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Plumbing the wormholes of string theory flux compactifications

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arxiv 2404.00803 v1 pith:JRYOH2L5 submitted 2024-03-31 hep-th

classification hep-th
keywords wormholesfluxfluxesnon-perturbativelystringtheoryadditionalbackgrounds
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Thus far, the known wormholes in string theory connecting disjoint boundaries represented by finite volume quotients of hyperbolic spaces leak: they are non-perturbatively unstable towards brane-anti-brane nucleation in the flux backgrounds that support these wormholes. Turning on additional fluxes suppressed this instability, but would not completely eliminate it. We present the first example of a non-perturbatively stable wormhole in type IIB supergravity on a warped squashed conifold with fluxes.

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  1. Fluxification and scalarization of the conifold black holes

    hep-th 2024-11 conditional novelty 6.0 of 10

    Two dimension-3 chiral operators of the Klebanov-Witten theory condense at the same critical chemical potential, producing flux-hair and scalar-hair black holes with ensemble-dependent phase dominance.

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