Abstract

A three-step procedure is proposed in type IIA string theory to stabilize multiple moduli in a dS vacuum. The first step is to construct a progenitor model with a localized stable supersymmetric Minkowski vacuum, or a discrete set of such vacua. It can be done, for example, using two non-perturbative exponents in the superpotential for each modulus, as in the KL model [1]. A large set of supersymmetric Minkowski vacua with strongly stabilized moduli is protected by a theorem on stability of these vacua in absence of flat directions [2]. The second step involves a parametrically small downshift to a supersymmetric AdS vacuum, which can be achieved by a small change of the superpotential. The third step is an uplift to a dS vacuum with a positive cosmological constant using the overline{D6} -brane contribution [3, 4]. Stability of the resulting dS vacuum is inherited from the stability of the original supersymmetric Minkowski vacuum if the supersymmetry breaking in dS vacuum is parametrically small [2, 5].

Highlights

  • Stability of the resulting dS vacuum is inherited from the stability of the original supersymmetric Minkowski vacuum if the supersymmetry breaking in dS vacuum is parametrically small [2, 5]

  • One may argue that the situation with dS vacua in the type IIA string theory became similar to the situation in the type IIB case

  • In this paper we would like to suggest a procedure which allows mass production of dS vacua in the type IIA string theory based on models which have as their progenitors stable supersymmetric Minkowski vacua

Read more

Summary

A general theory

Our strategy of finding a theory with a supersymmetric Minkowski vacuum state with a potential having a localized minimum consists of the following steps. An uplifting of this vacuum state to a dS state with a nearly vanishing VAdS can be achieved due to the anti-D3-brane contribution represented by a nilpotent field X. One can describe it by adding a term μ2X to the superpotential and a term XXto the Kahler potential, and taking X = 0 after calculating all quantities of interest, such as the potential.

The basic KL model
Multifield supersymmetric Minkowski vacua and their dS uplift
Multifield KL scenario
An example
A lesson from WZ model
Uplift to dS minimum
String theory embedding of the new 4d supergravity models
Conclusions
A very small downshift and uplift
A significant downshift and uplift
A large uplift without downshift
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call