We review the current status and recent progress of microscopic many-body approaches
and phenomenological models, which are employed to construct the equation of state of …

Despite their long history and astrophysical importance, some of the key properties of
neutron stars are still uncertain. The extreme conditions encountered in their interiors …

We report on Bayesian parameter estimation of the mass and equatorial radius of the
millisecond pulsar PSR J0030+ 0451, conditional on pulse-profile modeling of Neutron Star …

We present a systematic numerical relativity study of the mass ejection and the associated
electromagnetic transients and nucleosynthesis from binary neutron star (NS) mergers. We …

The density dependence of nuclear symmetry energy is among the most uncertain parts of
the Equation of State (EOS) of dense neutron-rich nuclear matter. It is currently poorly known …

Is the secondary component of GW190814 the lightest black hole or the heaviest neutron
star ever discovered in a double compact-object system [Abbott et al. Astrophys. J. 896, L44 …

In this article, I introduce ideas and techniques to extract information about the equation of
state of matter at very high densities from gravitational waves emitted before, during and …

The recent detection of GW190814 featured the merger of a binary with a primary having a
mass of and a secondary with a mass of. While the primary was most likely a black hole, the …

We combine gravitational wave (GW) and electromagnetic (EM) data to perform a Bayesian
parameter estimation of the binary neutron star (NS) merger GW170817. The EM likelihood …

Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …