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 …

Multi-messenger astrophysics, a long-anticipated extension to traditional multiwavelength
astronomy, has emerged over the past decade as a distinct discipline providing unique and …

Abstract The Einstein Telescope (ET), a proposed European ground-based gravitational-
wave detector of third-generation, is an evolution of second-generation detectors such as …

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 …

We have simulated the collapse and evolution of the core of a solar-metallicity 40 M⊙ star
and find that it explodes vigorously by the neutrino mechanism, despite its very high" …

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 …

Abstract Machine learning has emerged as a popular and powerful approach for solving
problems in astrophysics. We review applications of machine learning techniques for the …

This paper presents the results of a search for generic short-duration gravitational-wave
transients in data from the third observing run of Advanced LIGO and Advanced Virgo …

The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-
generation opportunity to obtain detailed information about the explosion of a star and …

Using 20 long-term 3D core-collapse supernova simulations, we find that lower
compactness progenitors that explode quasi-spherically due to the short delay to explosion …