Dark Matter and Collider Phenomenology of Universal Extra Dimensions
Dan Hooper, Stefano Profumo
TL;DR
This paper surveys Universal Extra Dimensions (UED), where all Standard Model fields propagate in flat, compactified extra dimensions, yielding a KK tower with near-degenerate masses. A key feature is KK parity, ensuring loop-level contributions to SM observables, pair production of KK states, and a stable LKP that can serve as dark matter; the most studied LKP is the KK photon B^{(1)}. The authors detail the KK spectrum, electroweak and collider constraints, and the rich dark matter phenomenology, including relic density, direct/indirect detection, gamma rays, and antimatter signals, while outlining collider signatures at the LHC and ILC and strategies to distinguish UED from SUSY. They also explore beyond-one-dimension scenarios, KK graviton considerations, and benchmark models, emphasizing the importance of multi-messenger probes to validate or refute UED as the correct description of TeV-scale physics.
Abstract
We review the phenomenology of models with flat, compactified extra dimensions where all of the Standard Model fields are allowed to propagate in the bulk, known as Universal Extra Dimensions (UED). UED make for an interesting TeV-scale physics scenario, featuring a tower of Kaluza-Klein (KK) states approximately degenerate in mass at the scale set by the inverse size of the compactification radius. KK parity, the four-dimensional remnant of momentum conservation in the extra dimensions, implies two basic consequences: (1) contributions to Standard Model observables arise only at loop level, and KK states can only be pair-produced at colliders, and (2) the lightest KK particle (LKP) is stable, providing a suitable particle dark matter candidate. After a theoretical overview on extra dimensional models, and on UED in particular, we introduce the model particle spectrum and the constraints from precision electroweak tests and current colliders data. We then give a detailed overview of the LKP dark matter phenomenology, including the LKP relic abundance, and direct and indirect searches. We then discuss the physics of UED at colliders, with particular emphasis on the signatures predicted for the Large Hadron Collider and at a future Linear Collider, as well as on the problem of discriminating between UED and other TeV-scale new physics scenarios, particularly supersymmetry. We propose a set of reference benchmark models, representative of different viable UED realizations. Finally, we collect in the Appendix all the relevant UED Feynman rules, the scattering cross sections for annihilation and coannihilation processes in the early universe and the production cross section for strongly interacting KK states at hadron colliders.
