The coalescence of double neutron star (NS–NS) and black hole (BH)–NS binaries are
prime sources of gravitational waves (GW) for Advanced LIGO/Virgo and future ground …

We present our current best estimate of the plausible observing scenarios for the Advanced
LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years …

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 …

Gravitational waves detected from the binary neutron star (NS) merger GW170817
constrained the NS equation of state by placing an upper bound on certain parameters …

The merger of two neutron stars has been predicted to produce an optical–infrared transient
(lasting a few days) known as a 'kilonova', powered by the radioactive decay of neutron-rich …

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 detailed study of the methodology for correlatingdark sirens'(compact binaries
coalescences without electromagnetic counterpart) with galaxy catalogs. We propose …

The first multimessenger detection of a binary neutron star (BNS) merger, GW170817, by
LIGO(Aasi et al. 2015) and Virgo(Acernese et al. 2015) enabled the first standard siren …

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 …

We perform a general-relativistic magnetohydrodynamics simulation for≈ 30 ms from the
merger of a binary neutron star throughout the formation of a remnant massive neutron star …