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Modern Cosmology and Structure Formation

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arxiv astro-ph/9411049 v1 pith:EHLDVVWE submitted 1994-11-11 astro-ph hep-ph

classification astro-phhep-ph
keywords structurecosmologyformationmodernobservationalsummarytheoryuniverse
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An introduction to modern cosmology is given, focusing on theories for the origin of structure in the Universe. After a brief review of the theory of growth of cosmological perturbations and a summary of some important observational results, most of the article is devoted to discussions of the inflationary Universe scenario and of topological defect models of structure formation. The final chapter is a summary of the theory of cosmic microwave background temperature fluctuations and of the current observational status.

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    In single-field inflation, gravitational interactions mixing short-wavelength tensor and scalar modes decohere long-wavelength scalar perturbations at a rate proportional to (H/M_p)^2, with no suppression by the slow-...

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