Stellar Mass Black Hole Formation and Multimessenger Signals from Core-Collapse Supernovae
Detection of gravitational waves from a nearby core-collapse supernova could be the next milestone of gravitational-wave astronomy and multimessenger astrophysics. In this presentation, I will discuss the numerical challenges in modeling for these systems that involved detailed both micro- and macro-physics and present a few recent full 3D simulations with neutrino transport. In particular, I will focus on the dynamics of stellar-mass black hole formation and the effects of rotation on the explosion engines and unique gravitational wave features that might be detected with the current gravitational wave detectors, e.g., Advanced LIGO, Virgo, and KAGRA.
[Lunchbox Registration]
If you will attend the seminar and would like to have a lunchbox on that day, please fill out the online registration form below by 10:00AM Nov. 18th (Wednesday morning). Late registration will not be accepted.
*Note:
1. The lunchboxes will only be prepared for the participation of professors and postdoctoral researchers.
2. In order to prevent the potential spread of COVID-19, we suggest that you bring your own face mask and wear it while attending the seminar.
3. You may check this web page again later after you have completed the online registration. The data for the list of registered attendees will be updated every 5 minutes and shown at the page.
