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Inflation and quintessence in brane cosmology

We examine both quintessence and inflation within the brane-world picture, wherein the world is (4+d)-dimensional, and all standard model fields are trapped on the surface of a p-dimensional brane. We examine the situation where the inter-brane potential is dominated by the exchange of either a massless or a massive mode, for the case where the extra dimensions have the topology of a torus. In doing so, we find that neither potential is flat enough to allow for sufficient inflation. We will also propose a brane-based model where there are two large extra dimensions. In deriving the low-energy theory on the brane, we show that this model can have applications to both quintessence as well as to inflation.

Identiferoai:union.ndltd.org:LACETR/oai:collectionscanada.gc.ca:QMM.81342
Date January 2004
CreatorsHoover, Douglas A. (Douglas Allan), 1979-
PublisherMcGill University
Source SetsLibrary and Archives Canada ETDs Repository / Centre d'archives des thèses électroniques de Bibliothèque et Archives Canada
LanguageEnglish
Detected LanguageEnglish
TypeElectronic Thesis or Dissertation
Formatapplication/pdf
CoverageMaster of Science (Department of Physics.)
RightsAll items in eScholarship@McGill are protected by copyright with all rights reserved unless otherwise indicated.
Relationalephsysno: 002173359, proquestno: AAIMR06405, Theses scanned by UMI/ProQuest.

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