal Impact	9.04
国际分区	PHYSICS, PARTICLES & FIELDS(Q1)
期刊索引	SCI Q1中科院 2 区

ISSN	0163-8998, 1545-4134
h-index	113
国内分区	物理与天体物理(2区)物理与天体物理物理核物理(2区)物理与天体物理物理粒子与场物理(2区)

涉及主题	物理核物理学量子力学粒子物理学原子物理学天体物理学天文光学数学工程类
出版信息	出版商: Annual Reviews Inc.，出版周期: Annual，期刊类型: book-series，开源期刊: 否
基本数据	创刊年份: 1990，原创研究文献占比: 0.00%，自引率:1.10%， Gold OA占比: 77.78%
平均审稿周期	网友分享经验：约稿?周期不定
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