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Minimum Toomre parameter in an exponential flat-rotation disk (Q(x)=Q0​ex−1/x)

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 Ω=Ω0​r0​/r, surface density Σ=Σ0​e1−r/r0​ and constant sound speed a0​, the Toomre parameter is Q(x)=Q0​ex−1/x, where x=r/r0​ and Q0​=2​Ω0​a0​/(πGΣ0​). Its logarithmic derivative is 1−1/x, so the minimum is Q0​ at r0​. The formal inner and outer limits both diverge; if Q0​<1, local axisymmetric instability occupies a bounded intermediate annulus. A central departure from the assumed flat rotation law can change the inner conclusion.

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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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