Hadronic and Hadron-Like Physics of Dark Matter

Symmetry

Vladimir Kuksa¹  MaximYu. Khlopov¹  Nikolay Volchanskiy¹  Vitaly Beylin¹ 

[1] Institute of Physics, Southern Federal University, Stachki 194, Rostov on Don 344090, Russia;

关键词: cosmology;    particle physics;    cosmo–particle physics;    QCD;    hyper-color;    dark atoms;    composite dark matter;   

DOI  :  10.3390/sym11040587

来源: DOAJ

【 摘 要 】

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.

【 授权许可】

Unknown