Stationary axisymmetric exteriors for perturbations of isolated bodies in general relativity, to second order

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dc.creatorMacCallum, Malcolm A. H.
dc.creatorMars, Marc
dc.creatorVera, Raül
dc.date2006-09-27
dc.date2006-12-04
dc.date.accessioned2026-07-07T10:24:31Z
dc.date.available2026-07-07T10:24:31Z
dc.descriptionPerturbed stationary axisymmetric isolated bodies, e.g. stars, represented by a matter-filled interior and an asymptotically flat vacuum exterior joined at a surface where the Darmois matching conditions are satisfied, are considered. The initial state is assumed to be static. The perturbations of the matching conditions are derived and used as boundary conditions for the perturbed Ernst equations in the exterior region. The perturbations are calculated to second order. The boundary conditions are overdetermined: necessary and sufficient conditions for their compatibility are derived. The special case of perturbations of spherical bodies is given in detail.
dc.descriptionRevTeX; 32 pp. Accepted by Phys. Rev. D. Added references and extra comments in introduction
dc.identifierhttps://arxiv.org/abs/gr-qc/0609127
dc.identifierhttp://arxiv.org/abs/gr-qc/0609127
dc.identifierPhys.Rev.D75:024017,2007
dc.identifierdoi:10.1103/PhysRevD.75.024017
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176217
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleStationary axisymmetric exteriors for perturbations of isolated bodies in general relativity, to second order
dc.typetext

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