8–13 Sept 2025
Integrated Innovation Building (IIB), RIKEN Kobe Campus
Asia/Tokyo timezone
Registration is closed. We look forward to seeing you in Kobe!

Investigating ultra-high-density equations of state through gravitational waves from binary neutron stars mergers

9 Sept 2025, 09:50
30m
Auditorium (8F) (Integrated Innovation Building (IIB), RIKEN Kobe Campus)

Auditorium (8F)

Integrated Innovation Building (IIB), RIKEN Kobe Campus

Minatojima-minamimachi 6-7-1, Kobe, Japan
8. Theory of compact stars, including neutron star mergers and supernovae NuSym Scientific Session

Speaker

Prof. Luca Baiotti (The University of Osaka)

Description

After an overview of the current status of astrophysical observations and numerical simulations of binary neutron star mergers, I will present our ideas on how to possibly discriminate equations of state (EOSs) with a quark-hadron crossover with respect to EOSs with purely hadronic matter or with a first-order quark-hadron transition through gravitational waves emitted in binary neutron star mergers.

Presentation Style Invited Speaker

Author

Prof. Luca Baiotti (The University of Osaka)

Presentation materials