Restrictions on relativistically rotating fluids
DOI10.1063/1.525131zbMath0469.76131OpenAlexW2062394815MaRDI QIDQ3923878
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Publication date: 1981
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://www.osti.gov/biblio/6613652
integral inequalitiesfinite maximum redshifthigh- redshift quasar modelKerr exteriorrelativistically rotating fluid with asymptotically flat exterior
Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)
Cites Work
- On fitting rotating bodies to exterior gravitational fields
- Generic instability of rotating relativistic stars
- General Relativistic Fluid Spheres
- Killing inequalities for relativistically rotating fluids
- Massive spheres in general relativity
- A Method for Generating New Solutions of Einstein's Equation. II
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