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The Early Universe | | Andrew R Liddle
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10 Dec 1996 | | Subject: | astro-ph hep-ph | | Abstract: | An introductory account is given of the modern understanding of the physics of the early Universe. Particular emphasis is placed on the paradigm of cosmological inflation, which postulates a period of accelerated expansion during the Universe’s earliest stages. Inflation provides a possible origin for structure in the Universe, such as microwave background anisotropies, galaxies and galaxy clusters; these observed structures can therefore be used to test models of inflation. A brief account is given of other early Universe topics, namely baryogenesis, topological defects, dark matter candidates and primordial black holes. | | Source: | arXiv, astro-ph/9612093 | | Services: | Forum | Review | PDF | Favorites | |
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