Dark Matter, Dark Energy and Rotation Curves

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dc.creatorSivaram, C.
dc.creatorA, Venkata Manohara Reddy.
dc.date2007-10-24
dc.date.accessioned2026-07-07T08:38:20Z
dc.date.available2026-07-07T08:38:20Z
dc.descriptionModels for DM are invoked with various density distributions, to account for flat rotation curves of galaxies. The effect of DE on these profiles for large galaxies and clusters are also studied. The rotation curves are shown to dip at a particular distance, when the effect of DE became significant.
dc.description9 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/0710.4384
dc.identifierhttp://arxiv.org/abs/0710.4384
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/140691
dc.subjectAstrophysics
dc.titleDark Matter, Dark Energy and Rotation Curves
dc.typetext

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