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Torus - Model
Marginal Torus - Model X3p
Model X3p is a marginal torus rotating in the prograde sense around a Kerr
black hole with a=0.5. The torus has an initial maximum density
of
at r=6.4 M. Figure 11(a) shows
that at mode saturation the disk remains largely unperturbed, with an insignificant
fractional density decrease of 0.01. Figure 11(b)
shows a gray-scale enhanced view of the inner region near the static limit
clearly shows that a highly symmetric, weak inflow has developed. The growth
of the PPI modes is weak, with both modes tracking one another, as seen
in Figure 11(c). Although Table 3 would suggest
that these modes have a vigorous growth rate, their maximum amplitude is
comparable to that of model E3r, and the outcome is very similar to that
model, which is interesting since model X3p is much more closely related,
in terms of its structural parameters, to model E3p. The m=1 mode
reaches a very broad, weak maximum at
.
As with model E3r, a noticeable amount of inflow is present from the outset
as can be seen in Figure 11(d), which shows
the mass influx in the equatorial plane inside the inner edge of the torus.
As with E3r, this model is marginal, and the early onset of an inflow is
to be expected. In comparing panels (c) and (d), we see that the inflow
is established before any significant mode growth has occured; inflow levels
off to a more or less constant value in the first 4 orbits; the mode growth
also levels off in this period. As with model E3r, early accretion appears
to be an effective mechanism for inhibiting mode growth.
Figure 11: X3p Model. (a) (Top left) Equatorial slice through
torus at saturation. Density contours linearly spaced between
and 0.0. (b) (Bottom left) Magnified view of flow near static limit at
saturation ( x 10 density enhancement). The edge of the central black circle
is the static limit. (c) (Top right) Mode growth. (d) (Bottom right) Mass
influx at inner edge of disk. (Black hole rotates in counter-clockwise
sense.)
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Next:ConclusionsUp:ResultsPrevious:Marginal
Torus - Model
Jean-Pierre De Villiers
2002-06-05