Naturally-Coupled Dark Sectors
arXiv:2105.04277
Abstract
The dark sector, composed of the fields neutral under the Standard Model (SM) gauge group, can couple to the SM through the Higgs, hypercharge and neutrino portals, and pull the SM towards its scale by loop corrections. This instability, not possible to prevent in the known SM completions like supersymmetry due to their sizable couplings to the SM, calls for alternative mechanisms which can neutralize sensitivities of the SM to the dark sector scale and to the ultraviolet cutoff above it. Here we review such a mechanism in which incorporation of gravity into the SM predicts the existence of a dark sector and allows it to be naturally-coupled to the SM. We discuss and illustrate salient processes which can probe the naturally-coupled dark sectors.
17 pages, 6 figures, 1 table. A review to appear in MDPI Galaxies Topical Collection "A Trip Across the Universe: Our Present Knowledge and Future Perspectives"
References in corpus (14)
- Dynamics of dark energy
- Inflation with Non-Minimal Coupling: Metric vs. Palatini Formulations
- Review of LHC Dark Matter Searches
- Current status of direct dark matter detection experiments
- Sterile Neutrinos as the Origin of Dark and Baryonic Matter
- Metric-affine Gravity and Inflation
- Determination of the strong coupling constant from transverse energy-energy correlations in multijet events at TeV using the ATLAS detector
- Dark sector origin of the KOTO and MiniBooNE anomalies
- The Search for Dark Matter
- Effects of Curvature-Higgs Coupling on Electroweak Fine-Tuning
- LIGO as a probe of Dark Sectors
- The Formulation of Quantum Field Theory in Curved Spacetime
- Naturalizing Gravity of the Quantum Fields, and the Hierarchy Problem
- Notes on Quantum Field Theory in Curved Spacetime: Problems Relating to the Concept of Particles and Hamiltonian Formalism