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Overview
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Explore advanced concepts in large scale structure theory through this comprehensive lecture delivered as part of the V Joint ICTP-Trieste/ICTP-SAIFR School on Cosmology. Delve into the theoretical foundations that govern the formation and evolution of cosmic structures across vast scales in the universe. Learn about the mathematical frameworks and physical principles that describe how matter organizes itself into the web-like patterns of galaxies, clusters, and voids observed in the cosmos today. Examine the role of dark matter, gravitational instabilities, and non-linear dynamics in shaping the large-scale distribution of matter. Understand how theoretical predictions connect to observational data from galaxy surveys and cosmic microwave background measurements. Gain insights into perturbation theory, correlation functions, and statistical methods used to analyze cosmic structure formation. This second installment in the lecture series builds upon foundational concepts to address more sophisticated aspects of cosmological structure theory, providing essential knowledge for students and researchers working in theoretical cosmology and astrophysics.
Syllabus
Roman Scoccimarro: Large scale structure theory - Class 2
Taught by
ICTP-SAIFR