Stringy Origin of Neutrino Masses within the Minimal Supersymmetric Standard Model

dc.creatorCvetic, Mirjam
dc.date1992-10-01
dc.date.accessioned2026-07-07T03:55:42Z
dc.date.available2026-07-07T03:55:42Z
dc.descriptionWe present a ``gravity-induced'' seesaw mechanism, which accommodates neutrino masses ($m_ν\propto m_u^2/M_I$, with $m_u$ the corresponding quark mass and $M_I\simeq 4\times10^{11}$ GeV) compatible with the MSW study of the Solar neutrino deficit within the minimal supersymmetric Standard Model (the grand desert with the gauge coupling unification at $M_U\simeq 2\times10^{16}$ GeV). We show that for large radius ($R^2/α'={\cal O}(20)$) Calabi-Yau spaces, threshold corrections ensure $M_U^2=M_C^2/{\cal O} (2R^2/α')$ and the magnitude of the non-renormalizable terms in the superpotential yields $M_I= {\cal O}(e^{-R^2/α'})M_C$. Here $M_C=g\times 5.2\times 10^{17}$GeV is the scale of the tree level (genus zero) gauge coupling ($g$) unification.
dc.description6 pages, UPR-528-T, (Talk presented at the XXVI International Conference on High Energy Physics, August 6-12, 1992, Dallas, Texas)
dc.identifierhttps://arxiv.org/abs/hep-ph/9210201
dc.identifierhttp://arxiv.org/abs/hep-ph/9210201
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44658
dc.subjectHigh Energy Physics - Phenomenology
dc.titleStringy Origin of Neutrino Masses within the Minimal Supersymmetric Standard Model
dc.typetext

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