Lecture 35 - The Expanding Universe
In 1922, Alexander Friedmann proved that an isotropic, homogeneous universe cannot be static. By 1929, Hubble demonstrated that the clusters of galaxies are receding from us. Even prior to that, George Lemaitre had argued that if the universe is expanding, then it must have been very small and very hot in the beginning. In 1940, George Gamow conjectured that the elements may have been synthesized in the early universe. In this first of six lectures on Cosmology, I explain the expanding universe scenario, and the synthesis of light elements such as Deuterium and Helium. The synthesis of heavy elements in the stars, as well as exotic scenarios like the coalescence of two neutron stars, is also discussed.