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How Can We Obtain a Large Majorana-Mass in Calabi-Yau Models ?

arXiv:hep-ph/9401332 · doi:10.1143/ptp/92.1.153

Abstract

In a certain type of Calabi-Yau superstring models it is clarified that the symmetry breaking occurs by stages at two large intermediate energy scales and that two large intermediate scales induce large Majorana-masses of right-handed neutrinos. Peculiar structure of the effective nonrenormalizable interactions is crucial in the models. In this scheme Majorana-masses possibly amount to $O(10^{9 \sim 10}\gev)$ and see-saw mechanism is at work for neutrinos. Based on this scheme we propose a viable model which explains the smallness of masses for three kind of neutrinos $ν_e, ν_μ \ {\rm and}\ ν_τ$. Special forms of the nonrenormalizable interactions can be understood as a consequence of an appropriate discrete symmetry of the compactified manifold.

30-pages + 6-figures, LaTeX, Preprint DPNU-94-02, AUE-01-94