6-dimensional brane world model
Author(s) -
Panagiota Kanti,
R. Madden,
Keith A. Olive
Publication year - 2001
Publication title -
physical review. d. particles, fields, gravitation, and cosmology/physical review. d. particles and fields
Language(s) - English
Resource type - Journals
eISSN - 1089-4918
pISSN - 0556-2821
DOI - 10.1103/physrevd.64.044021
Subject(s) - brane , physics , spacetime , de sitter universe , brane cosmology , anti de sitter space , cosmological constant , curvature , constant curvature , mathematical physics , classical mechanics , radius , constant (computer programming) , theoretical physics , geometry , quantum mechanics , mathematics , universe , computer security , computer science , programming language
We consider a 6D space-time which is periodic in one of the extra dimensionsand compact in the other. The periodic direction is defined by two 4-braneboundaries. Both static and non-static exact solutions, in which the internalspacetime has constant radius of curvature, are derived. In the case of staticsolutions, the brane tensions must be tuned as in the 5D Randall-Sundrum model,however, no additional fine-tuning is necessary between the brane tensions andthe bulk cosmological constant. By further relaxing the sole fine-tuning of themodel, we derive non-static solutions, describing de Sitter or Anti de Sitter4D spacetimes, that allow for the fixing of the inter-brane distance and theaccommodation of pairs of positive-negative and positive-positive tensionbranes. Finally, we consider the stability of the radion field in theseconfigurations by employing small, time-dependent perturbations around thebackground solutions. In analogy with results drawn in 5 dimensions, thesolutions describing a de Sitter 4D spacetime turn out to be unstable whilethose describing an Anti de Sitter geometry are shown to be stable.Comment: 22 pages, LaTeX file, no figure
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