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Explore the cutting-edge field of continuous gravitational wave astronomy through this comprehensive summer school program organized by the International Centre for Theoretical Sciences. Delve into the physics and detection methods for continuous gravitational waves, moving beyond the now-routine observations of compact binary mergers to investigate more exotic and persistent sources. Master the astrophysics of neutron stars and binary systems through detailed lectures covering stellar evolution, magnetic field dynamics, and emission mechanisms. Investigate the fascinating phenomenon of ultralight boson clouds that can form around black holes and their potential as gravitational wave sources. Study rapidly spinning neutron stars as continuous wave emitters, examining various emission mechanisms including magnetic dipole radiation, r-mode instabilities, and crustal deformations. Learn sophisticated search methodologies and data analysis techniques used to hunt for these elusive continuous signals in LIGO, Virgo, and KAGRA detector data. Gain insights from leading experts including Dipankar Bhattacharya on neutron star astrophysics, Nils Siemonsen on exotic black hole physics, Keith Riles on neutron star emission mechanisms, and Alicia Sintes on advanced search algorithms and current observational results. Understand the theoretical foundations, computational challenges, and observational prospects for detecting continuous gravitational waves in upcoming detector runs, positioning yourself at the forefront of this rapidly evolving field that promises to unlock new windows into extreme astrophysical phenomena.
