An Introduction to Cosmology
The third edition of this successful textbook is fully updated and includes important recent developments in cosmology. It begins with an introduction to cosmology and general relativity, and goes on to cover the mathematical models of standard cosmology. The physical aspects of cosmology, including primordial nucleosynthesis, the astroparticle physics of inflation, and the current ideas on structure formation are discussed. Alternative models of cosmology are reviewed, including the model of Quasi-Steady State Cosmology, which has recently been proposed as an alternative to Big Bang Cosmology.
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abundance antimatter approximation arcseconds assumed baryons big-bang black hole Brans-Dicke Brans-Dicke theory calculation Chapter cluster components consider coordinates cosmic cosmological constant curvature curve dark matter denote derived described deuterium discussed distance distribution early universe effect Einstein electromagnetic electrons emitted energy density energy tensor estimate Euclidean example expansion expressed field equations Figure fluctuations Friedmann models galactic galaxies geodesic geometry given gravitational horizon Hubble constant Hubble's Hubble's law inertial inflation inflationary interactions intergalactic large-scale structure leptons line element linear luminosity magnitude mass measured microwave background neutrinos Newtonian nucleosynthesis number density observations parameter particle horizon photon physics Planck particles primordial primordial nucleosynthesis QSSC quasars radiation radio sources radius range ratio redshift region relation relativistic relativity result Robertson-Walker scalar Show solution space spacetime spectrum sphere stars steady-state supernovae surface temperature theory transformation typical vector velocity wave equation wavelength world lines