Lagrangian invariants in the equilibrium conditions of an ideal rotating fluid

DOI10.1007/BF00644226zbMath0727.76130MaRDI QIDQ804445

O. V. Kravtsov

Publication date: 1991

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

variational methodequilibrium conditionsvelocity distributioncompressible fluidhomogeneous fluidan ideal fluidfluid with a magnetic fieldfreezing-in vector fieldsideal fluid in the past- Newtonian approximation of general relativityRiemann's resultsscalar potentialsself-gravitating configurations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) General theory of rotating fluids (76U05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Cites Work

• Unnamed Item
• Unnamed Item
• Unnamed Item
• On the stability of viscous fluid motions
• On the equilibrium figures of an ideal rotating liquid in the post- Newtonian approximation of general relativity. I: Equilibrium conditions
• ON HYDROMAGNETIC EQUILIBRIUM
• Vector-potential hamiltonian formulation of the general retativistic perfect fluid

This page was built for publication: Lagrangian invariants in the equilibrium conditions of an ideal rotating fluid