Maximal Possible Accretion Rates for Slim Disks

Details Maximal Possible Accretion Rates for Slim Disks Maximal Possible Accretion Rates for Slim Disks

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..968..405g&link_type=abstract

ASTROPHYSICS OF COMPACT OBJECTS: International Conference on Astrophysics of Compact Objects. AIP Conference Proceedings, Volum

Astronomy and Astrophysics

Astrophysics

Accretion And Accretion Disks, Black Holes, Hydrodynamics

Scientific paper

By adopting the correct vertical gravitational force in studies of
thermal equilibrium solutions, we find that there exists a maximal
possible accretion rate for each radius in the outer region of optically
thick accretion flows, such that only the inner regions of these flows
can possibly take the form of slim disks.

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