Fundamentals of CosmologySpringer Science & Business Media, 2001 - 302 стор. The book is aimed at physics students and professional physicists who wish to understand the basics of cosmology and general relativity as well as the most recent cosmological observations and models. It presents a self-contained introduction to general relativity that is based on the homogeneity and isotropy of the local universe. The simplicity of this space allows general relativity to be introduced in a very simple manner while laying the foundation for the treatment of more complicated problems. The latest cosmological observations and theories are discussed. Emphasis is placed on estimations of the densities of matter and of vacuum energy, and on investigations of the primordial density fluctuations and the nature of dark matter. |
Зміст
I | 1 |
II | 3 |
III | 10 |
IV | 11 |
V | 12 |
VI | 13 |
VII | 15 |
VIII | 17 |
XLIX | 151 |
L | 153 |
LI | 156 |
LII | 162 |
LIII | 168 |
LIV | 169 |
LV | 172 |
LVI | 174 |
IX | 19 |
X | 21 |
XI | 23 |
XII | 28 |
XIII | 30 |
XIV | 32 |
XV | 34 |
XVI | 38 |
XVII | 39 |
XIX | 51 |
XX | 54 |
XXI | 57 |
XXII | 59 |
XXIII | 62 |
XXV | 67 |
XXVI | 70 |
XXVII | 74 |
XXVIII | 85 |
XXIX | 88 |
XXX | 93 |
XXXI | 96 |
XXXII | 99 |
XXXIII | 103 |
XXXIV | 106 |
XXXV | 108 |
XXXVI | 111 |
XXXVII | 118 |
XXXVIII | 125 |
XXXIX | 126 |
XL | 129 |
XLI | 134 |
XLII | 136 |
XLIII | 137 |
XLIV | 139 |
XLV | 142 |
XLVI | 143 |
XLVII | 144 |
XLVIII | 148 |
LVII | 179 |
LVIII | 182 |
LIX | 186 |
LX | 191 |
LXI | 196 |
LXII | 198 |
LXIII | 206 |
LXIV | 209 |
LXV | 210 |
LXVI | 212 |
LXVII | 214 |
LXVIII | 221 |
LXIX | 226 |
LXX | 227 |
LXXI | 228 |
LXXII | 232 |
LXXIII | 234 |
LXXIV | 240 |
LXXV | 244 |
LXXVI | 247 |
LXXVII | 252 |
LXXVIII | 254 |
LXXIX | 256 |
LXXX | 259 |
LXXXI | 263 |
LXXXII | 264 |
LXXXIII | 265 |
LXXXIV | 268 |
LXXXV | 269 |
LXXXVI | 275 |
LXXXVII | 277 |
LXXXVIII | 279 |
LXXXIX | 283 |
XC | 285 |
XCI | 288 |
| 293 | |
| 299 | |
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Загальні терміни та фрази
absorption annihilation apparent magnitude Astrophys baryons Boltzmann equation calculated CBR anisotropies Cepheids Chap clock comoving coordinates constant cosmological cross-section dark matter deceleration density contrast density fluctuations determined dr² early universe Einstein electrons energy density estimated Exercise expansion rate flux Friedmann equation function galactic galactic halo galaxy clusters geodesic gives gravitational halo homogeneous universe horizon Hubble distance Hubble radius Hubble's law hydrogen implies inflation inflationary inflationary epoch inhomogeneities interactions Lorentz Lorentzian luminosity magnitude mass matter epoch measured neutrinos Newtonian nucleosynthesis number density objects observed over-dense region parameters particles peculiar velocities photons Phys potential primordial quasars radiation epoch ratio reactions recombination redshift relative relativistic Robertson-Walker metric scale factor Sect shown in Fig sin² spatial spectrum stars stellar structure formation supernovae t₁ temperature tensor thermal equilibrium trajectories trec vacuum energy wavelength wimps ΩΛ ΩΜ ΩΤ მე
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