Modern cosmology /
Scott Dodelson.
- San Diego, California : Academic Press, 2003.
- xiii, 440 pages. : illustrations ; 26 cm.
Includes bibliographical references (p. 426-434) and index.
Modern Cosmology begins with an introduction to the smooth, homogeneous universe described by a Friedman-Robertson-Walker metric, including careful treatments of dark energy, big bang nucleosynthesis, recombination, and dark matter. From this starting point, the reader is introduced to perturbations about an FRW universe: their evolution with the Einstein-Boltzmann equations, their generation by primordial inflation, and their observational consequences. These consequences include the anisotropy spectrum of the cosmic microwave background (CMB) featuring acoustic peaks and polarization