Off-Diagonal Dark-Matter Phenomenology: Exploring Enhanced Complementarity Relations in Non-Minimal Dark Sectors
arXiv:1708.09698 · doi:10.1103/PhysRevD.96.115009
Abstract
In most multi-component dark-matter scenarios, two classes of processes generically contribute to event rates at experiments capable of probing the nature of the dark sector. The first class consists of "diagonal" processes involving only a single species of dark-matter particle -- processes analogous to those which arise in single-component dark-matter scenarios. By contrast, the second class consists of "off-diagonal" processes involving dark-matter particles of different species. Such processes include inelastic scattering at direct-detection experiments, asymmetric production at colliders, dark-matter co-annihilation, and certain kinds of dark-matter decay. In typical multi-component scenarios, the contributions from diagonal processes dominate over those from off-diagonal processes. Unfortunately, this tends to mask those features which are most sensitive to the multi-component nature of the dark sector. In this paper, by contrast, we point out that there exist natural, multi-component dark-sector scenarios in which the off-diagonal contributions actually dominate over the diagonal. This then gives rise to a new, enhanced picture of dark-matter complementarity. In this paper, we introduce a scenario in which this situation arises and examine the enhanced picture of dark-matter complementarity which emerges.
17 pages, LaTeX, 2 figures. Replaced to match published version
References in corpus (16)
- PYTHIA 6.4 Physics and Manual
- Results from a search for dark matter in the complete LUX exposure
- Dark Matter Candidates from Particle Physics and Methods of Detection
- FeynRules - Feynman rules made easy
- Dark Matter Results From 54-Ton-Day Exposure of PandaX-II Experiment
- General Constraints on Dark Matter Decay from the Cosmic Microwave Background
- Limits on spin-dependent WIMP-nucleon cross section obtained from the complete LUX exposure
- Standard Model anatomy of WIMP dark matter direct detection II: QCD analysis and hadronic matrix elements
- Hitomi constraints on the 3.5 keV line in the Perseus galaxy cluster
- How Dark Are Majorana WIMPs? Signals from MiDM and Rayleigh Dark Matter
- Constraints on decaying Dark Matter from XMM-Newton observations of M31
- Constraints on the parameters of radiatively decaying dark matter from the dark matter halo of the Milky Way and Ursa Minor
- A New Direction in Dark-Matter Complementarity: Dark-Matter Decay as a Complementary Probe of Multi-Component Dark Sectors
- Search for dark matter in association with a Higgs boson decaying to -quarks in collisions at TeV with the ATLAS detector
- Search for dark matter produced in association with a hadronically decaying vector boson in pp collisions at =13 TeV with the ATLAS detector
- Search for new physics in the monophoton final state in proton-proton collisions at sqrt(s) = 13 TeV