The Beginning and Evolution of the Universe
arXiv:0706.1565 · doi:10.1086/529495
Abstract
We review the current standard model for the evolution of the Universe from an early inflationary epoch to the complex hierarchy of structure seen today. We summarize and provide key references for the following topics: observations of the expanding Universe; the hot early Universe and nucleosynthesis; theory and observations of the cosmic microwave background; Big Bang cosmology; inflation; dark matter and dark energy; theory of structure formation; the cold dark matter model; galaxy formation; cosmological simulations; observations of galaxies, clusters, and quasars; statistical measures of large-scale structure; and measurement of cosmological parameters. We conclude with discussion of some open questions in cosmology. This review is designed to provide a graduate student or other new worker in the field an introduction to the cosmological literature.
69 pages. Invited review article for Publications of the Astronomical Society of the Pacific. Supplementary references, tables, and more concise PDF file at http://www.physics.drexel.edu/universe
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Cited by in corpus (6)
- Model-Independent Distance Measurements from Gamma-Ray Bursts and Constraints on Dark Energy
- CMB Temperature Anisotropy from Broken Spatial Isotropy due to an Homogeneous Cosmological Magnetic Field
- Growth Index of DGP Model and Current Growth Rate Data
- Constraints on Kinematic Model from Recent Cosmic Observations: SN Ia, BAO and Observational Hubble Data
- Cosmological Studies with Radio Galaxies and Supernovae
- Constraints on dark energy from baryon acoustic peak and galaxy cluster gas mass measurements