2021
DOI: 10.48550/arxiv.2110.08276
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Bubble instability of mIIA on $\mathrm{AdS}_4\times S^6$

Abstract: We consider compactifications of massive IIA supergravity on a six-sphere. This setup is known to give rise to non-supersymmetric AdS 4 vacua preserving SO(7) as well as G 2 residual symmetry. Both solutions have a round S 6 metric and are supported by the Romans' mass and internal F 6 flux. While the SO(7) invariant vacuum is known to be perturbatively unstable, the G 2 invariant one has been found to have a fully stable Kaluza-Klein spectrum. Moreover, it has been shown to be protected against brane-jet inst… Show more

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Cited by 5 publications
(10 citation statements)
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“…Any possible decay of our vacua must therefore be necessarily through a non-pertubative channel, such as brane-jet instabilities [38,39] or bubble nucleations (see e.g. [40][41][42][43]). These possible decay mechanisms will have to deal with the presence of the N = (0, 4) vacua continuously connected to the non-supersymmetric family (4.23).…”
Section: Further Discussionmentioning
confidence: 99%
“…Any possible decay of our vacua must therefore be necessarily through a non-pertubative channel, such as brane-jet instabilities [38,39] or bubble nucleations (see e.g. [40][41][42][43]). These possible decay mechanisms will have to deal with the presence of the N = (0, 4) vacua continuously connected to the non-supersymmetric family (4.23).…”
Section: Further Discussionmentioning
confidence: 99%
“…Still, our vacua could decay semi-classically via more complicated bubbles of nothing containing defects, e.g. a D3-brane in S 5 similar to [38,39] or an O7-plane in S 1 [40]. However, because the volume form of the compactification is independent of the χ i deformations, our non-supersymmetric AdS 4 vacua are likely to be stable against the instanton decay constructed in [39], which is delocalised on the compactification space.…”
mentioning
confidence: 96%
“…a D3-brane in S 5 similar to [38,39] or an O7-plane in S 1 [40]. However, because the volume form of the compactification is independent of the χ i deformations, our non-supersymmetric AdS 4 vacua are likely to be stable against the instanton decay constructed in [39], which is delocalised on the compactification space. On the other hand, constructing the localised instanton solutions is extremely technically challenging.…”
mentioning
confidence: 97%
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“…Recently, in[27] so-called dilaton bubble solution was explicitly constructed for the G 2 -symmetric vacuum which is one of the seven AdS 4 vacua of massive type IIA supergravity known to be BF and brane-jet stable.…”
mentioning
confidence: 99%