The polarised IKKT matrix model

A bstract We establish a correspondence between a supersymmetric mass deformation of the IKKT matrix integral at large N and a background of Euclidean type IIB string theory. Both sides have sixteen supersymmetries and an SO(3) × SO(7) symmetry. In the limit of large mass the integral is dominated by a fuzzy sphere saddle point. This saddle corresponds to a Euclidean D 1-brane in a finite, Euclidean, ellipsoidal cavity. The cavity is supported by three-form NSNS flux that polarises N D -instantons into the D 1-brane. We furthermore use supersymmetric localisation to show that the deformed matrix integral can be reduced to a moduli space integral, allowing exact results away from the large mass limit. At small mass the D 1-branes can backreact on the geometry, and we discuss the possible formulation of a ‘timeless’ holography in such regimes.

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Publication Details

Journal
Journal of High Energy Physics
Published
2025-03-07
DOI
https://doi.org/10.1007/jhep03(2025)060
Citations
15
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
28.05
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article

The polarised IKKT matrix model

Sean A. Hartnoll, Jun Liu
15 citations
Journal of High Energy Physics
Black Holes and Theoretical Physics
28.05
article

The polarised IKKT matrix model

Sean A. Hartnoll, Jun Liu
article en
15 citations

Abstract

A bstract We establish a correspondence between a supersymmetric mass deformation of the IKKT matrix integral at large N and a background of Euclidean type IIB string theory. Both sides have sixteen supersymmetries and an SO(3) × SO(7) symmetry. In the limit of large mass the integral is dominated by a fuzzy sphere saddle point. This saddle corresponds to a Euclidean D 1-brane in a finite, Euclidean, ellipsoidal cavity. The cavity is supported by three-form NSNS flux that polarises N D -instantons into the D 1-brane. We furthermore use supersymmetric localisation to show that the deformed matrix integral can be reduced to a moduli space integral, allowing exact results away from the large mass limit. At small mass the D 1-branes can backreact on the geometry, and we discuss the possible formulation of a ‘timeless’ holography in such regimes.

Journal of High Energy PhysicsVol. 2025(3)
University of Cambridge (GB)
Openalex Percentile: Top 0%
Black Holes and Theoretical Physics
28.05
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