Mergers of binaries consisting of two neutron stars, or a black hole and a neutron star, offer a
unique opportunity to study a range of physical and astrophysical processes using two …

Gravitational waves emitted from the coalescence of neutron star binaries open a new
window to probe matter and fundamental physics in unexplored, extreme regimes. To extract …

Gravitational waves from coalescing neutron stars encode information about nuclear matter
at extreme densities, inaccessible by laboratory experiments. The late inspiral is influenced …

KAGRA is a newly build gravitational wave observatory, a laser interferometer with 3 km arm
length, located in Kamioka, Gifu, Japan. In this paper, one of a series of articles featuring …

Using hydrodynamical simulations for a large set of high-density matter equations of state
(EOSs), we systematically determine the threshold mass M thres for prompt black-hole …

We present a rapid analytic framework for predicting kilonova light curves following neutron
star (NS) mergers, where the main input parameters are binary-based properties …

Gravitational waves from neutron star binary inspirals contain information on strongly
interacting matter in unexplored, extreme regimes. Extracting this requires robust theoretical …

This study addresses the collapse behavior of neutron star (NS) mergers expressed through
the binary threshold mass M thres for prompt black-hole (BH) formation, which we determine …

While it is now known that the mergers of double neutron star binary systems (NSMs) are
copious producers of heavy elements, there remains much speculation about whether they …

Observations of gravitational waves (GW) provide us with a new probe to study the Universe.
GW events can be used as standard sirens if their redshifts are measured. Normally …