Speaker
Dr
Christian Ott
(Caltech, USA)
Description
The next galactic core-collapse supernova will be observed in the
electromagnetic spectrum, in neutrinos, and, for the first time, in
gravitational waves. I review gravitational wave emission from stellar
collapse and the subsequent core-collapse supernova evolution and
discuss how gravitational waves can be used to probe aspects of the
explosion mechanism and physical parameters of the progenitor star.
Author
Dr
Christian Ott
(Caltech, USA)
