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Stabilizing Moduli with a Positive Cosmological Constant in Heterotic M-Theory

Volker Braun, Burt A. Ovrut

TL;DR

The paper investigates moduli stabilization in strongly coupled heterotic M-theory with bulk branes, demonstrating that a pure five-brane setup fixes all moduli but yields a large negative cosmological constant. By introducing anti-five-branes, the authors add a controlled uplift term that can raise the vacuum energy to a small positive, metastable de Sitter minimum while preserving moduli stabilization and breaking $N=1$ supersymmetry. The analysis is carried out in simplified yet representative sectors (starting with $h^{1,1}=1$ and extending to $h^{1,1}=2$), and is then specialized to the Minimal Heterotic Standard Model, where anomaly cancellation fixes brane content and explicit Kahler moduli regions are identified where the observable bundle remains slope-stable. The results show that all moduli can be stabilized in a metastable de Sitter vacuum with a phenomenologically viable positive cosmological constant and a realistic MSSM-like visible sector, providing a concrete string-theoretic mechanism for SUSY breaking and cosmological constant tuning.

Abstract

It is shown that strongly coupled heterotic M-theory with anti-five-branes in the S^1/Z_2 bulk space can have meta-stable vacua which break N=1 supersymmetry and have a small, positive cosmological constant. This is demonstrated for the "minimal" heterotic standard model. This vacuum has the exact MSSM matter spectrum in the observable sector, a trivial hidden sector vector bundle and both five-branes and anti-five-branes in the bulk space. The Kahler moduli for which the cosmological constant has phenomenologically acceptable values are shown to also render the observable sector vector bundle slope-stable. A corollary of this result is that strongly coupled M-theory vacua with only five-branes in the S^1/Z_2 interval may have stabilized moduli, but at a supersymmetry preserving minimum with a large, negative cosmological constant.

Stabilizing Moduli with a Positive Cosmological Constant in Heterotic M-Theory

TL;DR

The paper investigates moduli stabilization in strongly coupled heterotic M-theory with bulk branes, demonstrating that a pure five-brane setup fixes all moduli but yields a large negative cosmological constant. By introducing anti-five-branes, the authors add a controlled uplift term that can raise the vacuum energy to a small positive, metastable de Sitter minimum while preserving moduli stabilization and breaking supersymmetry. The analysis is carried out in simplified yet representative sectors (starting with and extending to ), and is then specialized to the Minimal Heterotic Standard Model, where anomaly cancellation fixes brane content and explicit Kahler moduli regions are identified where the observable bundle remains slope-stable. The results show that all moduli can be stabilized in a metastable de Sitter vacuum with a phenomenologically viable positive cosmological constant and a realistic MSSM-like visible sector, providing a concrete string-theoretic mechanism for SUSY breaking and cosmological constant tuning.

Abstract

It is shown that strongly coupled heterotic M-theory with anti-five-branes in the S^1/Z_2 bulk space can have meta-stable vacua which break N=1 supersymmetry and have a small, positive cosmological constant. This is demonstrated for the "minimal" heterotic standard model. This vacuum has the exact MSSM matter spectrum in the observable sector, a trivial hidden sector vector bundle and both five-branes and anti-five-branes in the bulk space. The Kahler moduli for which the cosmological constant has phenomenologically acceptable values are shown to also render the observable sector vector bundle slope-stable. A corollary of this result is that strongly coupled M-theory vacua with only five-branes in the S^1/Z_2 interval may have stabilized moduli, but at a supersymmetry preserving minimum with a large, negative cosmological constant.

Paper Structure

This paper contains 6 sections, 1 theorem, 143 equations, 1 figure.

Key Result

Proposition 1

If all line bundles $\mathcal{O}_{{\widetilde{X}}}(a_1\tau_1+a_2\tau_2+b\phi)$ with have negative slope then the vector bundle ${\widetilde{\mathcal{V}_{}}}$ is equivariantly stable.

Figures (1)

  • Figure 1: Kähler Cone. The observable sector vector bundle is slope-stable in the region $\mathcal{K}^s$.

Theorems & Definitions (1)

  • Proposition 1