The Heterotic Road to the MSSM with R parity
Oleg Lebedev, Hans Peter Nilles, Stuart Raby, Saul Ramos-Sanchez, Michael Ratz, Patrick K. S. Vaudrevange, Akin Wingerter
TL;DR
This work extends a heterotic Z6-II orbifold search to identify numerous vacua that realize the MSSM spectrum with exact R-parity and vector-like exotics decoupled along D-flat directions. By enforcing a B−L–based family reflection symmetry and carefully analyzing F=0/D=0 conditions, the authors isolate 15 models with exact R-parity and viable top Yukawas, among them two explicit benchmark vacua with realistic Yukawa textures and See-Saw neutrino masses. They demonstrate that the μ-term can be correlated with the vacuum expectation value of the superpotential, potentially yielding a Minkowski-like vacuum with small gravitino mass in Model 1, while Model 2 presents different Higgs mixing and mass-generation patterns. The results illustrate that a non-negligible fraction of heterotic vacua can mimic MSSM physics, while also highlighting challenges such as dimension-5 proton decay operators and the need for moduli stabilization and SUSY-breaking mechanisms. Overall, the paper provides concrete string-theoretic pathways to MSSM-like physics with robust R-parity, along with detailed analyses of exotics, Yukawa structures, and neutrino masses in explicit vacua.
Abstract
In a previous paper, referred to as a "Mini-Landscape" search, we explored a "fertile patch" of the heterotic landscape based on a Z6-II orbifold with SO(10) and E6 local GUT structures. In the present paper we extend this analysis. We find many models with the minimal supersymmetric standard model spectra and an exact R parity. In all of these models, the vector-like exotics decouple along D flat directions. We present two "benchmark" models which satisfy many of the constraints of a realistic supersymmetric model, including non-trivial Yukawa matrices for 3 families of quarks and leptons and Majorana neutrino masses for right-handed neutrinos with non-trivial See-Saw masses for the 3 light neutrinos. In an appendix we comment on the important issue of string selection rules and in particular the so-called "gamma-rule".
