Tuesday, July 5, 2011

Introduction to modern cosmology 2ed wiley Ebook download


Introduction to modern cosmology 2ed wiley

Book information
  • Book title                    : Introduction to modern cosmology 2ed
  • Author                         : Andrew Liddle
File information
  • File size                     :12.43 Mb
  • File format                : PDF File









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Textbook title page

Preface xi

Constants, conversion factors and symbols xiv

1 A (Very) Brief History of Cosmological Ideas 1

2 Observational Overview 3
  • 2.1 In visible light 3
  • 2.2 In other wavebands 7
  • 2.3 Homogeneity and isotropy 8
  • 2.4 The expansion of the Universe 9
  • 2.5 Particles in the Universe 11
  • 2.5.1 What particles are there? 11
  • 2.5.2 Thermal distributions and the black-body spectrum 13
3 Newtonian Gravity 17
  • 3.1 The Friedmann equation 18
  • 3.2 On the meaning of the expansion 21
  • 3.3 Things that go faster than light 21
  • 3.4 The fluid equation 22
  • 3.5 The acceleration equation 23
  • 3.6 On mass, energy and vanishing factors of c2 24
4 The Geometry of the Universe 25
  • 4.1 Flat geometry 25
  • 4.2 Spherical geometry 26
  • 4.3 Hyperbolic geometry 28
  • 4.4 Infinite and observable Universes 29
  • 4.5 Where did the Big Bang happen? 29
  • 4.6 Three values of k 30
5 Simple Cosmological Models 33
  • 5.1 Hubble'slaw 33
  • 5.2 Expansion and redshift 34
  • 5.3 Solving the equations 355.3.1 Matter 36
  • 5.3.2 Radiation 37
  • 5.3.3 Mixtures 38
  • 5.4 Particle number densities 39
  • 5.5 Evolution including curvature 40
6 Observational Parameters 45
  • 6.1 The expansion rate HO 45
  • 6.2 The density parameter Q0 47
  • 6.3 The deceleration parameter QQ 48
7 The Cosmological Constant 51
  • 7.1 Introducing A 51
  • 7.2 Fluid description of A 52
  • 7.3 Cosmological models with A 53
8 The Age of the Universe 57

9 The Density of the Universe and Dark Matter 63
  • 9.1 Weighing the Universe 63
  • 9.1.1 Counting stars 63
  • 9.1.2 Nucleosynthesis foreshadowed 64
  • 9.1.3 Galaxy rotation curves 64
  • 9.1.4 Galaxy cluster composition 66
  • 9.1.5 Bulk motions in the Universe 67
  • 9.1.6 The formation of structure 68
  • 9.1.7 The geometry of the Universe and the brightness of supernovae . 68
  • 9.1.8 Overview 69
  • 9.2 What might the dark matter be? 69
  • 9.3 Dark matter searches 72
10 The Cosmic Microwave Background 75
  • 10.1 Properties of the microwave background 75
  • 10.2 The photon to baryon ratio 77
  • 10.3 The origin of the microwave background 78
  • 10.4 The origin of the microwave background (advanced) 81
11 The Early Universe 85
12 Nucleosynthesis: The Origin of the Light Elements 91
  • 12.1 Hydrogen and Helium 91
  • 12.2 Comparing with observations 94
  • 12.3 Contrasting decoupling and nucleosynthesis 96
13 The Inflationary Universe 99
  • 13.1 Problems with the Hot Big Bang 99
  • 13.1.1 The flatness problem 99
  • 13.1.2 The horizon problem 101
  • 13.1.3 Relic particle abundances 102
  • 13.2 Inflationary expansion 103
  • 13.3 Solving the Big Bang problems 104
  • 13.3.1 The flatness problem 104
  • 13.3.2 The horizon problem 105
  • 13.3.3 Relic particle abundances 106
  • 13.4 How much inflation? 106
  • 13.5 Inflation and particle physics 107
14 The Initial Singularity 111

15 Overview: The Standard Cosmological Model 115

Advanced Topic 1 General Relativistic Cosmology 119
  1. 1.1 The metric of space-time 119
  2. 1.2 The Einstein equations 120
  3. 1.3 Aside: Topology of the Universe 122
Advanced Topic 2 Classic Cosmology: Distances and Luminosities 125
  • 2.1 Light propagation and redshift 125
  • 2.2 The observable Universe 128
  • 2.3 Luminosity distance 128
  • 2.4 Angular diameter distance 132
  • 2.5 Source counts 134
Advanced Topic 3 Neutrino Cosmology 137
  • 3.1 The massless case 137
  • 3.2 Massive neutrinos 139
  • 3.2.1 Light neutrinos 139
  • 3.2.2 Heavy neutrinos 140
  • 3.3 Neutrinos and structure formation 140
Advanced Topic 4 Baryogenesis 143

Advanced Topic 5 Structures in the Universe 147
  • 5.1 The observed structures 147
  • 5.2 Gravitational instability 149
  • 5.3 The clustering of galaxies 150
  • 5.4 Cosmic microwave background anisotropies 152
  • 5.4.1 Statistical description of anisotropies 152
  • 5.4.2 Computing the Ct 154
  • 5.4.3 Microwave background observations 155
  • 5.4.4 Spatial geometry 1565.5 The origin of structure 157
Bibliography 161
Numerical answers and hints to problems 163
Index 167