The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …

The mergers of double neutron star (NS–NS) and black hole (BH)–NS binaries are
promising gravitational wave (GW) sources for Advanced LIGO and future GW detectors. The …

The cosmic origin of elements heavier than iron has long been uncertain. Theoretical
modelling,,,,,, shows that the matter that is expelled in the violent merger of two neutron stars …

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 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 …

An energetic γ-ray burst (GRB), GRB 211211A, was observed on 11 December 2021,.
Despite its long duration, typically associated with bursts produced by the collapse of …

Gravitational-wave observation together with a large number of electromagnetic
observations shows that the source of the latest gravitational-wave event, GW170817 …

We present a new moment-based energy-integrated neutrino transport code for neutron star
merger simulations in general relativity. In the merger context, ours is the first code to include …

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