Per Kraus JHEP12(1999)011 doi:10.1088/1126-6708/1999/12/011
Per Kraus1
Show affiliationsWe 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.
E-print Number: hep-th/9910149
Cited: by |
Refers: to
11.27.+d Extended classical solutions; cosmic strings, domain walls, texture
04.70.-s Physics of black holes
04.50.-h Higher-dimensional gravity and other theories of gravity
Issue 12 ( 1 December 1999)
Received 7 December 1999, accepted for publication 11 December 1999
Published 17 December 1999
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