Abstract
We construct instanton solutions describing the decay of flux
compactifications of a $6d$ gauge theory by generalizing the Kaluza-Klein
bubble of nothing. The surface of the bubble is described by a smooth
magnetically charged solitonic brane whose asymptotic flux is precisely that
responsible for stabilizing the 4d compactification. We describe several
instances of bubble geometries for the various vacua occurring in a $6d$
Einstein-Maxwell theory namely, AdS_4 x S^2, R^1,3 x S^2, and dS_4 x S^2.
Unlike conventional solutions, the bubbles of nothing introduced here occur
where a two-sphere compactification manifold homogeneously degenerates.
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