Asymptotic curvature divergences and non-gravitational theories

A bstract We analyse divergences of the scalar curvature R of the vector multiplet moduli space of type IIA string theory compactified on a Calabi-Yau X , along infinite-distance large volume limits. Extending previous results, we classify the origin of the divergence along trajectories which implement decompactifications to F-theory on X and/or emergent heterotic string limits. In all cases, the curvature divergence can be traced back to a 4d rigid field theory that decouples from gravity along the limit. This can be quantified via the asymptotic relation R ~ (Λ WGC / Λ sp ) 2 ν , with Λ WGC ≡ g rigid M P and Λ sp the species scale. In the UV, the 4d rigid field theory becomes a higher-dimensional, strongly-coupled rigid theory that also decouples from gravity. The nature of this UV theory is encoded in the exponent ν , and it either corresponds to a 5d SCFT, 6d SCFT or a Little String Theory.

Authors

Institutions

Publication Details

Journal
Journal of High Energy Physics
Published
2025-02-21
DOI
https://doi.org/10.1007/jhep02(2025)151
Citations
11
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
12.70

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Asymptotic curvature divergences and non-gravitational theories

Fernando Marchesano, Luca Melotti, Max Wiesner
11 citations
Journal of High Energy Physics
Cosmology and Gravitation Theories
12.70
article

Asymptotic curvature divergences and non-gravitational theories

Fernando Marchesano, Luca Melotti, Max Wiesner
article en
11 citations

Abstract

A bstract We analyse divergences of the scalar curvature R of the vector multiplet moduli space of type IIA string theory compactified on a Calabi-Yau X , along infinite-distance large volume limits. Extending previous results, we classify the origin of the divergence along trajectories which implement decompactifications to F-theory on X and/or emergent heterotic string limits. In all cases, the curvature divergence can be traced back to a 4d rigid field theory that decouples from gravity along the limit. This can be quantified via the asymptotic relation R ~ (Λ WGC / Λ sp ) 2 ν , with Λ WGC ≡ g rigid M P and Λ sp the species scale. In the UV, the 4d rigid field theory becomes a higher-dimensional, strongly-coupled rigid theory that also decouples from gravity. The nature of this UV theory is encoded in the exponent ν , and it either corresponds to a 5d SCFT, 6d SCFT or a Little String Theory.

Journal of High Energy PhysicsVol. 2025(2)
Consejo Superior de Investigaciones Científicas (ES), Harvard University Press (US), Universidad Autónoma de Madrid (ES)
National Science Foundation, Harvard University, Erwin Schrödinger International Institute for Mathematics and Physics, European Regional Development Fund, Agencia Estatal de Investigación
Openalex Percentile: Top 1%
Cosmology and Gravitation Theories
12.70
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Asymptotic curvature divergences and non-gravitational theories — Fernando Marchesano, Luca Melotti, et al. · Journal of High Energy Physics (2025) | TGRS Research Map | TGRS