How to Reach the Correct sin^2\theta_W and \alpha_S in String Theory
High Energy Physics - Theory
2008-11-26 v1 High Energy Physics - Phenomenology
Abstract
Effective theories with the matter content of the minimal supersymmetric Standard Model below the string scale M_string predict a wrong value for the weak--mixing angle sin^2\theta_W and strong coupling constant \alpha_S at the scale M_Z. To resolve this problem one needs large threshold corrections. At the same time one would like to avoid introducing new intermediate scales that are small compared to M_string. Two requests which seem to be incompatible. We show how both requirements can be satisfied in a class of (0,2) heterotic superstring compactifications with a natural choice of the vevs of the moduli fields entering the moduli dependent string threshold corrections.
Keywords
Cite
@article{arxiv.hep-th/9510009,
title = {How to Reach the Correct sin^2\theta_W and \alpha_S in String Theory},
author = {H. P. Nilles and S. Stieberger},
journal= {arXiv preprint arXiv:hep-th/9510009},
year = {2008}
}
Comments
11 LaTex pages with 2 figures