Classical color fields as a dark matter candidate

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dc.creatorDzhunushaliev, Vladimir
dc.date2006-12-17
dc.date2007-04-30
dc.date.accessioned2026-07-07T11:00:29Z
dc.date.available2026-07-07T11:00:29Z
dc.descriptionThe model of Dark Matter is proposed in which the Dark Matter is a classical color field. The color fields are invisible as they may interact with colored elementary particles like 't Hooft - Polyakov monopole only. The comparison with the Universal Rotation Curve is carried out.
dc.descriptionchanges in the text
dc.identifierhttps://arxiv.org/abs/astro-ph/0612473
dc.identifierhttp://arxiv.org/abs/astro-ph/0612473
dc.identifierCentralEur.J.Phys.5:342-350,2007
dc.identifierdoi:10.2478/s11534-007-0028-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187689
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleClassical color fields as a dark matter candidate
dc.typetext

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