General Relativistic Galaxy Rotation Curves: Implications for Dark Matter Distribution

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dc.creatorMenzies, Dylan
dc.creatorMathews, Grant J.
dc.date2006-04-21
dc.date.accessioned2026-07-07T07:09:39Z
dc.date.available2026-07-07T07:09:39Z
dc.descriptionIt has recently been suggested that observed galaxy rotation curves can be accounted for by general relativity without recourse to dark-matter halos. Good fits have been produced to observed galatic rotation curves using this model. We show that the implied total mass is infinite, adding to the evidence opposing the hypothesis.
dc.description8 pages, 5 figures, submitted to Class. Quant. Grav
dc.identifierhttps://arxiv.org/abs/gr-qc/0604092
dc.identifierhttp://arxiv.org/abs/gr-qc/0604092
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/111148
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleGeneral Relativistic Galaxy Rotation Curves: Implications for Dark Matter Distribution
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