In a single process, the merger of binary neutron star systems combines extreme gravity, the
copious emission of gravitational waves, complex microphysics and electromagnetic …

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 …

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 …

We present a systematic numerical relativity study of the dynamical ejecta, winds, and
nucleosynthesis in neutron star (NS) merger remnants. Binaries with the chirp mass …

The gravitational wave observations GW150914 and GW151226 by Advanced LIGO provide
the first opportunity to learn about physics in the extreme gravity environment of coalescing …

We present fully general-relativistic simulations of binary neutron star mergers with a
temperature and composition dependent nuclear equation of state. We study the dynamical …

We perform three-dimensional general-relativistic magnetohydrodynamic simulations with
weak interactions of binary neutron-star (BNS) mergers resulting in a long-lived remnant …

We present new (3+ 1) D numerical relativity simulations of the binary neutron star (BNS)
merger and postmerger phase. We focus on a previously inaccessible region of the binary …

Binary neutron star mergers observations are a unique way to constrain fundamental
physics and astrophysics at the extreme. The interpretation of gravitational-wave events and …

Inferring the properties of dense matter is one of the most exciting prospects from the
measurement of gravitational waves from neutron star mergers. However, it requires reliable …