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 …

This review aims at providing an extensive discussion of modern constraints relevant for
dense and hot strongly interacting matter. It includes theoretical first-principle results from …

We report on the population properties of compact binary mergers inferred from gravitational-
wave observations of these systems during the first three LIGO-Virgo observing runs. The …

Interpreting high-energy, astrophysical phenomena, such as supernova explosions or
neutron-star collisions, requires a robust understanding of matter at supranuclear densities …

Fully general-relativistic binary-neutron-star (BNS) merger simulations with quark-hadron
crossover (QHC) equations of state (EOS) are studied for the first time. In contrast to EOS …

We report a revised analysis for the radius, mass, and hot surface regions of the massive
millisecond pulsar PSR J0740+ 6620, studied previously with joint fits to NICER and XMM …

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 …

With the aim of exploring the evidence for or against phase transitions in cold and dense
baryonic matter, the inference of the sound speed and equation of state for dense matter in …

The symmetry energy and its density dependence are pivotal for many nuclear physics and
astrophysics applications, as they determine properties ranging from the neutron-skin …