Central behavior of rotating fluids
Copyright policy )Central behavior of rotating fluids
With a tetrad formalism, the leading terms near the center of a stationary rotating star are determined from Newtonian analogy and Einstein's equations. These are expanded to second order in the radius and it is shown that they are inconsistent with the metric being Petrov typeD.
- University of Windsor Canada
Quantum hydrodynamics and relativistic hydrodynamics, stationary, General theory of rotating fluids, Einstein's equations (general structure, canonical formalism, Cauchy problems), Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.), tetrad formalism
Quantum hydrodynamics and relativistic hydrodynamics, stationary, General theory of rotating fluids, Einstein's equations (general structure, canonical formalism, Cauchy problems), Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.), tetrad formalism
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