Towards a UV-Model of Kinetic Mixing and Portal Matter II: Exploring Unification in an $SU(N)$ Group
Thomas G. Rizzo

TL;DR
This paper investigates the unification of dark and Standard Model forces through an $SU(N)$ group, exploring how kinetic mixing and portal matter can fit into a grand unified theory framework, with constraints on model building.
Contribution
It introduces a top-down approach to unify dark and SM interactions via $SU(N)$ groups, analyzing constraints and potential models for force unification.
Findings
Highly constrained model possibilities due to strict building requirements
Unification of dark and SM sectors via $SU(N)$ groups with $N=6-10$
Potential inclusion of SM generational unification within the framework
Abstract
If dark matter (DM) interacts with the Standard Model (SM) via the kinetic mixing (KM) portal at low energies, it necessitates not only the existence of portal matter (PM) particles which carry both dark and SM quantum numbers, but also a possible UV completion into which this and the SM are both embedded. In earlier work, following a bottom-up approach, we attempted to construct a more unified framework of these SM and dark sector interactions. In this paper we will instead begin to explore, from the top-down, the possibility of the unification of these forces via the decomposition of a GUT-like group, , where is now a low energy diagonal subgroup of and where the familiar will play the role of a proxy for the conventional SM gauge group. In particular, for this study…
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Taxonomy
TopicsCold Atom Physics and Bose-Einstein Condensates · Dark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research
