Course

The Early Universe

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Best after Relativity, Statistical Physics, Differential Equations

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Start here 1.1 Homogeneity, Isotropy and the Cosmological Principle Unit 1 · The Expanding Universe Start Then in this unit: 1.2 Uniform Expansion and the Scale Factor; 1.3 Comoving Coordinates and Proper Distance; 1.4 Cosmological Redshift: Stretched with Space

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The map

1.1 Homogeneity, Isotropy and the Cosmological Principle Ready to start needs nothing · opens Start lesson

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Unit 1 · 0/5 The Expanding Universe

Unit 2 · 0/6 The Dynamics of Homogeneous Expansion

Unit 3 · 0/5 Non-Euclidean Spaces

Unit 4 · 0/5 The Spacetime Metric and Geodesics

Unit 5 · 0/6 Black-Body Radiation and the Thermal History

Unit 6 · 0/5 The Cosmic Microwave Background

Unit 7 · 0/6 The Cosmological Constant and the Accelerating Universe

Unit 8 · 0/6 Big-Bang Nucleosynthesis

Unit 9 · 0/7 Problems of the Hot Big Bang, and Inflation

Unit 10 · 0/7 Density Fluctuations and the Growth of Structure