Lecture

Cosmological Evolution: Matter and Radiation

Description

This lecture discusses the evolution of the universe, focusing on the contributions of matter and radiation. It covers the Friedmann equations, Hubble law, redshift, luminosity distance, and the impact of different matter components. The instructor explains the critical density, vacuum energy, and the mechanical interpretation of particle movements in potential fields.

About this result
This page is automatically generated and may contain information that is not correct, complete, up-to-date, or relevant to your search query. The same applies to every other page on this website. Please make sure to verify the information with EPFL's official sources.