Explaining the Electroweak Scale and Stabilizing Moduli in M Theory
Bobby S. Acharya, Konstantin Bobkov, Gordon L. Kane, Piyush Kumar, Jing Shao
TL;DR
This work provides a detailed mechanism for stabilizing all moduli in fluxless M theory on G2-holonomy manifolds via nonperturbative hidden-sector dynamics, yielding a (nearly) unique metastable de Sitter vacuum with spontaneously broken SUSY. A central result is the suppression of tree-level gaugino masses relative to the gravitino mass, which, together with anomaly-mediated contributions, produces a phenomenologically viable superpartner spectrum with TeV-scale gauginos and heavier scalars. Imposing a small cosmological constant drives the gravitino mass into the 1–100 TeV range, while the LHC signatures are predicted to be gluino-rich and distinct from Type IIB scenarios. The analysis covers both AdS and dS vacua, extends to hidden-sector matter, and shows that the resulting soft terms are largely controlled by the underlying geometric data of the G2 manifold, with robust implications for collider phenomenology and dark matter.
Abstract
In a recent paper \cite{Acharya:2006ia} it was shown that in $M$ theory vacua without fluxes, all moduli are stabilized by the effective potential and a stable hierarchy is generated, consistent with standard gauge unification. This paper explains the results of \cite{Acharya:2006ia} in more detail and generalizes them, finding an essentially unique de Sitter (dS) vacuum under reasonable conditions. One of the main phenomenological consequences is a prediction which emerges from this entire class of vacua: namely gaugino masses are significantly suppressed relative to the gravitino mass. We also present evidence that, for those vacua in which the vacuum energy is small, the gravitino mass, which sets all the superpartner masses, is automatically in the TeV - 100 TeV range.
