Special Issue "Aspects of Particle Physics and High Energy Physics- Dedicated to Zhengdao Li's 95 Anniversary"

A special issue of Symmetry (ISSN 2073-8994). This special issue belongs to the section "Physics".

Deadline for manuscript submissions: 29 February 2024 | Viewed by 4332

Special Issue Editors

1. Information Media Center, Hiroshima University, 1-7-1, Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8521, Japan
2. Core of Research for the Energetic Universe, Hiroshima University, Higashi-Hiroshima 739-8526, Japan
Interests: general aspects of computer science; computational science; high-energy physics and quantum fields; symmetry breaking; informatics in education
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Institute of Physics of Cantabria ,Universidad de Cantabria, Santander, Spain
Interests: physics
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SINP MSU, Lomonosov Moscow State University, Moscow, Russia
Interests: experience in experimental; high energy; heavy ion physics
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Special Issue Information

Dear Colleagues,

This Special Issue of Symmetry, devoted to quantum field theory, elementary particle theory, nuclear physics, statistical mechanics, fluid mechanics, and astrophysics, is dedicated to Prof. Dr. Zhengdao Li's 95th birthday. 

In 1948, Zhengdao Li, working as a student of Enrico Fermi in Chicago and as a colleague of J. Steinberger, was looking for interactions similar to beta decays. He proposed, in collaboration with M.N. Rosenbluth and Z. Yang, the existence of intermediate heavy bosons in weak interactions.

In 1956, in collaboration with Z. Yang, Li was encouraged by Wú Jiànxióng and colleagues to carry out an experiment which would demonstrate the parity violation in weak decays, for which they were awarded the Nobel Prize in Physics in 1957.

Li proposed to Jack Steinberger that he reanalyze his data on hyperon decays, which was actually the first parity violation experiment in weak interactions. The experiment on parity violation, performed in 1956 and published before his theoretical work with Z. Yang, lacked sufficient statistical significance. 

In those years, Li also carried out extensive analyses of other C.P.T symmetries in weak interactions.

Li collaborated extensively with Yang during the 1950s, leading to other important results in statistical mechanics, such as the Li–Yang theorem.

During the 1960s, his studies on massless particles were vital. It was these studies, in collaboration with Nauenberg and, independently, Kinoshita that led to the KLN theorem.

In the 1970s, his studies on matter at high densities influenced relativistic heavy ions collisions physics (RHIC).

Many other fields of physics, including statistical mechanics, astrophysics and hydrodynamics, have been covered by Zhengdao Li during his long career.

In this Special Issue, we want to invite contributions on the subjects developed by Prof. Dr. Zhengdao Li. Personal recollections by people close to him are also welcomed. 

As is apparent, Li’s work covered all the primary areas of active work at present on Particle Physics and High Energy Physics. Therefore, we welcome contributions relating to gravity, cosmology, particle physics phenomenology and experiment, supersymmetry, and relativistic heavy ion collision physics (phenomenology and experiment).

This is the year of Li’s 95th birthday; therefore, we hope to commemorate one of the most important physicists of our time and provide perspectives on the future of fundamental physics as seen by different contributors.

Prof. Dr. Tomohiro Inagaki
Prof. Dr. Alberto Ruiz Jimeno
Dr. Olga Kodolova
Guest Editors

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Published Papers (4 papers)

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Research

Article
Progress of Machine Learning Studies on the Nuclear Charge Radii
Symmetry 2023, 15(5), 1040; https://doi.org/10.3390/sym15051040 - 08 May 2023
Viewed by 688
Abstract
The charge radius is a fundamental physical quantity that describes the size of one nucleus, but contains rich information about the nuclear structure. There are already many machine learning (ML) studies on charge radii. After reviewing the relevant works in detail, the convolutional [...] Read more.
The charge radius is a fundamental physical quantity that describes the size of one nucleus, but contains rich information about the nuclear structure. There are already many machine learning (ML) studies on charge radii. After reviewing the relevant works in detail, the convolutional neural networks (CNNs) are established to reproduce the latest experimental values of charge radii. The extrapolating and interpolating abilities in terms of two CNN structures partnering two inputting matrix forms are discussed, and a testing root-mean-square (RMS) error 0.015 fm is achieved. The shell effect on charge radii of both isotones and isotopes are predicted successfully, and the CNN method works well when predicting the charge radii of a whole isotopic chain. Full article
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Article
Einstein–Yang–Mills-Aether Theory with Nonlinear Axion Field: Decay of Color Aether and the Axionic Dark Matter Production
Symmetry 2022, 14(8), 1621; https://doi.org/10.3390/sym14081621 - 06 Aug 2022
Viewed by 919
Abstract
We establish a nonlinear version of the SU(N)-symmetric theory, which describes self-consistently the interaction between the gravitational, gauge, vector and pseudoscalar (axion) fields. In the context of this theory the SU(N)-symmetric multiplet of vector fields is associated with the color aether, the decay [...] Read more.
We establish a nonlinear version of the SU(N)-symmetric theory, which describes self-consistently the interaction between the gravitational, gauge, vector and pseudoscalar (axion) fields. In the context of this theory the SU(N)-symmetric multiplet of vector fields is associated with the color aether, the decay of which in the early Universe produced the canonic dynamic aether and the axionic dark matter. The SU(N)-symmetric Yang–Mills field, associated with the color aether, forms the source, which transfers the energy of the decaying color aether to the axion field. The nonlinear modification of the model uses explicitly the requirement of discrete symmetry, prescribed by the axion field, and is based on the analogy with a nonlinear physical pendulum. We show that in the framework of this nonlinear regular model, the axion field can grow to an arbitrarily large value, thus explaining the abundance of the axionic dark matter in the Universe. Full article
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Article
Radiation Backreaction in Axion Electrodynamics
Symmetry 2022, 14(6), 1113; https://doi.org/10.3390/sym14061113 - 28 May 2022
Cited by 5 | Viewed by 926
Abstract
Energy–momentum conservation of classical axion electrodynamics is carefully analyzed in the Hamiltonian formulation of the theory. The term responsible for the energy transfer between the electromagnetic and the axion sectors is identified. As a special application, the axion-to-light Primakoff process in the background [...] Read more.
Energy–momentum conservation of classical axion electrodynamics is carefully analyzed in the Hamiltonian formulation of the theory. The term responsible for the energy transfer between the electromagnetic and the axion sectors is identified. As a special application, the axion-to-light Primakoff process in the background of a static magnetic field is worked out and the radiative self-damping of the axion oscillations is characterized quantitatively. The damping time turns out comparable to the age of the Universe in the preferred axion mass range. Full article
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Article
Symmetry Breaking of Universal Type and Particular Types
Symmetry 2022, 14(3), 563; https://doi.org/10.3390/sym14030563 - 12 Mar 2022
Cited by 1 | Viewed by 905
Abstract
The concepts of symmetry and its breakdown are investigated in two different terms according to whether the resulting asymmetry is universal or only obtained for a special configuration: we illustrate this by considering, in the first case, an example from the standard model [...] Read more.
The concepts of symmetry and its breakdown are investigated in two different terms according to whether the resulting asymmetry is universal or only obtained for a special configuration: we illustrate this by considering, in the first case, an example from the standard model of particles with some consequences for cosmological scenarios; and in the second case, we consider an example from specific solutions for the particle dynamics, and an example for a toy model of entangled spins. Full article
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