Symmetries of asymptotically flat axisymmetric spacetimes with null dust

dc.creatorvon der Goenna, U.
dc.creatorPravdova, A.
dc.date2000-02-18
dc.date.accessioned2026-07-07T03:24:46Z
dc.date.available2026-07-07T03:24:46Z
dc.descriptionSymmetries of spacetimes with null dust field as a source compatible with asymptotic flatness are studied by using the Bondi-Sachs-van der Burg formalism. It is shown that in an axially symmetric spacetime with null dust field in which at least locally a smooth null infinity in the sense of Penrose exists, the only allowable additional Killing vector forming with the axial one a two-dimensional Lie algebra (the axial and the additional Killing vector are not assumed to be hypersurface orthogonal) is a supertranslational Killing vector and the gravitational field is then non-radiative (the Weyl tensor has a non-radiative character).
dc.description8 pages, RevTeX, accepted for publication in J. Math. Phys
dc.identifierhttps://arxiv.org/abs/gr-qc/0002064
dc.identifierhttp://arxiv.org/abs/gr-qc/0002064
dc.identifierJ.Math.Phys. 41 (2000) 3035-3044
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33461
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSymmetries of asymptotically flat axisymmetric spacetimes with null dust
dc.typetext

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