Overview
This course aims to explore the quest for the 'Theory of Everything' in physics, which involves merging quantum theory and the general theory of relativity. The learning outcomes include understanding the behavior of very large and very small entities, as well as the attempt to unify these theories into a comprehensive mathematical framework. The course covers topics such as the size and spectrum of the Sun, nuclear fusion, radioactive decay, galaxies, measuring stars, the Doppler Effect, distances in space, the Hubble Law, and the age of the Universe. The teaching method involves a presentation by astrophysicist John Gribbin, supplemented with theoretical explanations and historical context. This course is intended for individuals interested in physics, astronomy, cosmology, and the fundamental principles governing the universe.
Syllabus
Introduction
Size of the Sun
Spectrum of the Sun
Nuclear Fusion
ProtonProton Chain
Radioactive Decay
Galaxy
Cepheid variables
Henrietta Swan
Measuring Stars
Andromeda Nebula
The Doppler Effect
Measuring the Distances
Velocity and Distance
Alexander Friedman
George Lamech
Arthur Eddington
Lamech
Observation
Hubbles Law
Hubble Constant
Hubble Telescope
Hubble Deep Field
Hubble Law
Virgo Cluster
The Beginning
Background Radiation
Planck Data
Standard Art Model
The Age of the Universe
Quantum Physics and General Theory
Taught by
The Royal Institution