Quintessential solution of dark matter rotation curves and its simulation by extra dimensions

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dc.creatorKiselev, V. V.
dc.date2003-03-09
dc.date2003-04-07
dc.date.accessioned2026-07-07T03:27:42Z
dc.date.available2026-07-07T03:27:42Z
dc.descriptionOn the base of an exact solution for the static spherically symmetric Einstein equations with the quintessential dark matter, we explain the asymptotic behavior of rotation curves in spiral galaxies. The parameter of the quintessence state, i.e. the ratio of its pressure to the density is tending to -1/3. We present an opportunity to imitate the relevant quintessence by appropriate scalar fields in the space-time with extra 2 dimensions.
dc.description11 pages, LaTeX file, 4 eps-figures, references added
dc.identifierhttps://arxiv.org/abs/gr-qc/0303031
dc.identifierhttp://arxiv.org/abs/gr-qc/0303031
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34534
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleQuintessential solution of dark matter rotation curves and its simulation by extra dimensions
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