On the stress-energy tensor of a rotating wormhole

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dc.creatorBergliaffa, S. E. Perez
dc.creatorHibberd, K. E.
dc.date2000-06-12
dc.date2000-07-26
dc.date.accessioned2026-07-07T03:25:03Z
dc.date.available2026-07-07T03:25:03Z
dc.descriptionWe analyze the stress-energy tensor necessary to generate a general stationary and axisymmetric spacetime. The constraints on the geometry arising from considering a perfect fluid as a source are derived. For a fluid with a nonzero stress tensor, we obtain two necessary conditions on the metric. As an example, we show that the rotating wormhole presented in the literature can not be described by either a perfect fluid or by a fluid with anisotropic stresses.
dc.description4 pages, LaTex. Revised version, with several changes
dc.identifierhttps://arxiv.org/abs/gr-qc/0006041
dc.identifierhttp://arxiv.org/abs/gr-qc/0006041
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33569
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn the stress-energy tensor of a rotating wormhole
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