Nonspherical mass motions are a generic feature of core-collapse supernovae, and
hydrodynamic instabilities play a crucial role in the explosion mechanism. The first …

Multi-dimensional fluid flow plays a paramount role in the explosions of massive stars as
core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these …

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 …

We have conducted 19 state-of-the-art 3D core-collapse supernova simulations spanning a
broad range of progenitor masses. This is the largest collection of sophisticated 3D …

To date, modern three-dimensional (3D) supernova (SN) simulations have not demonstrated
that explosion energies of 10 51 erg (= 1 bethe= 1 B) or more are possible for neutrino …

We calculate the gravitational-wave (GW) signatures of detailed three-dimensional (3D) core-
collapse supernova simulations spanning a range of massive stars. Most of the simulations …

Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the
infall dynamics of the stellar core, triggering and fueling the explosion and driving the …

Double neutron stars (DNSs) have been observed as Galactic radio pulsars, and the recent
discovery of gravitational waves from the DNS merger GW170817 adds to the known DNS …

The details of the physical mechanism that drives core-collapse supernovae (CCSNe)
remain uncertain. While there is an emerging consensus on the qualitative outcome of …

A bstract We revisit constraints on dark photons with masses below∼ 100 MeV from the
observations of Supernova 1987A. If dark photons are produced in sufficient quantity, they …