Hadronic and Hadron-Like Physics of Dark Matter

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 m...

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Main Authors: Vitaly Beylin, Maxim Yu. Khlopov, Vladimir Kuksa, Nikolay Volchanskiy
Format: Article
Language:English
Published: MDPI AG 2019-04-01
Series:Symmetry
Subjects:
Online Access:https://www.mdpi.com/2073-8994/11/4/587
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author Vitaly Beylin
Maxim Yu. Khlopov
Vladimir Kuksa
Nikolay Volchanskiy
author_facet Vitaly Beylin
Maxim Yu. Khlopov
Vladimir Kuksa
Nikolay Volchanskiy
author_sort Vitaly Beylin
collection DOAJ
description 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.
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spelling doaj.art-b6e5f24425b94901ae29c35bfcfad5d32022-12-22T02:53:55ZengMDPI AGSymmetry2073-89942019-04-0111458710.3390/sym11040587sym11040587Hadronic and Hadron-Like Physics of Dark MatterVitaly Beylin0Maxim Yu. Khlopov1Vladimir Kuksa2Nikolay Volchanskiy3Institute of Physics, Southern Federal University, Stachki 194, Rostov on Don 344090, RussiaInstitute of Physics, Southern Federal University, Stachki 194, Rostov on Don 344090, RussiaInstitute of Physics, Southern Federal University, Stachki 194, Rostov on Don 344090, RussiaInstitute of Physics, Southern Federal University, Stachki 194, Rostov on Don 344090, RussiaThe 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.https://www.mdpi.com/2073-8994/11/4/587cosmologyparticle physicscosmo–particle physicsQCDhyper-colordark atomscomposite dark matter
spellingShingle Vitaly Beylin
Maxim Yu. Khlopov
Vladimir Kuksa
Nikolay Volchanskiy
Hadronic and Hadron-Like Physics of Dark Matter
Symmetry
cosmology
particle physics
cosmo–particle physics
QCD
hyper-color
dark atoms
composite dark matter
title Hadronic and Hadron-Like Physics of Dark Matter
title_full Hadronic and Hadron-Like Physics of Dark Matter
title_fullStr Hadronic and Hadron-Like Physics of Dark Matter
title_full_unstemmed Hadronic and Hadron-Like Physics of Dark Matter
title_short Hadronic and Hadron-Like Physics of Dark Matter
title_sort hadronic and hadron like physics of dark matter
topic cosmology
particle physics
cosmo–particle physics
QCD
hyper-color
dark atoms
composite dark matter
url https://www.mdpi.com/2073-8994/11/4/587
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AT maximyukhlopov hadronicandhadronlikephysicsofdarkmatter
AT vladimirkuksa hadronicandhadronlikephysicsofdarkmatter
AT nikolayvolchanskiy hadronicandhadronlikephysicsofdarkmatter