Abstract

Abstract A few 9D interpolating models with two parameters are constructed and the massless spectra are studied by considering compactification of heterotic strings on a twisted circle with a Wilson line. It is found that there are some conditions between radius $R$ and Wilson line $A$ under which the gauge symmetry is enhanced. In particular, when the gauge symmetry is enhanced to $SO(18)\times SO(14)$, the cosmological constant is exponentially suppressed. We also construct a non-supersymmetric string model that is tachyon-free in all regions of moduli space and whose gauge symmetry involves $E_8$.

Highlights

  • LHC experiments suggest that supersymmetry (SUSY) does not exist at low energy scale

  • We provide the interpolations between the ten-dimensional non-supersymmetric SO(16) × SO(16) heterotic string model and one of the ten-dimensional supersymmetric heterotic strings[27] as model M2

  • We have found some conditions between circle radius R and Wilson line A under which additional massless states are present

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Summary

Introduction

LHC experiments suggest that supersymmetry (SUSY) does not exist at low energy scale. While several methods to construct such models have been proposed[14, 15, 16, 17, 18, 19, 20, 21], in this paper, we try to construct non-supersymmetric heterotic models with a small cosmological constant by focusing on so-called interpolating models[6, 8, 9, 10]. If model M1 is supersymmetric and the Z2 action contains (−1)F where F is the spacetime fermion number, the compactification causes SUSY breaking and the nine-dimensional interpolating model and model M2 become non-supersymmetric. In order to generate cases with NF −NB = 0, we need to increase the number of adjustable parameters One such possibility is to compactify more dimensions. We instead consider nine-dimensional interpolating models with one more parameter by introducing a constant Wilson line background

Interpolating models with no Wilson line
The construction of interpolating models
Two examples
Interpolating models with Wilson line
The limiting cases
The massless spectrum
Conclusions
A Notation for the partition functions
B The expansions of the characters
The case with no Wilson line
The case with Wilson line
Full Text
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