Rapidly Spinning Neutron Stars and Emission Mechanisms - Lecture 2

Explore the fascinating world of rapidly spinning neutron stars and their emission mechanisms in this lecture by Keith Riles, part of the Summer School on Gravitational-Wave Astronomy. Delve into the potential sources of continuous gravitational waves, focusing on rapidly spinning neutron stars in our galaxy. Learn about the astrophysics behind these extreme objects and the mechanisms that could lead to gravitational wave emission. Gain insights into the upcoming observing runs of LIGO, Virgo, and KAGRA, and understand the possibilities for detecting signals from these intriguing sources. This 91-minute lecture is essential for those interested in advancing their knowledge of gravitational-wave astronomy and the cutting-edge research in this field.

Rapidly Spinning Neutron Stars and Emission Mechanisms (Lecture 2) by Keith Riles