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Large Scale Structure Theory - Class 4

ICTP-SAIFR via YouTube

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 from Roman Scoccimarro of New York University as he presents the fourth installment of his specialized series on large scale structure theory, building upon previous concepts to examine more complex theoretical frameworks. Gain insights into the mathematical models and physical principles that describe how matter organizes itself into the cosmic web of galaxies, clusters, and voids we observe today. Understand the statistical methods and analytical techniques used to study structure formation, including perturbation theory, correlation functions, and power spectra. Examine how dark matter and dark energy influence the growth of structures over cosmic time, and discover the connections between theoretical predictions and observational data from large-scale surveys. This advanced-level presentation is designed for graduate students, researchers, and professionals in cosmology and astrophysics seeking to deepen their understanding of the theoretical underpinnings of cosmic structure formation.

Syllabus

Roman Scoccimarro: Large scale structure theory - Class 4

Taught by

ICTP-SAIFR

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