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 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 report results of a search for an isotropic gravitational-wave background (GWB) using
data from Advanced LIGO's and Advanced Virgo's third observing run (O3) combined with …

Mergers of binary neutron stars and black hole–neutron star binaries are among the most
promising sources for ground-based gravitational-wave (GW) detectors and are also high …

Gravitational-wave (GW) and electromagnetic (EM) signals from the merger of a neutron star
(NS) and a black hole (BH) are a highly anticipated discovery. We present a simple formula …

There is irresistible observational evidence that binary systems of compact objects with at
least one neutron star are progenitors of short gamma-ray bursts, as well as a production …

Seconds-long numerical-relativity simulations for black hole–neutron star mergers are
performed for the first time to obtain a self-consistent picture of the merger and post-merger …

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 …

The electromagnetic transients accompanying compact binary mergers (γ-ray bursts,
afterglows and 'macronovae') are crucial to pinpoint the sky location of gravitational wave …

We investigate the nucleosynthesis of heavy elements in the winds ejected by accretion
discs formed in neutron star mergers. We compute the element formation in disc outflows …