Search Talks

We are now in the era of multi-messenger astronomy, where neutron stars and black holes—the most extreme objects in the Universe—can be studied through both electromagnetic signals and gravitational waves. These compact remnants of massive stars provide unique windows into the short lives and deaths of their progenitors and the history of star formation across cosmic time. In this talk, I will show how we can apply cutting-edge computational models to uncover the origins of black holes and neutron stars and to address outstanding puzzles, including how and where the gravitational wave mergers detected by LIGO/Virgo/KAGRA are formed.