Viscosity and Langmuir wave-turbulence stress in unmagnetized accretion disks.

Details Viscosity and Langmuir wave-turbulence stress in unmagnetized accretion disks. Viscosity and Langmuir wave-turbulence stress in unmagnetized accretion disks.

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998acasn..39....1w&link_type=abstract

Acta Astron. Sin., Vol. 39, No. 1, p. 1 - 7

Astronomy and Astrophysics

Astronomy

1

Accretion Disks: Plasma, Accretion Disks: Cataclysmic Binaries, Accretion Disks: Active Galactic Nuclei, Accretion Disks: X-Ray Stars

Scientific paper

A model of unmagnetized accretion disks in which the viscosity originates from the Langmuir wave-turbulence stress is presented, and is compared with the standard α accretion disk model. The results show that the present wave-turbulence seems to be a more efficient viscosity mechanism for unmagnetized accretion disks than the flow-turbulence in the contex of the α model.

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