Summary
Coalescing binary neutron star systems, driven by gravitational-wave emission, provide a rare yet crucial natural laboratory for studying fundamental questions in astrophysics, nuclear physics, and gravitation under extreme conditions. This award supports theoretical research that strengthens the connection between the physical properties of neutron stars and the signals measured by current and next-generation gravitational-wave observatories. By improving the understanding of these observations, it contributes to U.S. leadership in gravitational-wave astronomy. The award also promotes workfor
