Learning

Theoretical Foundations of Large-Scale Structure

Homogeneous Cosmology and FRW Background → N-body Simulations and Calibration

This advanced graduate-level path develops the theoretical framework for understanding the large-scale structure of the universe, from linear perturbation theory to effective field theory approaches. It covers the statistical tools, bias models, nonlinear evolution, redshift-space distortions, and BAO modeling essential for modern cosmological analysis. The path emphasizes the conceptual connections between cosmology, field theory, and statistical physics, preparing learners for research in theoretical cosmology.