Bubbles of Nothing in Flux Compactifications
arXiv:1002.4408 · doi:10.1103/PhysRevD.82.086015
Abstract
We construct a simple AdS_4 x S^1 flux compactification stabilized by a complex scalar field winding the extra dimension and demonstrate an instability via nucleation of a bubble of nothing. This occurs when the Kaluza -- Klein dimension degenerates to a point, defining the bubble surface. Because the extra dimension is stabilized by a flux, the bubble surface must be charged, in this case under the axionic part of the complex scalar. This smooth geometry can be seen as a de Sitter topological defect with asymptotic behavior identical to the pure compactification. We discuss how a similar construction can be implemented in more general Freund -- Rubin compactifications.
16 pages, 5 figures References added
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- de Sitter Decays to Infinity
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- The decay of hot KK space
- Gravity waves from cosmic bubble collisions
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