Gravitational Waves and Neutron Star Equation of State

量子物理学・ナノサイエンス第428回セミナー

概要

The neutron star binary GW170817 detected via gravitational waves and the neutron star observed by NICER provide astronomical constraints on the equation of state (EoS) of dense matter. More precise and diverse astronomical observations are expected to further strengthen constraints on the EoS of dense matter. This presentation will focus on gravitational-wave observations and comprehensively discuss related topics. It will also include a brief introduction to research utilising next-generation gravitational-wave detectors.

• 量子物理学・ナノサイエンス第428回セミナー

• 東京科学大学理学院・物理学系 ナノサイエンスを拓く量子物理学拠点　共催