Colored dark matter

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dc.creatorDzhunushaliev, Vladimir
dc.date2007-11-12
dc.date2008-10-13
dc.date.accessioned2026-07-07T12:12:34Z
dc.date.available2026-07-07T12:12:34Z
dc.descriptionThe idea is considered that a classical non-Abelian gauge field can be considered as a dark matter candidate. It is shown that Yang-Mills equations have solutions with such distribution of the mass density that allows to describe a rotational curve of spiral galaxies. The conditions necessary for such consideration are considered. One parameter is estimated from Yang-Mills equations and from astrophysical observations (stars rotation curve). The agreement is to within 1%.
dc.descriptiontypos corrected
dc.identifierhttps://arxiv.org/abs/0711.1707
dc.identifierhttp://arxiv.org/abs/0711.1707
dc.identifierScience Echoes, Vol.4, No.1, 47-69 (2008)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/210584
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleColored dark matter
dc.typetext

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