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Recent progress and new challenges in isospin physics with heavy-ion reactions
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 …
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 …
medium effects at zero kinetic energy. Experimental and theoretical developments of the last …
[HTML][HTML] Can the PREX-2 and CREX results be understood by relativistic mean-field models with the astrophysical constraints?
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 …
isoscalar-and isovector-meson mixing, σ 2 δ 2 and ω μ ω μ ρ ν ρ ν. Taking into account the …
Hadron properties in the nuclear medium
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 …
QCD medium, the chiral order parameter such as⟨ q¯ q⟩ is expected to change as a …
The Challenge of the EMC Effect: existing data and future directions
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 …
from a nucleus A to the deuteron is not unity—even in deep inelastic scattering kinematics …
Sound velocity peak and conformality in isospin QCD
We study zero temperature equations of state (EOS) in isospin QCD within a quark-meson
model which is renormalizable and hence eliminates high density artifacts in models with …
model which is renormalizable and hence eliminates high density artifacts in models with …
[HTML][HTML] Neutron star equation of state: Quark mean-field (QMF) modeling and applications
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 …
open problem of the equation of state (EOS) of dense matter may be understood in the near …
Nuclear-bound quarkonia and heavy-flavor hadrons
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 …
binding of heavy quarkonia and heavy-flavor hadrons to atomic nuclei offers enormous …
Neutron star equation of state from the quark level in light of GW170817
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 …
physics, and particle physics. The equation of state (EOS) of NSs plays a crucial role in the …
and mesons with connection to anomalous glue
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 …
probe of gluon dynamics in low-energy QCD is presented. Recent highlights include the …