Speaker
Pia Jakobus
(Hamburg Observatory)
Description
Core-Collapse Supernovae, the explosions of massive stars, are among the several types of gravitational-wave sources yet to be discovered by gravitational wave interferometers. These cataclysmic events may yield insights into the nuclear EoS at multiple times nuclear saturation density. I will review the current advancements in deducing properties of the proto-compact star from gravitational wave spectrograms obtained through Core-Collapse Supernova simulations. Specifically, I want to discuss the excitation of an inner g-mode located in the interior of the proto-compact star. The frequency of this mode falls within the decihertz range and is linked to the speed of sound at approximately four times saturation density.
Primary author
Pia Jakobus
(Hamburg Observatory)
