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On the stress-energy tensor of a rotating wormhole

2000/06/12 by Santiago Esteban Perez Bergliaffa, S. E. Perez Bergliaffa, Bergliaffa, S. E. Perez +3 · 2 citations
Engineering · Environmental Science · Physics and Astronomy · #FOS: Physical sciences #Fluid Dynamics and Vibration Analysis #General Relativity and Quantum Cosmology (gr-qc) #Geotechnical and Geomechanical Engineering #Methane Hydrates and Related Phenomena #gr-qc

paper · pdf · doi:10.48550/arxiv.gr-qc/0006041

4 pages, LaTex. Revised version, with several changes

openalex publication_date 2000/06/12 · arxiv created 2000/07/26 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We 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.

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