Computer Science
Scientific paper
Oct 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988icar...76..182a&link_type=abstract
Icarus (ISSN 0019-1035), vol. 76, Oct. 1988, p. 182-198.
Computer Science
29
Degrees Of Freedom, Many Body Problem, Planetary Rings, Rotating Disks, Spin Dynamics, Boltzmann Transport Equation, Grazing Incidence, Optical Thickness, Particle Size Distribution
Scientific paper
The present treatment of the thermal equilibria of differentially-rotating, axisymmetric disks consisting of identical, spin-possessing as well as translational DOF-possessing hard sphere particles characterizes these disks' dynamics by means of two novel parameters: (1) the tangential restitution coefficient, and (2) the dimensionless moment of inertia. It is established that rings composed of spinning particles can generally be thermally balanced within more restricted ranges of the optical depth, as well as at higher values of the normal restitution coefficient, than spinless rings. Mean spin is indefinite in the present framework of neglected finite particle-size effects.
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