Speaker
Description
With the advent of modern neutrino and gravitational wave detectors, the promise of multi-messenger detections of the next galactic core-collapse supernova has become a certainty. These detections will give insight into more than just the core-collapse supernova mechanism: they may resolve longstanding questions about the structure of the progenitor star and fundamental neutrino physics. Using 1D CCSN simulations, I have explored multi-messenger neutrino and gravitational wave signals from the landscape of CCSN progenitors from 9-120 M
