Dark Dimension With (Little) Strings Attached

Abstract A relation between dark energy and the scale of new physics in weakly coupled string theory is motivated. This mixing between infrared and ultraviolet physics leads to a unique corner for real‐world phenomenology: barring fine‐tunings, the authors are naturally led to the “dark dimension” scenario, a single mesoscopic extra dimension of micron size with the standard model localized on D‐branes. Our explicit top‐down worldsheet derivation establishes it on a more solid grounding. Allowing some fine‐tuning, such that the vacuum energy only arise at higher orders in string perturbation theory, the “little string theory” scenario with a very weakly coupled string is an alternative possibility. In this case, the string scale lies at the edge of detectability of particle accelerators.

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Publication Details

Journal
Fortschritte der Physik
Published
2024-12-29
DOI
https://doi.org/10.1002/prop.202400265
Citations
7
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
2.32
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article

Dark Dimension With (Little) Strings Attached

Ivano Basile, Dieter Lüst
7 citations
Fortschritte der Physik
Cosmology and Gravitation Theories
2.32
article

Dark Dimension With (Little) Strings Attached

Ivano Basile, Dieter Lüst
article en
7 citations

Abstract

Abstract A relation between dark energy and the scale of new physics in weakly coupled string theory is motivated. This mixing between infrared and ultraviolet physics leads to a unique corner for real‐world phenomenology: barring fine‐tunings, the authors are naturally led to the “dark dimension” scenario, a single mesoscopic extra dimension of micron size with the standard model localized on D‐branes. Our explicit top‐down worldsheet derivation establishes it on a more solid grounding. Allowing some fine‐tuning, such that the vacuum energy only arise at higher orders in string perturbation theory, the “little string theory” scenario with a very weakly coupled string is an alternative possibility. In this case, the string scale lies at the edge of detectability of particle accelerators.

Fortschritte der PhysikVol. 73(4)
Max Planck Institute for Physics (DE), Ludwig-Maximilians-Universität München (DE)
Affordable and clean energy
Openalex Percentile: Top 12%
Cosmology and Gravitation Theories
2.32
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