Viscosity and mass transport in nonuniform Keplerian disks

Details Viscosity and mass transport in nonuniform Keplerian disks Viscosity and mass transport in nonuniform Keplerian disks

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990icar...88..146o&link_type=abstract

Icarus (ISSN 0019-1035), vol. 88, Nov. 1990, p. 146-171.

Computer Science

3

Accretion Disks, Kepler Laws, Krook Equation, Mass Transfer, Dynamic Characteristics, Optical Thickness, Steady State, Viscosity

Scientific paper

A quantitative formalism for Keplerian particulate disk dynamics having its basis in a heuristic description of viscous transport is presently applied to the case of a ring with optical thickness radial gradient. A steady-state velocity distribution solution directly yields both the radial mass transport and the viscosity. The analytical method employed involves the solution of a novel form of the Krook equation through the separation of the phase-space collisional-products distribution into a symmetrical component and a delta function-approachable remainder. While this model is simplified for the case treated, its general approach may be extended to less artificially restricted cases.

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