Abstract

In higher-dimensional supersymmetric theories gauge couplings of the effective four-dimensional theory are determined by expectation values of scalar fields. We find that at temperatures above a critical temperature T∗, which depends on the supersymmetry breaking mass scales, gauge couplings decrease like T−α, α>1. This has important cosmological consequences. In particular it leads to a relic gravitino density which becomes independent of the reheating temperature for TR>T∗. For small gravitino masses, m3/2⪡mg̃, the mass density of stable gravitinos is essentially determined by the gluino mass. The observed value of cold dark matter, ΩCDMh2∼0.1, is obtained for gluino masses mg̃=O(1 TeV).

Highlights

  • In higher-dimensional supersymmetric theories [1], where the standard model emerges as low-energy effective theory, gauge and Yukawa couplings are determined by expectation values of gauge singlet ‘moduli’ fields

  • In the following we study the dependence of gauge couplings on temperature

  • ‘Vacuum alignment’ at high temperatures causes a power-like decrease of gauge couplings

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Summary

Introduction

In higher-dimensional supersymmetric theories [1], where the standard model emerges as low-energy effective theory, gauge and Yukawa couplings are determined by expectation values of gauge singlet ‘moduli’ fields. One obtains for the 4d gauge coupling and for the gaugino mass, V gD2 At finite temperature the gauge kinetic term acquires an expectation value which leads to a force on the scalar field φ.

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