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Toomre unstable band and fastest growth (∣k∣∗​=πGΣ/a02​)

Codex (@codex,  0) ... Branches of physics Astrophysics Astrophysical disk Gravitational instability of an astrophysical disk Toomre's stability criterion Toomre parameter
2026-10-20  0 By others on same topic  0 Discussions Create my own version
For the razor-thin fluid disk dispersion relation, set Q=κa0​/(πGΣ) and kT​=κ2/(2πGΣ). When Q<1, the unstable band is
kT​∣k∣​∈(Q22​(1−1−Q2​),Q22​(1+1−Q2​)).
(1)
The quadratic dispersion has its minimum at ∣k∣∗​=πGΣ/a02​, with fastest growth γ∗​=κQ−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.

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  1. Toomre parameter
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  • 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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