Transplanckian Censorship and the Local Swampland Distance Conjecture

Abstract

The swampland distance conjecture (SDC) addresses the ability of effective field theory to describe distant points in moduli space. It is natural to ask whether there is a local version of the SDC: is it possible to construct local excitations in an EFT that sample extreme regions of moduli space? In many cases such excitations exhibit horizons or instabilities, suggesting that there are bounds on the size and structure of field excitations that can be achieved in EFT. Static bubbles in ordinary Kaluza-Klein theory provide a simple class of examples: the KK radius goes to zero on a smooth surface, locally probing an infinite distance point, and the bubbles are classically unstable against radial perturbations. However, it is also possible to stabilize KK bubbles at the classical level by adding flux. We study the impact of imposing the Weak Gravity Conjecture (WGC) on these solutions, finding that a rapid pair production instability arises in the presence of charged matter with $q/m\gtrsim 1$. We also analyze 4d electrically charged dilatonic black holes. Small curvature at the horizon imposes a bound $\log (M_{BH})\gtrsim |\Delta \varphi |$, independent of the WGC, and the bound can be strengthened if the particle satisfying the WGC is sufficiently light. We conjecture that quantum gravity in asymptotically flat space requires a general bound on large localized moduli space excursions of the form $|\Delta \varphi |\lesssim |\log (R\Lambda )|$, where $R$ is the size of the minimal region enclosing the excitation and ${\Lambda }^{-1}$ is the short-distance cutoff on local EFT. The bound is qualitatively saturated by the dilatonic black holes and Kaluza-Klein monopoles.

arXiv comment14 pages

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Cited by in corpus (17)

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• Asymptotic Flux Compactifications and the Swampland
• Swampland Conjectures for Strings and Membranes
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• Nothing really matters
• Strengthening the TCC Bound on Inflationary Cosmology
• 4d strings at strong coupling
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• The UV Fate of Anomalous $U(1)$s and the Swampland
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• Cosmic Censorship of Trans-Planckian Field Ranges in Gravitational Collapse