O(16) × O(16) heterotic theory on AdS3 × S3 × T4

A bstract In this paper, we study non-supersymmetric AdS 3 × S 3 vacuua of O (16) × O (16) heterotic theory on a string scale T 4 background, which are parameterized by a pair of flux integers. Adding the one-loop scalar potential to the effective theory contributes positively to the cosmological constant, but we find that there is no uplift to de Sitter for any values of the fluxes. We study the fluctuations around these vacua and show that all scalar and tensor modes from the six-dimensional effective theory lie above the Breitenlohner-Freedman bound. The moduli coming from the torus compactification will also be above the bound, at least for a large range of fluxes.

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Publication Details

Journal
Journal of High Energy Physics
Published
2026-03-23
DOI
https://doi.org/10.1007/jhep03(2026)212
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
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article

O(16) × O(16) heterotic theory on AdS3 × S3 × T4

Hassaan Saleem, Daniel Robbins
Journal of High Energy Physics
Black Holes and Theoretical Physics
article

O(16) × O(16) heterotic theory on AdS3 × S3 × T4

Hassaan Saleem, Daniel Robbins
article en

Abstract

A bstract In this paper, we study non-supersymmetric AdS 3 × S 3 vacuua of O (16) × O (16) heterotic theory on a string scale T 4 background, which are parameterized by a pair of flux integers. Adding the one-loop scalar potential to the effective theory contributes positively to the cosmological constant, but we find that there is no uplift to de Sitter for any values of the fluxes. We study the fluctuations around these vacua and show that all scalar and tensor modes from the six-dimensional effective theory lie above the Breitenlohner-Freedman bound. The moduli coming from the torus compactification will also be above the bound, at least for a large range of fluxes.

Journal of High Energy PhysicsVol. 2026(3)
University at Albany, State University of New York (US)
Openalex Percentile: Top 11%
Black Holes and Theoretical Physics
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