Gravitational wave detectors are already operating at interesting sensitivity levels, and they
have an upgrade path that should result in secure detections by 2014. We review the …

Gravitational Wave (GW) signal was first detected by Advanced Laser Interferometer
Gravitational-Wave Observatory (aLIGO) in 2005 making GW detection a hotspot. The low …

We investigate systematically the dynamical mass ejection, r-process nucleosynthesis, and
properties of electromagnetic counterparts of neutron-star (NS) mergers in dependence on …

The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and
study gravitational waves (GWs) of astrophysical origin. Direct detection of GWs holds the …

The advanced interferometer network will herald a new era in observational astronomy.
There is a very strong science case to go beyond the advanced detector network and build …

The two-body dynamics in general relativity has been solved perturbatively using the post-
Newtonian (PN) approximation. The evolution of the orbital phase and the emitted …

We perform hydrodynamical simulations of neutron-star mergers for a large sample of
temperature-dependent nuclear equations of state and determine the threshold mass above …

We demonstrate by a large set of merger simulations for symmetric binary neutron stars
(NSs) that there is a tight correlation between the frequency peak of the postmerger …

Neutron star (NS) merger simulations are conducted for 38 representative microphysical
descriptions of high-density matter in order to explore the equation-of-state (EoS) …

RELATIVISTIC SIMULATIONS OF BLACK HOLE–NEUTRON STAR COALESCENCE: THE
JET EMERGES - IOPscience Skip to content IOP Science home Accessibility Help Search all …