Abstract

A mechanism for addressing the 'decompactification problem' is proposed, which consists of balancing the vacuum energy in Scherk-Schwarzed theories against contributions coming from non- perturbative physics. Universality of threshold corrections ensures that, in such situations, the stable minimum will have consistent gauge couplings for any gauge group that shares the same N = 2 beta function for the bulk excitations as the gauge group that takes part in the minimisation. Scherk- Schwarz compactification from 6D to 4D in heterotic strings is discussed explicitly, together with two alternative possibilities for the non-perturbative physics, namely metastable SQCD vacua and a single gaugino condensate. In the former case, it is shown that modular symmetries gives various consistency checks, and allow one to follow soft-terms, playing a similar role to R-symmetry in global SQCD. The latter case is particularly attractive when there is nett Bose-Fermi degeneracy in the massless sector. In such cases, because the original Casimir energy is generated entirely by excited and/or non-physical string modes, it is completely immune to the non-perturbative IR physics. The large separation between UV and IR contributions to the potential greatly simplifies the analysis of stabilisation, and is a general possibility that has not been considered before.

Highlights

  • The purpose of this paper is to argue that there is a way to realise order one couplings at large volume dynamically and without fine-tuning, providing a solution to the decompactification problem for a much broader class of models

  • It is argued that a general means of addressing the decompactification problem dynamically is to balance non-perturbative physics contributions to the vacuum energy against the Casimir energy in Scherk-Schwarzed theories

  • By contrast gauge symmetries with the wrong-sign beta function will remain as effectively global symmetries. Both the ISS mechanism and a single gaugino condensate were considered for the stabilising non-perturbative physics in the case of compactification from 6D to 4D in heterotic strings

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Summary

The mechanism in a 5D non-maximal Scherk-Schwarz model

It is convenient to proceed by developing the 5D example of the mechanism outlined in the Introduction, with the non-perturbative physics being the ISS mechanism. If one wishes to adopt the ISS results at face-value (with no extra KK modes to complicate things), one can impose a modest energy gap between the dynamical scale of the the SQCD theory and the mass-scale of the lowest lying KK modes, and in addition between the two sources of superymmetry breaking to ensure that the ISS analysis is not disrupted by the soft-terms that are already induced by the SS mechanism. The last constraint is on the elementary supersymmetric Dirac mass required in the ISS mechanism: it should take values mD 1/R It is simple and natural – not crucial – to take mD to be induced by the compactification, so that it too is proportional to 1/R, with constant of proportionality αD = RmD 1. It will be convenient to assume αD ∼ αF,B

The generic Casimir energy case
Spectrum and congruence subgroups in the effective supergravity theory
Calculation of Casimir energy
The congruence subgroup method for mapping soft-terms between Seiberg duals
Generic Casimir energy
UV-Casimir energy balanced against a gaugino condensate
Conclusion
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