An approximate global solution to the gravitational field of a perfect fluid in slow rotation

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dc.creatorCabezas, J. A.
dc.creatorRuiz, E.
dc.date2006-11-20
dc.date.accessioned2026-07-07T07:31:56Z
dc.date.available2026-07-07T07:31:56Z
dc.descriptionUsing the Post-Minkowskian formalism and considering rotation as a perturbation, we compute an approximate interior solution for a stationary perfect fluid with constant density and axial symmetry. A suitable change of coordinates allows this metric to be matched to the exterior metric to a particle with a pole-dipole-quadrupole structure, relating the parameters of both.
dc.description11 pages, english version
dc.identifierhttps://arxiv.org/abs/gr-qc/0611099
dc.identifierhttp://arxiv.org/abs/gr-qc/0611099
dc.identifierActas de los ERE 1987, Publicaciones del IAC, Serie C, No. 6, 1988, 215-230
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118936
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAn approximate global solution to the gravitational field of a perfect fluid in slow rotation
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