Cylindrically Symmetric, Static, Perfect-Fluid Solutions of Einstein's Field Equations

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dc.creatorSharif, M.
dc.date2007-02-08
dc.date.accessioned2026-07-07T07:51:19Z
dc.date.available2026-07-07T07:51:19Z
dc.descriptionPerfect-fluid, static, cylindrically symmetric solutions of Einstein's field equations are obtained for the equations of state $ρ+3p=0$ and $ρ=p$. In the former case, the density and the pressure turn out to be constant while in the later case, they depend on the radial parameter $r$. Evan's solution corresponding to the equation of state $ρ=p$ is included in the solutions discussed here.
dc.description5 pages, LaTex
dc.identifierhttps://arxiv.org/abs/gr-qc/0702045
dc.identifierhttp://arxiv.org/abs/gr-qc/0702045
dc.identifierJ.Korean Phys.Soc. 37 (2000) 624-625
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/125468
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCylindrically Symmetric, Static, Perfect-Fluid Solutions of Einstein's Field Equations
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