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bhishantryphysics

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Mar 25th, 2017
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  1. Chapter 1 Introduction 1
  2. Chapter 2 Fundamental Observations 7
  3. 2.1 Dark night sky 7
  4. 2.2 Isotropy and homogeneity 11
  5. 2.3 Redshift proportional to distance 15
  6. 2.4 Types of particles 22
  7. 2.5 Cosmic microwave background 28
  8. Chapter 3 Newton Versus Einstein 32
  9. 3.1 Equivalence principle 33
  10. 3.2 Describing curvature 39
  11. 3.3 Robertson-Walker metric 44
  12. 3.4 Proper distance 47
  13. Chapter 4 Cosmic Dynamics 55
  14. 4.1 Friedmann equation 57
  15. 4.2 Fluid and acceleration equations 65
  16. 4.3 Equations of state 68
  17. 4.4 Learning to love lambda 71
  18. Chapter 5 Single-Component Universes 79
  19. 5.1 Evolution of energy density 79
  20. 5.2 Curvature only 86
  21. 5.3 Spatially flat universes 91
  22. 5.4 Matter only 94
  23. 5.5 Radiation only 95
  24. 5.6 Lambda only 97
  25. Chapter 6 Multiple-Component Universes 101
  26. 6.1 Matter + curvature 104
  27. 6.2 Matter + lambda 108
  28. 6.3 Matter + curvature + lambda 112
  29. 6.4 Radiation + matter 116
  30. 6.5 Benchmark Model 118
  31. Chapter 7 Measuring Cosmological Parameters 126
  32. 7.1 A search for two numbers 126
  33. 7.2 Luminosity distance 131
  34. 7.3 Angular-diameter distance 136
  35. 7.4 Standard candles & H0 141
  36. 7.5 Standard candles & acceleration 144
  37. Chapter 8 Dark Matter 155
  38. 8.1 Visible matter 156
  39. 8.2 Dark matter in galaxies 159
  40. 8.3 Dark matter in clusters 164
  41. 8.4 Gravitational lensing 170
  42. 8.5 What’s the matter? 175
  43. Chapter 9 The Cosmic Microwave Background 179
  44. 9.1 Observing the CMB 180
  45. 9.2 Recombination and decoupling 185
  46. 9.3 The physics of recombination 189
  47. 9.4 Temperature fluctuations 196
  48. 9.5 What causes the fluctuations? 201
  49. Chapter 10 Nucleosynthesis & the Early Universe 208
  50. 10.1 Nuclear physics and cosmology 209
  51. 10.2 Neutrons and protons 213
  52. 10.3 Deuterium synthesis 218
  53. 10.4 Beyond deuterium 222
  54. 10.5 Baryon – antibaryon asymmetry 228
  55. Chapter 11 Inflation & the Very Early Universe 233
  56. 11.1 The flatness problem 234
  57. 11.2 The horizon problem 236
  58. 11.3 The monopole problem 238
  59. 11.4 The inflation solution 242
  60. 11.5 The physics of inflation 247
  61. Chapter 12 The Formation of Structure 255
  62. 12.1 Gravitational instability 258
  63. 12.2 The Jeans length 261
  64. 12.3 Instability in an expanding universe 266
  65. 12.4 The power spectrum 272
  66. 12.5 Hot versus cold 276
  67. Chapter 13 Epilogue 284
  68. Chapter 14 Annotated Bibliography 286
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