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A distance conjecture beyond moduli?

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arxiv 2407.03715 v3 pith:44NRJSW5 submitted 2024-07-04 hep-th

A distance conjecture beyond moduli?

classification hep-th
keywords distancefieldconjecturemodulipotentialtheoriesasymptoticaway
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The distance conjecture states that for theories with moduli coupled to gravity a tower of states becomes light exponentially in the geodesic distance in moduli space. This specifies how effective field theories break down for large field values. However, phenomenological field theories have no moduli, but a scalar potential that deforms dynamical trajectories away from geodesic curves. In this note we speculate on how one should generalise the distance conjecture, in asymptotic field regimes, to include a scalar potential. We test the generalised distance conjecture in a few cases, demonstrate a link with pseudo-/fake supersymmetry and apply it to the ekpyrotic scenario in cosmology. For the latter we observe that the pre-uplift KKLT potential could provide a stringy embedding of ekpyrosis away from the asymptotic regimes in field space.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Sharpened Dynamical Cobordism

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    Sharpened Dynamical Cobordism ties the allowed range of critical exponent δ to theory structure ξ, flagging obstructions from non-trivial cobordism charges that require new degrees of freedom.

  2. Optimal paths across potentials on scalar field space

    hep-th 2026-04 unverdicted novelty 7.0

    Optimal transport yields a generalized Wasserstein distance on field space, obtained from a WKB expansion of a Schrödinger equation and extended to dynamical gravity via the Wheeler-DeWitt equation in the ADM formalism.

  3. The CFT Distance Conjecture and Tensionless String Limits in $\mathcal N=2$ Quiver Gauge Theories

    hep-th 2026-01 unverdicted novelty 7.0

    In N=2 SU quiver theories the large-N Hagedorn temperature depends only on quiver length for linear cases and equals that of N=4 SYM for holographic quivers, with a universal lower bound of 1/sqrt(2) on the exponentia...