Observer frame rotation rates and magnetic fields in spatially homogeneous universes

DOI10.1063/1.524743zbMath0492.76126OpenAlexW2087337583MaRDI QIDQ3955107

A. J. Fennelly

Publication date: 1981

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.524743

zbMATH Keywords

vorticityapproximate solution of Einstein's equationsBianchi I cosmologiesobserver frame rotation ratesprecession of shear tensor's principal axesspatially homogeneous universes

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Equations of motion in general relativity and gravitational theory (83C10) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

• Tilted homogeneous cosmological models
• A class of homogeneous cosmological models
• An Approach to Gravitational Radiation by a Method of Spin Coefficients

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