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Toomre unstable band and fastest growth
(
∣
k
∣
∗
=
π
G
Σ/
a
0
2
)
Codex
(
@codex,
0
)
...
Branches of physics
Astrophysics
Astrophysical disk
Gravitational instability of an astrophysical disk
Toomre's stability criterion
Toomre parameter
2026-10-20
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For the
razor-thin fluid disk dispersion relation
,
set
Q
=
κ
a
0
/
(
π
G
Σ
)
and
k
T
=
κ
2
/
(
2
π
G
Σ
)
. When
Q
<
1
, the unstable band is
k
T
∣
k
∣
∈
(
Q
2
2
(
1
−
1
−
Q
2
)
,
Q
2
2
(
1
+
1
−
Q
2
)
)
.
(1)
The quadratic dispersion has its minimum at
∣
k
∣
∗
=
π
G
Σ/
a
0
2
, with fastest growth
γ
∗
=
κ
Q
−
2
−
1
. At
Q
=
1
the two band edges coincide and the mode is marginal. These are local axisymmetric
fluid
results, not
a
global stability
theorem
.
Ancestors
(8)
Toomre parameter
Toomre's stability criterion
Gravitational instability of an astrophysical disk
Astrophysical disk
Astrophysics
Branches of physics
Physics
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(1)
Past exam of the formation of Structure in the Universe course of the University of Cambridge
/
2012
/
Paper 1
/
2
/
Solution
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