Abstract

Topology-changing transitions between vacua of different effective dimensionality are studied in the context of a 6-dimensional Einstein-Maxwell theory. The landscape of this theory includes a 6d6d de Sitter vacuum (dS6dS_6), a number of dS4×S2dS_4 \times S_2 and AdS4×S2AdS_4 \times S_2 vacua, and a number of AdS2×S4AdS_2 \times S_4 vacua. We find that compactification transitions dS6→AdS2×S4dS_6 \to AdS_2 \times S_4 occur through the nucleation of electrically charged black hole pairs, and transitions from dS6dS_6 to dS4×S2dS_4 \times S_2 and AdS4×S2AdS_4 \times S_2 occur through the nucleation of magnetically charged spherical black branes. We identify the appropriate instantons and describe the spacetime structure resulting from brane nucleation.

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