Abstract

We study M-theory compactification on ${\mathbb{T}^7/ \mathbb{Z}_2^3}$ in the presence of a seven-flux, metric fluxes and KK monopoles. The effective four-dimensional supergravity has seven chiral multiplets whose couplings are specified by the $G_2$-structure of the internal manifold. We supplement the corresponding superpotential by a KKLT type non-perturbative exponential contribution for all, or for some of the seven moduli, and find a discrete set of supersymmetric Minkowski minima. We also study type IIA and type IIB string theory compactified on ${\mathbb{T}^6/ \mathbb{Z}_2^2}$. In type IIA, we use a six-flux, geometric fluxes and non-perturbative exponents. In type IIB theory, we use F and H fluxes, and non-geometric Q and P fluxes, corresponding to consistently gauged supergravity with certain embedding tensor components, \emph{without non-perturbative exponents}. Also in these situations, we produce discrete Minkowski minima. Finally, to construct dS vacua starting from these Minkowski progenitors, we follow the procedure of mass production of dS vacua.

Highlights

  • In [1,2], we introduced a method to construct de Sitter minima, starting from Minkowski minima in type IIA and type IIB string theory

  • To summarize the results obtained so far, in Model 2, Model 3, and Model 4 we find that quadratic tree-level contributions to the superpotential can take the place of some of the nonperturbative exponential terms that are usually required

  • M-theory is supposed to unify all of the consistent versions of superstring theory

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Summary

INTRODUCTION

In [1,2], we introduced a method to construct de Sitter minima, starting from Minkowski minima in type IIA and type IIB string theory. The purpose of this article is to use M-theory on the generalized twisted seven-torus to identify some relatively simple discrete supersymmetric Minkowski vacua in which all of the 14 real scalars are stabilized. These vacua can be used to stabilize all of the 14 moduli in dS minima, 2470-0010=2020=101(4)=046018(8). By including additional flux contributions, we can stabilize dS vacua in models where only some of the moduli have exponential terms in the superpotentials Some of these M-theory models have an interpretation as type IIA models compactified on T 6=Z22 with fluxes. We show that in this model one can construct stable dS vacua without using any nonperturbative exponential contribution in the superpotential

GENERALIZED TWISTED SEVEN-TORUS
GENERALIZED TWISTED SIX-TORUS
M-THEORY EXAMPLES
C12 C13 C21 C22 C23 C31
DISCUSSION
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