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Scale-separated vacua with extended supersymmetry

hep-th · 2026-04-29 · unverdicted · novelty 8.0

First examples of scale-separated vacua with extended supersymmetry are constructed as circle compactifications of 4D massive IIA solutions with additional fluxes and sources.

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.

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 4 of 4 citing papers after filters.

  • Scale-separated vacua with extended supersymmetry hep-th · 2026-04-29 · unverdicted · none · ref 2

    First examples of scale-separated vacua with extended supersymmetry are constructed as circle compactifications of 4D massive IIA solutions with additional fluxes and sources.

  • Alice in Warpland: KK modes, Warped Compactifications and the Swampland hep-th · 2026-03-11 · unverdicted · none · ref 94

    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.

  • Morse-Bott inequalities, Topology Change and Cobordisms to Nothing hep-th · 2024-10-28 · unverdicted · none · ref 109

    Morse-Bott inequalities yield homology bounds and topology-change counts for generic cobordisms to nothing in string theory compactifications.

  • Dark energy from string theory: an introductory review hep-th · 2026-03-26 · unverdicted · none · ref 249

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