Hadronic and Hadron-Like Physics of Dark Matter Vitaly Beylin∗ Research Institute of Physics, Southern Federal University, Prospekt Stachki, 194, 344090 Rostov-na-Donu, Russia Maxim Yu. Khlopov† Research Institute of Physics, Southern Federal University, Prospekt Stachki, 194, 344090 Rostov-na-Donu, Russia APC Laboratory 10, rue Alice Domon et L´eonie Duquet, CEDEX 13, 75205 Paris, France and National Research Nuclear University “MEPHI” (Moscow State Engineering Physics Institute), 31 Kashirskoe Chaussee, Moscow 115409, Russia Vladimir Kuksa‡ Research Institute of Physics, Southern Federal University, Prospekt Stachki, 194, 344090 Rostov-na-Donu, Russia Nikolay Volchanskiy§ Research Institute of Physics, Southern Federal University, Prospekt Stachki, 194, 344090 Rostov-na-Donu, Russia and Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Joliot-Curie 6, Dubna 141980, Russia The problems of simple elementary weakly interacting massive particles (WIMPs) appeal to ex- tend 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. arXiv:1904.12013v1 [hep-ph] 26 Apr 2019 ∗
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[email protected] 2 I. INTRODUCTION The nature of dark matter is inevitably linked to beyond the Standard Model (BSM) physics of elementary particles.