The Inner Boundary Condition for a Thin Disk Accreting Into a Black Hole

Details The Inner Boundary Condition for a Thin Disk Accreting Into a Black Hole The Inner Boundary Condition for a Thin Disk Accreting Into a Black Hole

2000-04-10

arxiv.org/abs/astro-ph/0004129v1

Astronomy and Astrophysics

Astrophysics

3 pages, latex, submitted on April 10, 2000 to The Astrophysical Journal Letters

Scientific paper

Contrary to some recent claims the `no torque inner boundary condition' as
applied at the marginally stable orbit is correct for geometrically thin disks
accreting into black holes.

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