Probes for Dark Matter Physics
arXiv:1802.10184 · doi:10.1142/S0218271818410134
Abstract
The existence of cosmological dark matter is in the bedrock of the modern cosmology. The dark matter is assumed to be nonbaryonic and to consist of new stable particles. However if composite dark matter contains stable electrically charged leptons and quarks bound by ordinary Coulomb interaction in elusive dark atoms, these charged constituents of dark atoms can be the subject of direct experimental test at the colliders. In such models the excessive negatively double charged particles are bound with primordial helium in O-helium atoms, maintaining specific nuclear-interacting form of the dark matter. The successful development of composite dark matter scenarios appeals to experimental search for doubly charged constituents of dark atoms, making experimental search for exotic stable double charged particles experimentum crucis for dark atoms of composite dark matter. (abridged)
Invited contribution to the IJMPD special issue "New trends in High Energy Physics. Cosmology and Astroparticle physics". arXiv admin note: text overlap with arXiv:1711.10773, arXiv:1402.0181
References in corpus (11)
- Dark Matter Candidates from Particle Physics and Methods of Detection
- Dark matter and cosmic structure
- Exciting Dark Matter and the INTEGRAL/SPI 511 keV signal
- Stable Massive Particles at Colliders
- Dark Matter from new Technicolor Theories
- Mirror particles and mirror matter: 50 years of speculation and search
- Towards Working Technicolor: Effective Theories and Dark Matter
- Composite dark matter from a model with composite Higgs boson
- Strong Interactive Massive Particles from a Strong Coupled Theory
- Cosmology with Mirror Dark Matter
- Search for Dark Matter
Cited by in corpus (8)
- Axion Dark Matter Search with Interferometric Gravitational Wave Detectors
- Status, Challenges and Directions in Indirect Dark Matter Searches
- Axion dark matter search using arm cavity transmitted beams of gravitational wave detectors
- Double charged heavy constituents of dark atoms and superheavy nuclear objects
- The maximum mass of dark matter existing in compact stars based on the self-interacting fermionic model
- Cosmoparticle physics of dark matter
- Observational constraints on dark matter decaying via gravity portals
- Search for H2 cloudlets in our backyard