Cosmological Perturbation Theory and Structure Formation

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dc.creatorBertschinger, Edmund
dc.date2000-12-31
dc.date.accessioned2026-07-07T01:57:14Z
dc.date.available2026-07-07T01:57:14Z
dc.descriptionThese lecture notes discuss several topics in the physics of cosmic structure formation starting from the evolution of small-amplitude fluctuations in the radiation-dominated era. The topics include relativistic cosmological perturbation theory with the scalar-vector-tensor decomposition, the evolution of adiabatic and isentropic initial fluctuations, microwave background anisotropy, spatial and angular power spectra, the cold dark matter linear transfer function, Press-Schechter theory, and a brief introduction to numerical simulation methods.
dc.description25 pages, 2 eps figures. To appear in Proceedings of Cosmology 2000, Lisbon, July 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0101009
dc.identifierhttp://arxiv.org/abs/astro-ph/0101009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2304
dc.subjectAstrophysics
dc.titleCosmological Perturbation Theory and Structure Formation
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