Quantum Chromodynamics, the theory of quarks and gluons, whose interactions can be
described by a local SU (3) gauge symmetry with charges called “color quantum numbers” …

The nuclear equation of state (EOS) is at the center of numerous theoretical and
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …

We discuss an interpretation that a peak in the sound velocity in neutron star matter, as
suggested by the observational data, signifies strongly coupled conformal matter. The …

In recent years our understanding of neutron stars has advanced remarkably, thanks to
research converging from many directions. The importance of understanding neutron star …

We consider quarkyonic matter to naturally explain the observed properties of neutron stars.
We argue that such matter might exist at densities close to that of nuclear matter, and at the …

We review results for the phase diagram of QCD, the properties of quarks and gluons and
the resulting properties of strongly interacting matter at finite temperature and chemical …

Generating an ensemble of equations of state that fulfill multimessenger constraints, we
statistically determine the properties of dense matter found inside neutron stars (NSs). We …

Information on the phase structure of strongly interacting matter at high baryon densities can
be gained from observations of neutron stars and their detailed analysis. In the present work …

The current status of theoretical studies on the quantum chromodynamics (QCD) phase
diagram at finite temperature and baryon chemical potential is reviewed with special …

Magnetic fields created in the noncentral heavy-ion collision are studied within a
microscopic transport model, namely the Ultrarelativistic Quantum Molecular Dynamics …