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March 25, 2026Journal of High Energy Physics2 citationsOpen Access

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

DRDaniel RobbinsUniversity at Albany, State University of New YorkHSHassaan SaleemUniversity at Albany, State University of New York

Key Points

  • This research investigates non-supersymmetric AdS3 × S3 vacuua in O(16) × O(16) heterotic string theory.
  • Studied effective theory on AdS3 × S3 × T4 background.
  • Analyzed one-loop contributions to the cosmological constant.
  • Examined scalar and tensor mode fluctuations around vacua.
  • Assessed moduli behavior from torus compactification.
  • Cosmological constant increases with one-loop scalar potential but does not yield de Sitter uplift.
  • All scalar and tensor modes exceed the Breitenlohner-Freedman bound.
  • Torus moduli remain above the bound for a large range of flux values.

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.

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Cite This Study

Robbins et al. (2026) studied this question.

synapsesocial.com/papers/69c37ba2b34aaaeb1a67e4c4https://doi.org/10.1007/jhep03(2026)212
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