The following web-adapted movie showcases
numerical computations of gravitomagnetic (Lense-Thirring)
precession of geometrically thin accretion disks.
The gravitomagnetic effect is treated to the lowest
post-Newtonian order. The physics of the accretion disk is
treated in the Newtonian approximation.
The radiation torque is treated in the Pringle approximation.
For all computations the black hole has a mass of two solar masses.
The horizon radius is at 2M (Schwarszchild coordinates), while the
inner edge of the disk is at 6M (the radius of the inner-most stable circular orbit).
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n = 3 LFGMR Mode Frequency Growth Rate Q ![]() Hi-Res Quicktime (33.6MB) Lo-Res Quicktime (6.9MB) MPEG (3.5MB) |
n = 12 LFGMR Mode Frequency = 0.03mHz Growth Rate = -0.2mHz Q = 0.15 ![]() Hi-Res Quicktime (53.0MB) Lo-Res Quicktime (16.1MB) MPEG (5.4MB) |
n = 50 LFGMR Mode Frequency = 0.3mHz Growth Rate = -5.0mHz Q = 0.06 ![]() Hi-Res Quicktime (62.7MB) Lo-Res Quicktime (20.9MB) MPEG (6.5MB) |
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m = 14 HFGM Mode Frequency = 16Hz Growth Rate = -7.1Hz Q = 2.3 ![]() Hi-Res Quicktime (38.5MB) Lo-Res Quicktime (6.9MB) MPEG (5.9MB) This view is similar to the final view of the n=50 LFGMR mode, except the m=14 HFGM mode is also present. |
m = 2 HFGM Mode Frequency = 27Hz Growth Rate = -1.8Hz Q = 15 ![]() Hi-Res Quicktime (7.4MB) Lo-Res Quicktime (2.0MB) MPEG (1.7MB) |
m = 1 HFGM Mode Frequency = 29Hz Growth Rate = -0.6mHz Q = 48 ![]() Hi-Res Quicktime (6.9MB) Lo-Res Quicktime (1.7MB) MPEG (1.7MB) |
last updated 5.18.99 by jmf
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