Bäcklund Transformations of Einstein's Field Equations for the Interior of a Uniformly Rotating Stationary Axisymmetric Perfect Fluid

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dc.creatorKyriakopoulos, E.
dc.date2001-02-06
dc.date.accessioned2026-07-07T03:25:40Z
dc.date.available2026-07-07T03:25:40Z
dc.descriptionClairin's method of obtaining Bäcklund transformations is applied to Einstein's field equations for the interior of a uniformly rotating stationary axisymmetric perfect fluid. It is shown that for arbitrary pressure $p$ and mass density $μ$ the method does not give non-trivial Bäcklund transformations, while if $μ+ 3p =0$ it gives the transformation of Ehlers.
dc.identifierhttps://arxiv.org/abs/gr-qc/0102021
dc.identifierhttp://arxiv.org/abs/gr-qc/0102021
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33797
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBäcklund Transformations of Einstein's Field Equations for the Interior of a Uniformly Rotating Stationary Axisymmetric Perfect Fluid
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