JCW had long wanted to write a new monograph on supernovae. Despite an immense
explosion in the literature and many review articles, there had not been one since that of …

We study gravitational waves (GWs) from a set of 2D multigroup neutrino radiation
hydrodynamic simulations of core-collapse supernovae (CCSNe). Our goal is to systematize …

Recently born magnetars are promising candidates for the engines powering fast radio
bursts (FRBs). The focus thus far has been placed on millisecond magnetars born in rare …

The coalescence of binary neutron stars (NSs) may in some cases produce a stable massive
NS remnant rather than a black hole. Due to the substantial angular momentum from the …

We present gravitational wave (GW) signal predictions from four 3D multigroup neutrino
hydrodynamics simulations of core-collapse supernovae of progenitors with 11.2, 20 and 27 …

Abstract Approximately 1/4–1/2 of short duration gamma-ray bursts (GRBs) are followed by
variable X-ray emission lasting∼ 100 s with a fluence comparable or exceeding that of the …

The next galactic core-collapse supernova (CCSN) has already exploded, and its
electromagnetic (EM) waves, neutrinos, and gravitational waves (GWs) may arrive at any …

Interferometric detectors will very soon give us an unprecedented view of the gravitational-
wave sky, and in particular of the explosive and transient Universe. Now is the time to …

Massive neutron stars (NSs) with lifetimes of at least several seconds are expected to be the
result of a sizable fraction of NS mergers. We study their formation using a large set of …

We present a detailed theoretical analysis of the gravitational wave (GW) signal of the post-
bounce evolution of core-collapse supernovae (SNe), employing for the first time relativistic …