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Hadronic and Hadron-Like Physics of Dark Matter

1
Institute of Physics, Southern Federal University, Stachki 194, Rostov on Don 344090, Russia
2
APC Laboratory 10, rue Alice Domon et Léonie Duquet, CEDEX 13, 75205 Paris, France
3
National Research Nuclear University “MEPHI” (Moscow State Engineering Physics Institute), 31 Kashirskoe Chaussee, Moscow 115409, Russia
4
Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Joliot-Curie 6, Dubna 141980, Russia
*
Author to whom correspondence should be addressed.
Symmetry 2019, 11(4), 587; https://doi.org/10.3390/sym11040587
Received: 29 March 2019 / Revised: 15 April 2019 / Accepted: 17 April 2019 / Published: 23 April 2019
(This article belongs to the Special Issue Cosmological Inflation, Dark Matter and Dark Energy)
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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. View Full-Text
Keywords: cosmology; particle physics; cosmo–particle physics; QCD; hyper-color; dark atoms; composite dark matter cosmology; particle physics; cosmo–particle physics; QCD; hyper-color; dark atoms; composite dark matter
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited (CC BY 4.0).
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Beylin, V.; Khlopov, M.Y.; Kuksa, V.; Volchanskiy, N. Hadronic and Hadron-Like Physics of Dark Matter. Symmetry 2019, 11, 587.

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