A model of accretion disks with plasma wave-turbulence stress viscosity.

Details A model of accretion disks with plasma wave-turbulence stress viscosity. A model of accretion disks with plasma wave-turbulence stress viscosity.

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ppmto..13..174w&link_type=abstract

Publ. Purple Mt. Obs., Vol. 13, No. 2, p. 174 - 180

Computer Science

Accretion Disks: Models, Accretion Disks: Plasma Waves, Accretion Disks: Viscosity

Scientific paper

The viscosity has been a basic problem which is very important but hard to solve in the accretion disk theory. A model of accretion disks with plasma wave-turbulence stress viscosity can be established on the basis of the wave-flow coupling equations system. Here a specific case with stimulated Langmuir wave turbulence is presented and compared with the well-known standard α-viscous law model. The results show that the wave-turbulence stress as a viscous mechanism is more efficient as well as more plausible and self-consistent than the flow-turbulence stress in the α-models.

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