The general relativistic geometry of the Navarro-Frenk-White model

Simple item page
dc.creatorMatos, Tonatiuh
dc.creatorNunez, Dario
dc.date2003-03-26
dc.date.accessioned2026-07-07T06:30:56Z
dc.date.available2026-07-07T06:30:56Z
dc.descriptionWe derive the space time geometry associated with the Navarro Frenk White dark matter galactic halo model. We discuss several properties of such a spacetime, with particular attention to the corresponding Newtonian limit, stressing the qualitative and quantitative nature of the differences between the relativistic and the Newtonian description. We also discuss on the characteristics of the possible stress energy tensors which could produce such a geometry, via the Einstein's equations.
dc.description5 pages and 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0303594
dc.identifierhttp://arxiv.org/abs/astro-ph/0303594
dc.identifierRev.Mex.Fis. 51 (2005) 71-75
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/98469
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe general relativistic geometry of the Navarro-Frenk-White model
dc.typetext

Files

Collections

arXiv