Hadronic and hadron-like physics of Dark Matter
arXiv:1904.12013 · doi:10.3390/sym11040587
Abstract
The problems of simple elementary weakly interacting massive particles (WIMPs) appeal to extend the physical basis for nonbaryonic dark matter. Such extension involves more sophisticated dark matter candidates from physics beyond the Standard Model (BSM) of elementary particles. We discuss several models of dark matter, predicting new colored, hyper-colored or techni-colored particles and their accelerator and non-accelerator probes. The nontrivial properties of the proposed dark matter candidates can shed new light on the dark matter physics. They provide interesting solutions for the puzzles of direct and indirect dark matter search.
39 pages; matches published version
References in corpus (24)
- Dark Matter Candidates from Particle Physics and Methods of Detection
- First results from DAMA/LIBRA and the combined results with DAMA/NaI
- Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation
- Cosmology and Astrophysics of Minimal Dark Matter
- First Dark Matter Results from the XENON100 Experiment
- Dark matter and cosmic structure
- DARWIN: towards the ultimate dark matter detector
- Particle physics catalysis of thermal Big Bang Nucleosynthesis
- Dark Matter from new Technicolor Theories
- Ultra Minimal Technicolor and its Dark Matter TIMP
- Towards Working Technicolor: Effective Theories and Dark Matter
- Towards Closing the Window on Strongly Interacting Dark Matter: Far-Reaching Constraints from Earth's Heat Flow
- Composite dark matter from a model with composite Higgs boson
- Big Bang Nucleosynthesis with Long Lived Charged Massive Particles
- Strong Interactive Massive Particles from a Strong Coupled Theory
- Dynamical generation of the weak and Dark Matter scales from strong interactions
- Remnants of dark matter clumps
- Dark Matter as a weakly coupled Dark Baryon
- Small-scale clumps of dark matter
- A minimal model for two-component dark matter
- UV complete composite Higgs models
- Search for Dark Matter
- Uranus's anomalously low excess heat constrains strongly interacting dark matter
- Decaying Dark Atom constituents and cosmic positron excess
Cited by in corpus (5)
- New physics of strong interaction and Dark Universe
- Glueballs in a Thermal Squeezeout Model
- Composite Dark Matter and Neutrino Masses from a Light Hidden Sector
- Cosmoparticle physics of dark matter
- Proposition of FSR Photon Suppression Employing a Two-Positron Decay Dark Matter Model to Explain Positron Anomaly in Cosmic Rays