- Lectures
- Institute of Physics
- Location
5F, 1st Meeting Room, Institute of Physics
- Speaker Name
Dr. Hung Tan (Institute of Physics, Academia Sinica)
- State
Definitive
- Url
https://www.phys.sinica.edu.tw/lecture_detail.php?id=3156&eng=T
Abstract
The detection of GW170817 demonstrated that gravitational-wave observations provide a powerful probe of neutron star interiors. Neutron star cores are of particular interest, as they contain cold, ultra-dense matter whose properties remain highly uncertain. The Cosmic Explorer, a next-generation gravitational-wave detector, is expected to observe on the order of 100 neutron star merger events per year with an order-of-magnitude improvement in sensitivity over current detectors. In this talk, I will explore the potential of Cosmic Explorer to constrain the neutron star equation of state.
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