Binary neutron star mergers observations are a unique way to constrain fundamental
physics and astrophysics at the extreme. The interpretation of gravitational-wave events and …

The first multimessenger observation of a binary neutron star (BNS) merger in August 2017
demonstrated the huge scientific potential of these extraordinary events. This breakthrough …

Magnetic fields are expected to play a key role in the dynamics and the ejection
mechanisms that accompany the merger of two neutron stars. General relativistic …

We perform a long and accurate large-eddy simulation of a binary neutron star merger,
following the newly formed remnant up to 110 milliseconds. The combination of high-order …

GW170817 and GRB 170817A provided direct evidence that binary neutron star (NSNS)
mergers can produce short gamma-ray bursts (sGRBs). However, questions remain about …

We investigate the impact of a mean field model for the α Ω dynamo potentially active in the
postmerger phase of a binary neutron star coalescence. We do so by deriving equations for …

The amplification of magnetic fields plays an important role in explaining numerous
astrophysical phenomena associated with binary neutron star mergers, such as mass …

We use covariant density functional theory to obtain the equation of state (EoS) of matter in
compact stars at non-zero temperature, including the full baryon octet as well as the Δ …

The recent detections of the∼ 10 s long γ-ray bursts (GRBs) 211211A and 230307A
followed by softer temporally extended emission (EE) and kilonovae point to a new GRB …

We perform general relativistic, magnetohydrodynamic simulations of merging binary
neutron stars incorporating neutrino transport and magnetic fields. Our new radiative …