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Dynamics of Anti-de Sitter Domain Walls

Per Kraus

hep-tharXiv:hep-th/9910149

Abstract

We study solutions corresponding to moving domain walls in the Randall-Sundrum universe. The bulk geometry is given by patching together black hole solutions in AdS5, and the motion of the wall is determined from the junction equations. Observers on the wall interpret the motion as cosmological expansion or contraction. We describe the possible wall trajectories, and examine the consequences for localized gravity on the wall.

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