Course Outline
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Unit #
- Introduction
- Fundamental Observations
2.1 The Night Sky is Dark
2.2 On Large Scales, the Universe Is Isotropic and Homogeneous
2.3 Galaxies Show a Redshift Proportional to Their Distance
2.4 The Universe Contains Different Types of Particles
2.5 The Universe Is Filled with a Cosmic Microwave Background
- Newton Versus Einstein
3.1 Newton's Way
3.2 Einstein's Way: Special Relativity
3.3 Einstein’s Way: General Relativity and the Equivalence Principle
3.4 Describing Curvature
3.5 The Robertson-Walker Metric
3.6 Proper Distance
- Cosmic Dynamics
4.1 Einstein's Field Equation
4.2 The Friedmann Equation
4.3 The Fluid and Acceleration Equations
4.4 Equations of State
4.5 Learning to Love Lambda
- Model Universes
5.1 Evolution of Energy Density
5.2 Empty Universe
5.3 Single-Component Universes
5.3.1 Matter only
5.3.2 Radiation only
5.3.3 Lambda only
5.4 Multiple-Component Universes
5.4.1 Matter + Curvature
5.4.2 Matter + Lambda
5.4.3 Matter + Curvature + Lambda
5.4.4 Radiation + Matter
5.4 Benchmark Model
- Measuring Cosmological Parameters
6.1 "A Search for Two Numbers"
6.2 Luminosity Distance
6.3 Angular-Diameter Distance
6.4 Standard Candles and the Hubble Constant
6.5 Standard Candles and the Accelerating Universe
- Dark Matter
7.1 Visible Matter
7.2 Dark Matter in Galaxies
7.3 Dark Matter in Clusters
7.4 Gravitational Lensing
7.5 What's the Matter?
- The Cosmic Microwave Background
8.1 Observing the CMB
8.2 Recombination and Decoupling
8.3 The Physics of Recombination
8.4 Temperature Fluctuations
8.5 What Causes the Fluctuations?
- Nucleosynthesis and the Early Universe
9.1 Nuclear Physics and Cosmology
9.2 Neutrons and Protons
9.3 Deuterium Synthesis
9.4 Beyond Deuterium
9.5 Baryon-Antibaryon Asymmetry
- Inflation and the Very Early Universe
10.1 The Flatness Problem
10.2 The Horizon Problem
10.3 The Monopole Problem
10.4 The Inflation Solution
10.5 The Physics of Inflation
- Structure Formation: Gravitational Instability
11.1 The Matthew Effect
11.2 The Jeans Length
11.3 Instability in an Expanding Universe
11.4 The Power Spectrum
11.5 Hot Versus Cold
11.6 Baryon Acoustic Oscillations
- Structure Formation: Baryons and Photons
12.1 Baryonic Matter Today
12.2 Reionization of Hydrogen
12.3 The First Stars and Quasars
12.4 Making Galaxies
12.5 Making Stars
17 January 2017
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