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Hadronic and Hadron-like physics of dark matter

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dc.contributor.authorBeylin, V.
dc.contributor.authorKuksa, V.
dc.contributor.authorVolchanskiy, N.
dc.contributor.authorKhlopov, M. Y.
dc.contributor.authorХлопов, Максим Юрьевич
dc.date.accessioned2024-11-21T08:35:44Z
dc.date.available2024-11-21T08:35:44Z
dc.date.issued2019
dc.description.abstract© 2019 by the authors. 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.
dc.identifier.citationHadronic and Hadron-like physics of dark matter / Beylin, V. [et al.] // Symmetry. - 2019. - 11. - № 4. - 10.3390/sym11040587
dc.identifier.doi10.3390/sym11040587
dc.identifier.urihttps://www.doi.org/10.3390/sym11040587
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85065483718&origin=resultslist
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000467314400146
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/18012
dc.relation.ispartofSymmetry
dc.titleHadronic and Hadron-like physics of dark matter
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue4
oaire.citation.volume11
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