Stationary Axisymmetric Solutions of the Einstein Equations with Rigidly Rotating Perfect Fluid and Nonlinear Charged Sources

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dc.creatorSalazar, Humberto
dc.creatorCordero, Ruben
dc.date1999-07-22
dc.date.accessioned2026-07-25T17:22:08Z
dc.descriptionA class of stationary rigidly rotating perfect fluid coupled with non-linear electromagnetic fields was investigated. An exact solution of the Einstein equations with sources for the Carter B(+) branch was found, for the equation of state $3p + ε= constant$. We use a structural function for the Born-Infeld non-linear electrodynamics which is invariant under duality rotations and a metric possessing a four- parameter group of motions. The solution is of Petrov type D and the eigenvectors of the electromagnetic field are aligned to the Debever-Penrose vectors.
dc.descriptionLatex file, 14 pages. Already published
dc.identifierhttps://arxiv.org/abs/gr-qc/9907069
dc.identifierhttp://arxiv.org/abs/gr-qc/9907069
dc.identifierInt.J.Theor.Phys. 35 (1996) 1259
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/47773
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleStationary Axisymmetric Solutions of the Einstein Equations with Rigidly Rotating Perfect Fluid and Nonlinear Charged Sources
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