Prologue |
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1 | (169) |
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1 Building blocks of the cosmos |
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5 | (21) |
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1.1 Cosmological principles |
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5 | (4) |
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9 | (2) |
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1.3 Building blocks of the universe |
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11 | (11) |
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22 | (2) |
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1.5 The darkness of the night sky |
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24 | (2) |
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2 Expansion of the universe |
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26 | (21) |
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26 | (2) |
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2.2 The distance to the nearest stars |
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28 | (3) |
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2.3 The redshift-distance relation |
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31 | (2) |
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2.4 Unlocking the extragalactic distance scale |
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33 | (6) |
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2.5 What is the Hubble constant? |
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39 | (2) |
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2.6 Steady state cosmology |
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41 | (6) |
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3 Cosmic microwave background |
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47 | (12) |
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48 | (2) |
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50 | (2) |
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3.3 The isotropy of the cosmic microwave background |
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52 | (1) |
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3.4 The epoch of thermalisation |
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53 | (1) |
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3.5 The last scattering epoch |
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54 | (2) |
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56 | (3) |
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4 The first 10-43 second of the universe |
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59 | (26) |
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59 | (2) |
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61 | (3) |
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64 | (2) |
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66 | (1) |
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67 | (2) |
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69 | (1) |
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70 | (2) |
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72 | (1) |
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73 | (2) |
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4.10 Symmetry breaking and inflation |
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75 | (5) |
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4.11 Why is the universe so uniform? |
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80 | (2) |
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4.12 The flatness problem |
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82 | (1) |
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82 | (3) |
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5 Genesis of baryons and helium |
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85 | (12) |
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5.1 The matter-antimatter puzzle |
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86 | (3) |
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5.2 Generation of the baryon number |
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89 | (2) |
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5.3 Proton decay experiments |
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91 | (1) |
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5.4 The weak interaction freeze-out |
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92 | (1) |
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5.5 Primordial nucleosynthesis |
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93 | (2) |
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95 | (2) |
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97 | (16) |
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6.1 The density of the universe |
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97 | (5) |
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6.2 Curved space and general relativity |
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102 | (4) |
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106 | (4) |
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6.4 Impediments to the tests |
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110 | (3) |
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113 | (19) |
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7.1 Local indicators of dark matter |
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114 | (1) |
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7.2 Luminous regions of galaxies |
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115 | (2) |
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117 | (1) |
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7.4 Galaxy groups, clusters, and superclusters |
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118 | (1) |
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7.5 Large-scale flows and dark matter |
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118 | (2) |
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7.6 A universe at the critical density? |
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120 | (2) |
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7.7 Deuterium and the baryon density |
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122 | (2) |
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124 | (1) |
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7.9 WIMPs: exotic particle dark matter |
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125 | (4) |
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129 | (3) |
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132 | (26) |
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8.1 Life after the main sequence: white dwarfs |
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133 | (2) |
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8.2 The formation of a neutron star |
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135 | (2) |
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8.3 Observing neutron stars |
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137 | (2) |
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139 | (1) |
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140 | (12) |
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152 | (2) |
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8.7 MACHOS: astrophysical dark matter? |
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154 | (4) |
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158 | (12) |
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9.1 Recombination and decoupling |
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158 | (1) |
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9.2 The search for the intergalactic medium |
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159 | (2) |
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161 | (3) |
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164 | (1) |
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165 | (5) |
10 Origin of structure |
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170 | (23) |
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170 | (2) |
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10.2 Cold dark matter and bottom-up formation |
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172 | (4) |
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10.3 A radical view: from cosmic pancakes and filaments to galaxies |
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176 | (5) |
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10.4 Origin of the fluctuations |
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181 | (3) |
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10.5 A low density universe? |
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184 | (3) |
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10.6 Detection of temperature fluctuations |
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187 | (3) |
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10.7 The whispers of creation |
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190 | (3) |
11 Large-scale structure |
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193 | (26) |
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11.1 The greatest structures: galaxy clusters |
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193 | (3) |
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196 | (2) |
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11.3 Large-scale flows revisited |
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198 | (4) |
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11.4 The challenges of cold dark matter |
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202 | (2) |
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11.5 Dark energy and cold dark matter |
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204 | (4) |
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11.6 Problems with cold dark matter |
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208 | (3) |
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11.7 Hot and cold, or merely warm |
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211 | (1) |
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212 | (7) |
12 Galaxy formation |
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219 | (18) |
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12.1 Formation of the stars |
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219 | (4) |
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223 | (2) |
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12.3 Supernova remnants and enrichment |
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225 | (2) |
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227 | (3) |
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230 | (2) |
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12.6 Formation of elliptical and spiral galaxies |
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232 | (1) |
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233 | (2) |
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12.8 The cosmological hierarchy |
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235 | (2) |
13 What lies ahead |
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237 | (5) |
Index |
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242 | |