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- Chapter 1 Introduction 1
- Chapter 2 Fundamental Observations 7
- 2.1 Dark night sky 7
- 2.2 Isotropy and homogeneity 11
- 2.3 Redshift proportional to distance 15
- 2.4 Types of particles 22
- 2.5 Cosmic microwave background 28
- Chapter 3 Newton Versus Einstein 32
- 3.1 Equivalence principle 33
- 3.2 Describing curvature 39
- 3.3 Robertson-Walker metric 44
- 3.4 Proper distance 47
- Chapter 4 Cosmic Dynamics 55
- 4.1 Friedmann equation 57
- 4.2 Fluid and acceleration equations 65
- 4.3 Equations of state 68
- 4.4 Learning to love lambda 71
- Chapter 5 Single-Component Universes 79
- 5.1 Evolution of energy density 79
- 5.2 Curvature only 86
- 5.3 Spatially flat universes 91
- 5.4 Matter only 94
- 5.5 Radiation only 95
- 5.6 Lambda only 97
- Chapter 6 Multiple-Component Universes 101
- 6.1 Matter + curvature 104
- 6.2 Matter + lambda 108
- 6.3 Matter + curvature + lambda 112
- 6.4 Radiation + matter 116
- 6.5 Benchmark Model 118
- Chapter 7 Measuring Cosmological Parameters 126
- 7.1 A search for two numbers 126
- 7.2 Luminosity distance 131
- 7.3 Angular-diameter distance 136
- 7.4 Standard candles & H0 141
- 7.5 Standard candles & acceleration 144
- Chapter 8 Dark Matter 155
- 8.1 Visible matter 156
- 8.2 Dark matter in galaxies 159
- 8.3 Dark matter in clusters 164
- 8.4 Gravitational lensing 170
- 8.5 What’s the matter? 175
- Chapter 9 The Cosmic Microwave Background 179
- 9.1 Observing the CMB 180
- 9.2 Recombination and decoupling 185
- 9.3 The physics of recombination 189
- 9.4 Temperature fluctuations 196
- 9.5 What causes the fluctuations? 201
- Chapter 10 Nucleosynthesis & the Early Universe 208
- 10.1 Nuclear physics and cosmology 209
- 10.2 Neutrons and protons 213
- 10.3 Deuterium synthesis 218
- 10.4 Beyond deuterium 222
- 10.5 Baryon – antibaryon asymmetry 228
- Chapter 11 Inflation & the Very Early Universe 233
- 11.1 The flatness problem 234
- 11.2 The horizon problem 236
- 11.3 The monopole problem 238
- 11.4 The inflation solution 242
- 11.5 The physics of inflation 247
- Chapter 12 The Formation of Structure 255
- 12.1 Gravitational instability 258
- 12.2 The Jeans length 261
- 12.3 Instability in an expanding universe 266
- 12.4 The power spectrum 272
- 12.5 Hot versus cold 276
- Chapter 13 Epilogue 284
- Chapter 14 Annotated Bibliography 286
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