Stability of the Anisotropic Brane Cosmology

Details Stability of the Anisotropic Brane Cosmology Stability of the Anisotropic Brane Cosmology

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002asph.conf..165k&link_type=abstract

ASTROPARTICLE PHYSICS . Proceedings of the First NCTS Workshop . Held 6-8 December 2001 in Kenting, Taiwan . Edited by Husain At

Physics

Scientific paper

The stability of the Bianchi type I anisotropic brane cosmology will be analyzed in this talk. Analysis is presented for the model with a perfect fluid. It is shown that the anisotropic expansion is smeared out dynamically in the large time limit. It is shown that the initial state is highly isotropic for the brane universe except for a very particular case. Moreover, it is also shown that the Bianchi type I anisotropic cosmology is stable against any anisotropic perturbation for the brane model in the large time limit. This talk is based on a paper in collaboration with Chiang-Mei Chen 1

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