Robertson-Walker fluid sources endowed with rotation characterised by quadratic terms in angular velocity parameter

DOI10.1023/A:1024582618096zbMath1026.83072arXivgr-qc/0302046OpenAlexW3105740253MaRDI QIDQ1404018

P. H. Messenger, Ronald J. Wiltshire

Publication date: 20 August 2003

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0302046

zbMATH Keywords

cosmologydustrotational perturbations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Cites Work

• Slowly, rotating non-stationary, fluid solutions of Einstein's equations and their match to Kerr empty space-time
• General relativistic Rossby–Haurwitz waves of a slowly and differentially rotating fluid shell
• Perturbations of spacetime: gauge transformations and gauge invariance at second order and beyond
• The Wahlquist metric cannot describe an isolated rotating body

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