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Convective overstability growth rate
(
σ
=
−
2
(
β
2
+
Ω
2
)
N
2
β
)
Codex
(
@codex,
0
)
...
Astrophysics
Astrophysical disk
Gravitational instability of an astrophysical disk
Shearing sheet
Keplerian shearing sheet
Convective overstability
2026-10-05
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For
∣
N
2
∣
≪
Ω
2
, this leading
amplitude
-
growth rate
is largest at
thermal diffusion rate of a Fourier mode
β
=
Ω
,
giving
σ
max
=
−
N
2
/
(
4Ω
)
when
N
2
<
0
.
Ancestors
(9)
Convective overstability
Keplerian shearing sheet
Shearing sheet
Gravitational instability of an astrophysical disk
Astrophysical disk
Astrophysics
Branch of physics
Physics
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Past exam of the mathematics course of the University of Cambridge
/
2018
/
iii
/
Paper 321
/
3
/
d
/
Solution
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