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

Like all true stars, massive stars are gravitationally confined thermonuclear reactors whose
composition evolves as energy is lost to radiation and neutrinos. Unlike lower-mass stars …

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 …

As the number of merging binary black holes observed with ground-based gravitational-
wave detectors grows, increasingly accurate theoretical models are required to compare …

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Gravitational-wave detections are starting to allow us to probe the physical processes in the
evolution of very massive stars through the imprints they leave on their final remnants …

Studying the formation and evolution of black hole binaries (BHBs) is essential for the
interpretation of current and forthcoming gravitational wave (GW) detections. We investigate …

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 …

Understanding the link between massive (≳ 30 M⊙) stellar black holes (BHs) and their
progenitor stars is a crucial step to interpret observations of gravitational-wave events. In this …

The first four gravitational wave events detected by LIGO were all interpreted as merging
black hole binaries (BHBs), opening a new perspective on the study of such systems. Here …