Speaker
Prof.
Tomoya Takiwaki
(National Astronomical Observatory of Japan)
Description
Neutrino and gravitational wave are indispensable messengers of core-collapse supernovae. Those messengers have important information on how the supernovae are initiated.
Helped by recent development of the simulation technique, we can provide the prediction on the gravitational waveforms and neutrino light curves as well as the neutrino spectrum.
In addition to the normal non-rotating progenitors, we succeed the simulations of rapidly rotating progenitors. Their messengers have surprisingly interesting features. In this talk, we discuss which physical quantity we can extract from the messengers in the core-collapse supernovae.
Primary author
Prof.
Tomoya Takiwaki
(National Astronomical Observatory of Japan)
