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Asymmetric Dark Matter in Baryon Asymmetrical Universe

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dc.contributor.authorBeylin, V. A.
dc.contributor.authorKhlopov, M. Y.
dc.contributor.authorSopin, D. O.
dc.contributor.authorХлопов, Максим Юрьевич
dc.date.accessioned2024-12-04T10:23:35Z
dc.date.available2024-12-04T10:23:35Z
dc.date.issued2024
dc.description.abstractNew heavy particles with electroweak charges arise in extensions of the standard model. They should take part in sphaleron transitions in the early Universe, which balance baryon asymmetry with the excess of new charged particles. If electrically charged with charge ў??2n, they bind with n nuclei of primordial helium in dark atoms of dark matter. This makes it possible to find the ratio of densities of asymmetric dark matter and baryonic matter. Examples of the model with new, successive, and stable generation of quarks and leptons and the minimal walking technicolor model are considered.
dc.identifier.citationBeylin, V. A. Asymmetric Dark Matter in Baryon Asymmetrical Universe / Beylin, V. A., Khlopov, M. Y., Sopin, D. O. // Symmetry. - 2024. - 16. - № 3. - 10.3390/sym16030311
dc.identifier.doi10.3390/sym16030311
dc.identifier.urihttps://www.doi.org/10.3390/sym16030311
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85189036168&origin=resultslist
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/25907
dc.relation.ispartofSymmetry
dc.titleAsymmetric Dark Matter in Baryon Asymmetrical Universe
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue3
oaire.citation.volume16
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relation.isAuthorOfPublication.latestForDiscovery4d7bf61d-b2ed-4073-a582-ab128ad9e096
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