The Standard Model and Dark Matter in a unified Einstein-Dirac system with discrete extra dimensions

TL;DR

This paper develops a unified Einstein-Dirac model with discrete extra dimensions that incorporates the Standard Model and dark matter candidates, predicting particle masses and interactions consistent with experimental data.

Contribution

It introduces a generalized Einstein-Dirac framework with discrete extra dimensions, unifying Standard Model fields and dark matter candidates within a gravitational setting.

Findings

Predicted Weinberg angle, Higgs, and top quark masses match experiments.

Kaluza-Klein modes of quark-leptons are potential dark matter candidates.

Small mixing angles lead to heavy Kaluza-Klein partners with weak couplings.

Abstract

The Dirac-Einstein system of quark-leptons coupled to gravity is constructed generalized in the space-time extended with chiral and dark discrete extra dimensions. The Einstein's gravity, all the Standard Model's gauge vector, and Higgs fields together with a dark photon, whose mass is generated by a dark Higgs scalar, can be incorporated in this framework as components of the generalized vielbein. The Standard Model derived from the extended Einstein-Hilbert action must satisfy some conditions leading to the predictions of Weinberg angle, Higgs and top quark masses in excellent agreement with experiments. Since, the Dirac operator extended by discrete derivatives has resulted in a non-diagonal mass matrix, which mixes each quark-lepton with its Kaluza-Klein partner. On one hand, the small mixing angle set a Stueckelberg mass to the quark-leptons' Kaluza-Klein partners at least in the hundreds TeV range. On the other hand, it implies weak couplings between the Kaluza-Klein partners of quark-leptons and the Standard Model's gauge vector fields. This feature indicates that these Kaluza-Klein modes can be considered as candidates of dark matters.