Recent progress and new challenges in isospin physics with heavy-ion reactions

BA Li, LW Chen, CM Ko - Physics Reports, 2008 - Elsevier
The ultimate goal of studying isospin physics via heavy-ion reactions with neutron-rich,
stable and/or radioactive nuclei is to explore the isospin dependence of in-medium nuclear …

In-medium nuclear interactions of low-energy hadrons

E Friedman, A Gal - Physics Reports, 2007 - Elsevier
Exotic atoms provide a unique laboratory for studying strong interactions and nuclear
medium effects at zero kinetic energy. Experimental and theoretical developments of the last …

Hadron properties in the nuclear medium

RS Hayano, T Hatsuda - Reviews of Modern Physics, 2010 - APS
The QCD vacuum shows the dynamical breaking of chiral symmetry. In the hot and/or dense
QCD medium, the chiral order parameter such as⟨ q¯ q⟩ is expected to change as a …

[HTML][HTML] Neutron star equation of state: Quark mean-field (QMF) modeling and applications

A Li, ZY Zhu, EP Zhou, JM Dong, JN Hu… - Journal of High Energy …, 2020 - Elsevier
Because of the development of many-body theories of nuclear matter, the long-standing,
open problem of the equation of state (EOS) of dense matter may be understood in the near …

[HTML][HTML] Can the PREX-2 and CREX results be understood by relativistic mean-field models with the astrophysical constraints?

T Miyatsu, MK Cheoun, K Kim, K Saito - Physics Letters B, 2023 - Elsevier
We construct new effective interactions using the relativistic mean-field models with the
isoscalar-and isovector-meson mixing, σ 2 δ 2 and ω μ ω μ ρ ν ρ ν. Taking into account the …

The Challenge of the EMC Effect: existing data and future directions

S Malace, D Gaskell, DW Higinbotham… - International Journal of …, 2014 - World Scientific
Since the discovery that the ratio of inclusive charged lepton (per-nucleon) cross-sections
from a nucleus A to the deuteron is not unity—even in deep inelastic scattering kinematics …

Neutron star equation of state from the quark level in light of GW170817

ZY Zhu, EP Zhou, A Li - The Astrophysical Journal, 2018 - iopscience.iop.org
The matter state inside neutron stars (NSs) is an exciting problem in astrophysics, nuclear
physics, and particle physics. The equation of state (EOS) of NSs plays a crucial role in the …

Nuclear-bound quarkonia and heavy-flavor hadrons

G Krein, AW Thomas, K Tsushima - Progress in Particle and Nuclear …, 2018 - Elsevier
In our quest to win a deeper understanding of how QCD actually works, the study of the
binding of heavy quarkonia and heavy-flavor hadrons to atomic nuclei offers enormous …

and mesons with connection to anomalous glue

SD Bass, P Moskal - Reviews of Modern Physics, 2019 - APS
A review of the present understanding of η′ and η meson physics and these mesons as a
probe of gluon dynamics in low-energy QCD is presented. Recent highlights include the …

Implications of neutron star properties for the existence of light dark matter

TF Motta, PAM Guichon… - Journal of Physics G …, 2018 - iopscience.iop.org
It was recently suggested that the discrepancy between two methods of measuring the
lifetime of the neutron may be a result of an unseen decay mode into a dark matter particle …