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This course provides an introduction to Cosmological Perturbation Theory, focusing on the fundamental concepts and principles in this field. Students will learn about the theory's applications in understanding the universe's large-scale structure and evolution. The course aims to equip learners with the necessary skills to analyze and interpret cosmological data using perturbation theory. The teaching method involves theoretical lectures and possibly practical exercises to reinforce learning. This course is intended for students and professionals interested in cosmology, astrophysics, or theoretical physics, looking to deepen their understanding of the universe's dynamics and evolution.
