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Isotropization in Brane Gas Cosmology

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arxiv hep-th/0207168 v3 pith:IGHNXWWB submitted 2002-07-18 hep-th astro-phgr-qchep-ph

Isotropization in Brane Gas Cosmology

classification hep-th astro-phgr-qchep-ph
keywords cosmologydimensionsspatialbraneisotropizationlargethreeallows
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Brane Gas Cosmology (BGC) is an approach to unifying string theory and cosmology in which matter is described by a gas of strings and branes in a dilaton gravity background. The Universe is assumed to start out with all spatial dimensions compact and small. It has previously been shown that in this context, in the approximation of neglecting inhomogeneities and anisotropies, there is a dynamical mechanism which allows only three spatial dimensions to become large. However, previous studies do not lead to any conclusions concerning the isotropy or anisotropy of these three large spatial dimensions. Here, we generalize the equations of BGC to the anisotropic case, and find that isotropization is a natural consequence of the dynamics.

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