Abstract

The compactification from the 11-dimensional Horava-Witten orbifold to 5-dimensional heterotic M-theory on a Schoen Calabi-Yau threefold is reviewed, as is the specific S U ( 4 ) vector bundle leading to the “heterotic standard model” in the observable sector. A generic formalism for a consistent hidden sector gauge bundle, within the context of strongly coupled heterotic M-theory, is presented. Anomaly cancellation and the associated bulk space 5-branes are discussed in this context. The further compactification to a 4-dimensional effective field theory on a linearized BPS double domain wall is then presented to order κ 11 4 / 3 . Specifically, the generic constraints required for anomaly cancellation and by the linearized domain wall solution, restrictions imposed by the vanishing of the D-terms and, finally, the constraints imposed by the necessity for positive, perturbative squared gauge couplings to this order are presented in detail.

Highlights

  • One of the major prerogatives of the Large Hadron Collider (LHC) at CERN is to search for low-energy N = 1 supersymmetry

  • It has long been known that specific vacua of both the weakly coupled [1,2] and strongly coupled [3,4,5] E8 × E8 heterotic superstring can produce effective theories with at least a quasi-realistic particle spectrum exhibiting N = 1 supersymmetry [6,7,8,9,10]

  • We present the precise constraints required by such a vacuum within the context of heterotic strongly coupled M-theory

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Summary

Introduction

Symmetry 2018, 10, 723 papers on the heterotic standard model, in analogy with the KKLT mechanism [38] in Type II string theory, allowed the hidden sector to contain an anti-5-brane– explicitly breaking N = 1 supersymmetry [39,40] This was done so that the potential energy could admit a meta-stable de Sitter space vacuum. We consider a specific set of vacua for which the hidden sector vector bundle is restricted to be the Whitney sum of one non-Abelian SU ( N ) bundle with a single line bundle, while allowing only one five-brane in the bulk space Under these circumstances, the constraint equations greatly simplify and are explicitly presented. We demonstrate how the parameters associated with these bundles are computed for a specific choice of these objects

The Compactification Vacuum
The Calabi-Yau Threefold
The Observable Sector Gauge Bundle
The Hidden Sector Gauge Bundle
Bulk Space Five-Branes
Anomaly Cancellation
The κ11
Corrections to a Fayet-Iliopoulos Term
Gauge Threshold Corrections
A Specific Class of Examples
Full Text
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