The ground-based gravitational wave (GW) detectors LIGO and Virgo have enabled the birth
of multi-messenger GW astronomy via the detection of GWs from merging stellar-mass black …

We present an improved version of the 3D Monte Carlo radiative transfer code possis to
model kilonovae from neutron star mergers, wherein nuclear heating rates, thermalization …

Fast neutron-rich material ejected dynamically over≲ 10 ms during the merger of a binary
neutron star (BNS) can give rise to distinctive electromagnetic counterparts to the system's …

In this paper, we model the dynamics and radiation physics of the rarity event GRB 221009A
afterglow in detail. By introducing a top-hat jet that propagates in an environment dominated …

In the gravitational wave event GW170817, there was a∼ 10 h gap before electromagnetic
(EM) observations, without detection of the cocoon. The cocoon is heated by a short gamma …

Kilonovae are optical transients following the merger of neutron star binaries, which are
powered by the r-process heating of merger ejecta. However, if a merger remnant is a long …

Given an increasing number of gamma-ray bursts accompanied by potential kilonovae,
there is a growing importance to advance modelling of kilonova afterglows. In this work, we …

We study the long-term () evolution of the accretion disc after a neutron star (NS)–NS or NS–
black hole merger, taking into account the radioactive heating by r-process nuclei formed in …

The behaviour of a short gamma-ray burst (sGRB) afterglow light curve can reveal the
angular structure of the relativistic jet and constrain the observer's viewing angle. The …

Recent work by Moroianu et al. has suggested that the binary neutron star (BNS) merger
GW190425 might have a potential fast radio burst (FRB) counterpart association …