Speaker
Tomoya Takiwaki
(Tomoya)
Description
Gravitational wave signal from core-collapse supernova is the key to understand the mechanism of core-collapse supernovae. The evolution of the frequency of the signal tells us the property of neutron star and information of the accretion flow near the neutron star. In this study, I will introduce the gravitational waveform based on our recent 3D simulations and discuss what information extracted from the signal.
Primary author
Tomoya Takiwaki
(Tomoya)
