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The asymptotic dS Swampland Conjecture - a simplified derivation and a potential loophole

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

Recently, arguments for a refined de Sitter conjecture were put forward in arXiv:1810.05506. Using the large distance conjecture of arXiv:hep-th/0605264, the authors provide evidence for this dS conjecture in asymptotic regimes of field space, where the parametric control of string theory becomes arbitrarily good. Their main tool is Bousso's covariant entropy bound arXiv:hep-th/9905177. Here, we present a simpler way to reach a similar conclusion. The argument is based on the fact that the cutoff of an effective theory with gravity decreases as the number of species grows. We then discuss a loophole in this argument and its possible counterpart in the assumptions underlying the entropy-based derivation. The idea is to consider potentials which, while they remain below an exponentially falling bound, have small oscillations leading locally to relatively flat regions or even to an infinite series of dS minima.

citation-role summary

background 2

citation-polarity summary

fields

hep-th 2

years

2026 1 2025 1

verdicts

UNVERDICTED 2

roles

background 2

polarities

background 1 support 1

representative citing papers

Dark energy from string theory: an introductory review

hep-th · 2026-03-26 · unverdicted · novelty 2.0

String theory imposes constraints on dark energy but permits various construction attempts for de Sitter vacua and single-field exponential quintessence models despite obstructions.

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Showing 2 of 2 citing papers.

  • An M-theory dS maximum from Casimir energies on Riemann-flat manifolds hep-th · 2025-07-02 · unverdicted · none · ref 154 · internal anchor

    Explicit scale-separated dS5 maximum in M-theory on a 6D Riemann-flat manifold with vacuum energy 10^{-8} in Planck units, obtained via Casimir energies and fluxes.

  • Dark energy from string theory: an introductory review hep-th · 2026-03-26 · unverdicted · none · ref 166 · internal anchor

    String theory imposes constraints on dark energy but permits various construction attempts for de Sitter vacua and single-field exponential quintessence models despite obstructions.