Neutron Star Perturbation Theory - Lecture 2

Delve into the intricacies of neutron star physics in this comprehensive lecture on Neutron Star Perturbation Theory. As part of the IAGRG School on Gravitation and Cosmology, renowned expert Nils Andersson from the University of Southampton delivers an in-depth exploration of this cutting-edge topic. Learn about the complex behavior of these dense stellar remnants, focusing on how perturbations affect their structure and dynamics. Gain insights into the mathematical frameworks and physical principles used to analyze neutron star oscillations, instabilities, and their implications for gravitational wave astronomy. Suitable for graduate students and researchers in gravitational physics, this 1 hour and 34 minute lecture provides a solid foundation for understanding the forefront of compact object research in the era of gravitational wave detection.

Neutron Star Perturbation Theory (Lecture 2) by Nils Andersson