Cosmological Perturbation Theory - CMB by D Pogosyan

Explore the second lecture on Cosmological Perturbation Theory and Cosmic Microwave Background (CMB) delivered by D Pogosyan as part of the "Cosmology - The Next Decade" program. Delve into advanced concepts of cosmology, focusing on the mathematical framework used to describe small fluctuations in the early universe and their evolution into the CMB we observe today. Gain insights into how these theories help explain the formation of large-scale structures in the universe and provide evidence for the Lambda Cold Dark Matter (LCDM) model. Enhance your understanding of key topics in modern cosmology, including dark matter, dark energy, and the challenges facing current cosmological models.

Cosmological Perturbation Theory / CMB (Lecture 2) by D Pogosyan