Strong Gravity
Cosmic collisions: neutron-star astrophysics with gravitational wavesConfirmed
by
→
America/Toronto
PI/4-405 - Bob Room (Perimeter Institute for Theoretical Physics)
PI/4-405 - Bob Room
Perimeter Institute for Theoretical Physics
60
Description
As endpoints of massive stellar evolution, showcases for the densest matter in the universe, and sites for heavy element nucleosynthesis, neutron star mergers are superb laboratories for astrophysics, strong gravity and nuclear physics. Gravitational-wave observations of these mergers are beginning to reveal neutron stars’ internal structure, provide insight into the astrophysical processes that form them, and expose their role in the chemical evolution of the Galaxy. I will survey some of my recent work in these areas and describe how our theoretical understanding of neutron stars is being shaped by gravitational-wave discoveries.
Organised by
Will East