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- W2057029652 abstract "It was proved in the previous work that there must be a maximal possible accretion rate $$ dot M_{max} $$ for a slim disk. Here we discuss how the value of $$ dot M_{max} $$ depends on the two fundamental parameters of the disk, namely the mass of the central black hole M and the viscosity parameter α. It is shown that $$ dot M_{max} $$ increases with decreasing α, but is almost independent of M if $$ dot M_{max} $$ is measured by the Eddington accretion rate $$ dot M_{Edd} $$ , which is in turn proportional to M." @default.
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- W2057029652 date "2009-12-01" @default.
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- W2057029652 title "Maximal possible accretion rates for slim disks" @default.
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- W2057029652 doi "https://doi.org/10.1007/s11433-009-0236-5" @default.
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