Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...416..291r&link_type=abstract
Astrophysical Journal v.416, p.291
Astronomy and Astrophysics
Astronomy
5
Celestial Mechanics, Stellar Dynamics, Stars: Rotation
Scientific paper
The Riemann ellipsoidal model of self-gravitating systems assumes that the velocity field is linear. The symplectic model eliminates this restrictive ansatz while still retaining much of the simplicity of the original Riemann model. The kinetic energy of a Riemann ellipsoid is its linear velocity field value; the kinetic energy in the symplectic model is the exact expression. The Riemann hydrodynamic equations form a Hamiltonian dynamical system on co-adjoint orbits of a 15-dimensional Lie subgroup GCM(3) of the noncompact symplectic group Sp(3R). A symplectic model phase space is a co-adjoint orbit of the more general 21-dimensional group Sp(3,R). The Hamiltonian dynamics of self-gravitating symplectic systems is derived and proved to form a Lax system. But a symplectic system is not proved in this article to be a particular solution to the perfect fluid equations. A self-gravitating symplectic system approximates the dynamics of rotating stars and galaxies if the macroscopic symplectic degrees of freedom are adiabatically decoupled from the intrinsic individual particle degrees of freedom.
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