WMAPping the Inflationary Universe

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dc.creatorRangarajan, Raghavan
dc.date2007-06-28
dc.date.accessioned2026-07-07T08:12:51Z
dc.date.available2026-07-07T08:12:51Z
dc.descriptionAn epoch of accelerated expansion, or inflation, in the early universe solves several cosmological problems. While there are many models of inflation only recently has it become possible to discriminate between some of the models using observations of the cosmic microwave background radiation and large-scale structure. In this talk, we discuss inflation and its observational consequences, and then the status of current cosmological observations and their implications for different models of inflation.
dc.description6 pages; Invited talk at the 17th DAE-BRNS High Energy Physics Symposium at the Indian Institute of Technology, Kharagpur, December 11-15, 2006
dc.identifierhttps://arxiv.org/abs/0706.4166
dc.identifierhttp://arxiv.org/abs/0706.4166
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/132599
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleWMAPping the Inflationary Universe
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