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Analytic bounds on late-time axion-scalar cosmologies,

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

3 Pith papers citing it

citation-role summary

background 2

citation-polarity summary

years

2026 2 2025 1

verdicts

UNVERDICTED 3

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background 2

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background 2

representative citing papers

Alice in Warpland: KK modes, Warped Compactifications and the Swampland

hep-th · 2026-03-11 · unverdicted · novelty 7.0

In codimension-one warped compactifications with exponential potentials, the KK mass decay rate λ_KK is reduced by warping but still satisfies the Sharpened Distance Conjecture precisely when the higher-dimensional potential obeys the Strong de Sitter condition.

Bounding axion dark energy

astro-ph.CO · 2026-04-10 · unverdicted · novelty 6.0

An analytic bound on axion parameters in thawing quintessence is derived independently of initial conditions and used with cosmological observations plus quantum gravity constraints to exclude large regions of axion dark energy parameter space.

citing papers explorer

Showing 3 of 3 citing papers.

  • Alice in Warpland: KK modes, Warped Compactifications and the Swampland hep-th · 2026-03-11 · unverdicted · none · ref 91

    In codimension-one warped compactifications with exponential potentials, the KK mass decay rate λ_KK is reduced by warping but still satisfies the Sharpened Distance Conjecture precisely when the higher-dimensional potential obeys the Strong de Sitter condition.

  • Extending the Dynamical Systems Toolkit: Coupled Fields in Multiscalar Dark Energy hep-th · 2025-09-02 · unverdicted · none · ref 30

    New dynamical systems variables for coupled axion-saxion fields yield a general non-geodesicity expression at fixed points and identify genuinely non-geodesic attractors under exponential couplings.

  • Bounding axion dark energy astro-ph.CO · 2026-04-10 · unverdicted · none · ref 77

    An analytic bound on axion parameters in thawing quintessence is derived independently of initial conditions and used with cosmological observations plus quantum gravity constraints to exclude large regions of axion dark energy parameter space.